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            type="text/xsl"?><rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#"><channel rdf:about="http://onlinelibrary.wiley.com/rss/journal/10.1002/(ISSN)1099-1034" xmlns="http://purl.org/rss/1.0/"><title>Geological Journal</title><description> Wiley Online Library : Geological Journal</description><link>http://dx.doi.org/10.1002%2F%28ISSN%291099-1034</link><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc</dc:publisher><dc:language xmlns:dc="http://purl.org/dc/elements/1.1/">en</dc:language><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/">© John Wiley &amp; Sons, Ltd.</dc:rights><prism:issn xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">0072-1050</prism:issn><prism:eIssn xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1099-1034</prism:eIssn><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-01-01T00:00:00-05:00</dc:date><prism:coverDisplayDate xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">January/February 2012</prism:coverDisplayDate><prism:volume xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">47</prism:volume><prism:number xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1</prism:number><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">110</prism:endingPage><image rdf:resource="http://onlinelibrary.wiley.com/store/10.1002/gj.v47.1/asset/cover.gif?v=1&amp;s=e9d555e6a31d61074afa40bcbaccef6908abc1fb"/><items><rdf:Seq><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.2415"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1350"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1339"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1343"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1344"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1345"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1334"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1330"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1327"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1342"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1333"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1337"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1338"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1341"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1340"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1328"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1332"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1321"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1322"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1323"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1312"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1320"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1314"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1316"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1311"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1313"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1315"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1309"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1308"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1307"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1305"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1302"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1300"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1297"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1324"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1329"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1331"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1336"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1335"/><rdf:li rdf:resource="http://dx.doi.org/10.1002%2Fgj.1346"/></rdf:Seq></items></channel><item rdf:about="http://dx.doi.org/10.1002%2Fgj.2415" xmlns="http://purl.org/rss/1.0/"><title>Archaeocyaths from South America: review and a new record</title><link>http://dx.doi.org/10.1002%2Fgj.2415</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Archaeocyaths from South America: review and a new record</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">P. D. González</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">M. F. Tortello</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">S. E. Damborenea</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">M. Naipauer</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">A. M. Sato</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">R. Varela</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-02-07T06:27:18.312337-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.2415</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.2415</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.2415</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Special Issue Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>In South America, autochthonous archaeocyathan faunas preserved in Early Cambrian limestones have not been found yet. Nevertheless, a few well-documented occurrences of these fossils in clasts contained in coarse-grained rocks of a wide age range have been discovered in recent years. Erratic limestone blocks from the Late Carboniferous–Early Permian Fitzroy Tillite Formation in the Falkland/Malvinas Islands yielded three archaeocyath taxa. Also, seven taxa were reported from archaeocyathan limestone clasts in a metaconglomerate of the Cambro-Ordovician El Jagüelito Formation in northern Patagonia. In addition, a new record from the Late Carboniferous–Early Permian Sauce Grande Formation diamictites in Sierras Australes, Buenos Aires Province, Argentina, is presented herein. Preservation of this scarce new material is poor, but at least three different taxa can be distinguished. The most likely source of all archaeocyathan limestone clasts found in southern South America is the Shackleton Limestone from the Transantarctic Mountains in East Antarctica. The new record from the Sauce Grande Formation and the inferred clast provenance reinforce the correlation between this unit, the Dwyka Tillite (South Africa) and the Fitzroy Tillite Formation (Falklands/Malvinas), suggesting a very wide distribution of these Antarctic occurrences during the Late Carboniferous–Early Permian Gondwana glaciation (Episode III). Thus, even though being allochthonous, archaeocyaths are emerging as a new key biological feature for Gondwana palaeogeographic reconstructions. Copyright © 2012 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>In South America, autochthonous archaeocyathan faunas preserved in Early Cambrian limestones have not been found yet. Nevertheless, a few well-documented occurrences of these fossils in clasts contained in coarse-grained rocks of a wide age range have been discovered in recent years. Erratic limestone blocks from the Late Carboniferous–Early Permian Fitzroy Tillite Formation in the Falkland/Malvinas Islands yielded three archaeocyath taxa. Also, seven taxa were reported from archaeocyathan limestone clasts in a metaconglomerate of the Cambro-Ordovician El Jagüelito Formation in northern Patagonia. In addition, a new record from the Late Carboniferous–Early Permian Sauce Grande Formation diamictites in Sierras Australes, Buenos Aires Province, Argentina, is presented herein. Preservation of this scarce new material is poor, but at least three different taxa can be distinguished. The most likely source of all archaeocyathan limestone clasts found in southern South America is the Shackleton Limestone from the Transantarctic Mountains in East Antarctica. The new record from the Sauce Grande Formation and the inferred clast provenance reinforce the correlation between this unit, the Dwyka Tillite (South Africa) and the Fitzroy Tillite Formation (Falklands/Malvinas), suggesting a very wide distribution of these Antarctic occurrences during the Late Carboniferous–Early Permian Gondwana glaciation (Episode III). Thus, even though being allochthonous, archaeocyaths are emerging as a new key biological feature for Gondwana palaeogeographic reconstructions. Copyright © 2012 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1350" xmlns="http://purl.org/rss/1.0/"><title>Structure and U–Pb zircon geochronology in the Variscan foreland of SW Sardinia, Italy</title><link>http://dx.doi.org/10.1002%2Fgj.1350</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Structure and U–Pb zircon geochronology in the Variscan foreland of SW Sardinia, Italy</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">P. Pavanetto</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">A. Funedda</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">C. J. Northrup</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">M. Schmitz</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">J. Crowley</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">A. Loi</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-02-07T06:27:05.870871-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1350</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1350</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1350</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Research Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>New field mapping, U–Pb zircon geochronology and structural analysis of the southernmost Sardinia metamorphic basement, considered a branch of the Variscan foreland, indicate that it is, in part, allochthonous and was structurally emplaced within the foreland area, rather than being older depositional basement beneath the foreland succession. The Bithia Formation, classically considered part of the ‘Southern Sulcis metamorphic Complex’ (and here termed the Bithia tectonic unit, or BTU), is a greenschist facies metamorphic unit commonly interpreted as Precambrian in age. New geochronology of felsic volcanic rocks in the BTU, however, yield a U–Pb zircon age of 457.01 ± 0.17 Ma (Upper Ordovician). Thus, the depositional age of the unit is younger than the weakly metamorphosed Lower Cambrian rocks of the adjacent foreland succession. New detailed mapping and analysis of the field relationships between the BTU and foreland succession indicates that their contact is a mylonitic shear zone. The metamorphic character, general lithology, and deformational history of the BTU are similar to those of units in the Variscan Nappe Zone located northeast of the foreland area. We reinterpret the BTU as a synformal klippe of material related tectonically to the Variscan Nappe Zone. We infer that it was thrust over and became infolded into the foreland during late stages of the Variscan contractional deformation. Copyright © 2012 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>New field mapping, U–Pb zircon geochronology and structural analysis of the southernmost Sardinia metamorphic basement, considered a branch of the Variscan foreland, indicate that it is, in part, allochthonous and was structurally emplaced within the foreland area, rather than being older depositional basement beneath the foreland succession. The Bithia Formation, classically considered part of the ‘Southern Sulcis metamorphic Complex’ (and here termed the Bithia tectonic unit, or BTU), is a greenschist facies metamorphic unit commonly interpreted as Precambrian in age. New geochronology of felsic volcanic rocks in the BTU, however, yield a U–Pb zircon age of 457.01 ± 0.17 Ma (Upper Ordovician). Thus, the depositional age of the unit is younger than the weakly metamorphosed Lower Cambrian rocks of the adjacent foreland succession. New detailed mapping and analysis of the field relationships between the BTU and foreland succession indicates that their contact is a mylonitic shear zone. The metamorphic character, general lithology, and deformational history of the BTU are similar to those of units in the Variscan Nappe Zone located northeast of the foreland area. We reinterpret the BTU as a synformal klippe of material related tectonically to the Variscan Nappe Zone. We infer that it was thrust over and became infolded into the foreland during late stages of the Variscan contractional deformation. Copyright © 2012 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1339" xmlns="http://purl.org/rss/1.0/"><title>Geochemical processes and sedimentological characteristics of Holocene lagoon deposits, Alikes Lagoon, Zakynthos Island, western Greece</title><link>http://dx.doi.org/10.1002%2Fgj.1339</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Geochemical processes and sedimentological characteristics of Holocene lagoon deposits, Alikes Lagoon, Zakynthos Island, western Greece</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">D. Panagiotaras</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">D. Papoulis</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">N. Kontopoulos</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">P. Avramidis</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-01-16T10:49:45.264964-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1339</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1339</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1339</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Research Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>In this paper we present sedimentological, geochemical, mineralogical and <sup>14</sup>C Accelerator Mass Spectrometry (AMS) dating data of a 21.0-m core obtained from Alikes Lagoon, Zakynthos Island. It is the first time that sedimentological and geochemical data are presented, up to 21-m depth, from an Holocene coastal lagoon environment of the Ionia Sea, western Greece. The sedimentological properties and the geochemical composition of sediments were studied for the time period between 8540 years <span class="smallCaps">bp</span> to present. Samples were analysed for their particle size, calcium carbonate and total organic carbon (TOC) content. Moreover, bulk sample chemical analyses for major and trace elements were carried out, as well as bulk, oriented mineralogical analyses for the clay fraction (&lt;2 µm) were determined by powder X-Ray diffraction. The grain size characteristics, statistical parameters and TOC, for the Holocene analysed samples, suggest a coastal environment (restricted-shallow) with reduced salinity such as a tidal flat and/or particularly marsh in a lagoon margin. Sediment characteristics as well as trace element records may contain additional new palaeoclimate information that provide important new constraint on sediment depositional environment and Holocene climate. Stratigraphic variation of geochemical indices, such as Rb/Ti, Cs/Ti, Eu/Eu*, Th/Ti, La/Ti, Ta/Ti, Yb/Ti and Y/Ti, for the sediments with ages from 8540 to 7210 years <span class="smallCaps">bp</span>, remain relatively constant indicating that the provenance of the Alikes Lagoon remained similar throughout the mid Holocene. However, geochemical indices in sediments with ages from 7110 years <span class="smallCaps">bp</span> to present, indicate the transition from a warm and wet climate in the middle Holocene to a relatively cold climatic conditions in modern times. Copyright © 2012 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>In this paper we present sedimentological, geochemical, mineralogical and 14C Accelerator Mass Spectrometry (AMS) dating data of a 21.0-m core obtained from Alikes Lagoon, Zakynthos Island. It is the first time that sedimentological and geochemical data are presented, up to 21-m depth, from an Holocene coastal lagoon environment of the Ionia Sea, western Greece. The sedimentological properties and the geochemical composition of sediments were studied for the time period between 8540 years bp to present. Samples were analysed for their particle size, calcium carbonate and total organic carbon (TOC) content. Moreover, bulk sample chemical analyses for major and trace elements were carried out, as well as bulk, oriented mineralogical analyses for the clay fraction (&lt;2 µm) were determined by powder X-Ray diffraction. The grain size characteristics, statistical parameters and TOC, for the Holocene analysed samples, suggest a coastal environment (restricted-shallow) with reduced salinity such as a tidal flat and/or particularly marsh in a lagoon margin. Sediment characteristics as well as trace element records may contain additional new palaeoclimate information that provide important new constraint on sediment depositional environment and Holocene climate. Stratigraphic variation of geochemical indices, such as Rb/Ti, Cs/Ti, Eu/Eu*, Th/Ti, La/Ti, Ta/Ti, Yb/Ti and Y/Ti, for the sediments with ages from 8540 to 7210 years bp, remain relatively constant indicating that the provenance of the Alikes Lagoon remained similar throughout the mid Holocene. However, geochemical indices in sediments with ages from 7110 years bp to present, indicate the transition from a warm and wet climate in the middle Holocene to a relatively cold climatic conditions in modern times. Copyright © 2012 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1343" xmlns="http://purl.org/rss/1.0/"><title>Phylogenetic analysis of the late Cambrian–early Ordovician genus Parabolinella Brøgger (Trilobita, Olenidae)</title><link>http://dx.doi.org/10.1002%2Fgj.1343</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Phylogenetic analysis of the late Cambrian–early Ordovician genus Parabolinella Brøgger (Trilobita, Olenidae)</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">DANIELA S. MONTI</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">VIVIANA A. CONFALONIERI</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-01-16T05:09:58.491585-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1343</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1343</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1343</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Special Issue Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>Phylogenetic relationships among species of the family Olenidae (Trilobita, Ptychopariida) were traditionally established by the direct comparison of morphological features and the evaluation of stratigraphic placement. In this study, a cladistic analysis of <em>Parabolinella</em> Brøgger is conducted in order to test the supposed monophyly of the genus and to determine the relationships of its species. Twenty-one taxa (sixteen of this genus) from the late Cambrian and Tremadocian of Baltica, Avalonia, Laurentia, South China and the western margin of Gondwana were revised. Forty non-ordered characters were considered in the analysis, 34 belonging to the cephalon, four to the pygidium, and two to the thorax. Some of these characters were specially defined for this study. The phylogenetic analysis was performed under unweighted parsimony. The obtained tree is partially consistent with the stratigraphic record of the studied species and shows correspondence with global late Cambrian and early Ordovician palaeogeography. <em>Parabolinella</em> may have originated in deep water sites of the Oaxaca region, Mexico and then migrated to other regions. The genus diversified in outer shelf facies of the Baltica Province during the late Cambrian and Tremadocian, whereas it would have dispersed to the South China Province in early Tremadocian times. Copyright © 2012 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>Phylogenetic relationships among species of the family Olenidae (Trilobita, Ptychopariida) were traditionally established by the direct comparison of morphological features and the evaluation of stratigraphic placement. In this study, a cladistic analysis of Parabolinella Brøgger is conducted in order to test the supposed monophyly of the genus and to determine the relationships of its species. Twenty-one taxa (sixteen of this genus) from the late Cambrian and Tremadocian of Baltica, Avalonia, Laurentia, South China and the western margin of Gondwana were revised. Forty non-ordered characters were considered in the analysis, 34 belonging to the cephalon, four to the pygidium, and two to the thorax. Some of these characters were specially defined for this study. The phylogenetic analysis was performed under unweighted parsimony. The obtained tree is partially consistent with the stratigraphic record of the studied species and shows correspondence with global late Cambrian and early Ordovician palaeogeography. Parabolinella may have originated in deep water sites of the Oaxaca region, Mexico and then migrated to other regions. The genus diversified in outer shelf facies of the Baltica Province during the late Cambrian and Tremadocian, whereas it would have dispersed to the South China Province in early Tremadocian times. Copyright © 2012 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1344" xmlns="http://purl.org/rss/1.0/"><title>Systematic, morphometric and palaeobiogeographic study of Blainia gregaria Walcott, 1916 (Trilobita, Ptychopariida), Middle Cambrian of the Precordillera of western Argentina</title><link>http://dx.doi.org/10.1002%2Fgj.1344</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Systematic, morphometric and palaeobiogeographic study of Blainia gregaria Walcott, 1916 (Trilobita, Ptychopariida), Middle Cambrian of the Precordillera of western Argentina</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Osvaldo L. Bordonaro</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Brian R. Pratt</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Virginia Robledo</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-01-13T13:46:59.837951-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1344</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1344</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1344</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Special Issue Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>The ptychoparioid trilobite <em>Blainia gregaria</em> Walcott, 1916 is described for the first time from the late middle Cambrian (Series 3) of the Argentine Precordillera. It occurs commonly in the upper part of La Laja Formation, a carbonate platform succession that crops out in the Precordillera Oriental of San Juan where it reaches a thickness of some 600 m. Sections were sampled on cerro Tres Marías in Sierra de Marquesado and in quebrada de Zonda at the northern termination of Sierra Chica de Zonda. More than 1200 specimens were recovered from 22 stratigraphic levels over a thickness of 155 m, located in the uppermost 15 m of the Soldano Member, the approximately 100 m thick Rivadavia Member, and in the lower 40 m of the Juan Pobre Member. Our biometric study dealt with 205 cranidia and 365 pygidia from cerro Tres Marías. Measured dimensions of a subset of this collection provide bivariate datasets that in some characters show broad scatter plots and relatively low linear correlation coefficients, indicative of rather wide intraspecific morphological variation. Six morphotypes (three cranidial and three pygidial), recognized mainly on the basis of shape, occur together in the same collections. This evidence for an unusually high degree of variability leads to a proposed synonymy of some 30 previously named species in North America belonging to two genera, <em>Blainia</em> Walcott, 1916 and <em>Glyphaspis</em> Poulsen, 1927, the latter considered a junior synonym. The biogeographic distribution of <em>B. gregaria</em>, as redefined here, shows that it was an endemic Laurentian species that inhabited the inner parts of the carbonate platform that rimmed the craton and mantled portions of its interior. Its presence in western Argentina is further evidence for the very close faunal relationship between the Precordilleran terrane, known as Cuyania, and Laurentia during the Cambrian. Copyright © 2012 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>The ptychoparioid trilobite Blainia gregaria Walcott, 1916 is described for the first time from the late middle Cambrian (Series 3) of the Argentine Precordillera. It occurs commonly in the upper part of La Laja Formation, a carbonate platform succession that crops out in the Precordillera Oriental of San Juan where it reaches a thickness of some 600 m. Sections were sampled on cerro Tres Marías in Sierra de Marquesado and in quebrada de Zonda at the northern termination of Sierra Chica de Zonda. More than 1200 specimens were recovered from 22 stratigraphic levels over a thickness of 155 m, located in the uppermost 15 m of the Soldano Member, the approximately 100 m thick Rivadavia Member, and in the lower 40 m of the Juan Pobre Member. Our biometric study dealt with 205 cranidia and 365 pygidia from cerro Tres Marías. Measured dimensions of a subset of this collection provide bivariate datasets that in some characters show broad scatter plots and relatively low linear correlation coefficients, indicative of rather wide intraspecific morphological variation. Six morphotypes (three cranidial and three pygidial), recognized mainly on the basis of shape, occur together in the same collections. This evidence for an unusually high degree of variability leads to a proposed synonymy of some 30 previously named species in North America belonging to two genera, Blainia Walcott, 1916 and Glyphaspis Poulsen, 1927, the latter considered a junior synonym. The biogeographic distribution of B. gregaria, as redefined here, shows that it was an endemic Laurentian species that inhabited the inner parts of the carbonate platform that rimmed the craton and mantled portions of its interior. Its presence in western Argentina is further evidence for the very close faunal relationship between the Precordilleran terrane, known as Cuyania, and Laurentia during the Cambrian. Copyright © 2012 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1345" xmlns="http://purl.org/rss/1.0/"><title>The origin and maturation of lagoonal glauconites: a case study from the Oligocene Maniyara Fort Formation, western Kutch, India</title><link>http://dx.doi.org/10.1002%2Fgj.1345</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">The origin and maturation of lagoonal glauconites: a case study from the Oligocene Maniyara Fort Formation, western Kutch, India</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Santanu Banerjee</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Shovan Lal Chattoraj</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">P. K. Saraswati</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Somnath Dasgupta</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Urbashi Sarkar</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Adam Bumby</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-12-07T00:44:57.491517-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1345</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1345</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1345</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Research Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>An integrated study of the sedimentology, micropalaeontology, mineralogy and geochemistry of glauconites in the Oligocene Maniyara Fort Formation (western Kutch, India), has been undertaken. Authigenic glauconites, mostly of evolved type, formed within a back-barrier lagoonal environment. Foraminifera help constrain the biostratigraphy and along with sedimentological evidence, provide information on the depositional conditions. Glauconite in the Maniyara Fort Formation occurs either as infillings within intra-particle pores of larger foraminifers, or as an altered form of faecal pellets. X-ray diffraction studies reveal the less mature nature of glauconite infillings compared to the glauconite pellets. Electron microprobe investigation confirms a relative enrichment of K<sub>2</sub>O and total Fe<sub>2</sub>O<sub>3</sub> in the latter. Both varieties of glauconite formed by initial authigenic precipitation of K-poor glauconite and subsequently matured by addition of potassium in the interlayer sites and fixation of total iron in the octahedral sites; calcium, magnesium and aluminum were released from the glauconite structure concomitantly. Alkaline conditions during the entire process of glauconite formation did not allow dissolution of foraminiferal tests. Mineralogical and chemical characteristics of the Maniyara Fort Formation glauconites are more similar to deep marine glauconites than those reported from other shallow or marginal marine settings. A low negative cerium anomaly, as well as abundant pyrite, suggests formation of glauconite in sub-oxic micro-environments, created by decay of organic matter associated with foraminiferal chambers and faecal pellets. Sub-oxic condition apparently prevailed relatively longer within the Maniyara Fort Formation lagoons. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>An integrated study of the sedimentology, micropalaeontology, mineralogy and geochemistry of glauconites in the Oligocene Maniyara Fort Formation (western Kutch, India), has been undertaken. Authigenic glauconites, mostly of evolved type, formed within a back-barrier lagoonal environment. Foraminifera help constrain the biostratigraphy and along with sedimentological evidence, provide information on the depositional conditions. Glauconite in the Maniyara Fort Formation occurs either as infillings within intra-particle pores of larger foraminifers, or as an altered form of faecal pellets. X-ray diffraction studies reveal the less mature nature of glauconite infillings compared to the glauconite pellets. Electron microprobe investigation confirms a relative enrichment of K2O and total Fe2O3 in the latter. Both varieties of glauconite formed by initial authigenic precipitation of K-poor glauconite and subsequently matured by addition of potassium in the interlayer sites and fixation of total iron in the octahedral sites; calcium, magnesium and aluminum were released from the glauconite structure concomitantly. Alkaline conditions during the entire process of glauconite formation did not allow dissolution of foraminiferal tests. Mineralogical and chemical characteristics of the Maniyara Fort Formation glauconites are more similar to deep marine glauconites than those reported from other shallow or marginal marine settings. A low negative cerium anomaly, as well as abundant pyrite, suggests formation of glauconite in sub-oxic micro-environments, created by decay of organic matter associated with foraminiferal chambers and faecal pellets. Sub-oxic condition apparently prevailed relatively longer within the Maniyara Fort Formation lagoons. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1334" xmlns="http://purl.org/rss/1.0/"><title>Discovery of Silurian sponge spicules from the Argentine Precordillera</title><link>http://dx.doi.org/10.1002%2Fgj.1334</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Discovery of Silurian sponge spicules from the Argentine Precordillera</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">M. S. Beresi</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-12-06T23:34:38.565436-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1334</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1334</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1334</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Special Issue Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>An association of silicified spicules of hexactinellid sponges was collected from Silurian sandstones at the top of the La Chilca Formation, cropping out at Cerro del Fuerte, 20 km east of Jáchal, in the San Juan Precordillera of west-central Argentina. This is the first occurrence of a Silurian spicule fauna recorded at higher palaeolatitudes from Argentina and the entire South American part of Gondwana. The spicules were extracted by means of formic acid treatment from sandstones of the uppermost part of the La Chilca Formation, which ranges in age from the late Hirnantian to Llandovery, based on graptolites, brachiopods and conodonts. The spicule association is composed only of scarce siliceous hexactine-based spicules which cannot be attributed to any specific hexactinellid taxon. The fragmentary preservation of this allochthonous sponge assemblage points toward preburial transport. These spicules represent the only microfauna found in the uppermost sandstones. Macrofossils are absent. No conodonts have been recovered in these levels. Two interpretations on the spicules of the Precordillera can be argued: (a) that those early Silurian hexactinellids could have occurred in quartz sandstones of the shore-facies to off-shore transitional associations, in the upper La Chilca Formation, or (b) that these sponges flourished in mainly calcareous shales in quiet deep-water conditions, and that their fragile spicules were removed and deposited by oceanic currents, on the top of the outer-shelf sand bars.</p></div><div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Both hypotheses on the palaeoenvironmental origin of these spicules are substantially different, but the scarcity of spicules does not allow a more precise interpretation. The discovery of these hexactinellid spicules provides a new perspective on Silurian sponge occurrence and distribution for the Argentine Precordillera. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>An association of silicified spicules of hexactinellid sponges was collected from Silurian sandstones at the top of the La Chilca Formation, cropping out at Cerro del Fuerte, 20 km east of Jáchal, in the San Juan Precordillera of west-central Argentina. This is the first occurrence of a Silurian spicule fauna recorded at higher palaeolatitudes from Argentina and the entire South American part of Gondwana. The spicules were extracted by means of formic acid treatment from sandstones of the uppermost part of the La Chilca Formation, which ranges in age from the late Hirnantian to Llandovery, based on graptolites, brachiopods and conodonts. The spicule association is composed only of scarce siliceous hexactine-based spicules which cannot be attributed to any specific hexactinellid taxon. The fragmentary preservation of this allochthonous sponge assemblage points toward preburial transport. These spicules represent the only microfauna found in the uppermost sandstones. Macrofossils are absent. No conodonts have been recovered in these levels. Two interpretations on the spicules of the Precordillera can be argued: (a) that those early Silurian hexactinellids could have occurred in quartz sandstones of the shore-facies to off-shore transitional associations, in the upper La Chilca Formation, or (b) that these sponges flourished in mainly calcareous shales in quiet deep-water conditions, and that their fragile spicules were removed and deposited by oceanic currents, on the top of the outer-shelf sand bars.Both hypotheses on the palaeoenvironmental origin of these spicules are substantially different, but the scarcity of spicules does not allow a more precise interpretation. The discovery of these hexactinellid spicules provides a new perspective on Silurian sponge occurrence and distribution for the Argentine Precordillera. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1330" xmlns="http://purl.org/rss/1.0/"><title>Proposal of a reference section and point for the Cambrian Series 2–3 boundary in the Mediterranean subprovince in Murero (NE Spain) and its intercontinental correlation</title><link>http://dx.doi.org/10.1002%2Fgj.1330</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Proposal of a reference section and point for the Cambrian Series 2–3 boundary in the Mediterranean subprovince in Murero (NE Spain) and its intercontinental correlation</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Rodolfo Gozalo</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">María Eugenia Dies Álvarez</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">José Antonio Gámez Vintaned</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Andrey Yu. Zhuravlev</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Blanca Bauluz</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Ignacio Subías</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Juan B. Chirivella Martorell</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Eduardo Mayoral</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Hans-Jürgen Gursky</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">José Antonio Andrés</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Eladio Liñán</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-12-04T22:40:49.226486-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1330</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1330</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1330</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Special Issue Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>The classical lower-middle Cambrian boundary is approximately equivalent with the boundary of the Cambrian Series 2 and 3, which is now in the process of definition by the International Subcommission on Cambrian Stratigraphy. Currently, there are two oryctocephalid trilobite species first appearance data (FAD) that are suggested as possible markers of this level: <em>Ovatoryctocara granulata</em> Tchernysheva, 1962 and <em>Oryctocephalus indicus</em> (Reed, 1910), respectively. Until now neither of these two species has been recorded in the Mediterranean subprovince or Baltica. As a result, in these regions a level potentially correlating with either the FAD of <em>Ovatoryctocara granulata</em> or <em>Oryctocephalus indicus</em> has to be located using the available bio-, isotope-, and event-stratigraphy data.</p></div><div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Carbon isotope signatures reveal global oceanic perturbations adjacent to the Cambrian Series 2 and Series 3 (former lower-middle Cambrian) boundary. This event, first called the Valdemiedes Event (it was defined in Murero, NE Spain; Liñán <em>et al.</em>, 1993a), caused a noticeable extinction of trilobites, mostly olenellids and protolenids (which were replaced in some regions by paradoxidids), as well as an almost complete extermination of some other early Cambrian marine animals. Both isotope and palaeontological evidence show that the disappearance of olenellids in Laurentia, protolenids in Siberia and the appearance of the first <em>Acadoparadoxides</em> in Western Gondwana, Baltica, Avalonia, and Siberia, which was formerly thought to be a series of diachronous regional perturbations, were nearly contemporaneous events. Features of a global ecological crisis and faunal replacement being taken together with a pronounced global δ<sup>13</sup>C<sub>org</sub> negative excursion would serve as the best indicator of the lower boundary of the Cambrian Series 3 and Stage 5 in the Mediterranean subprovince and is correlatable with the <em>Ovatoryctocara granulata</em> FAD. Another δ<sup>13</sup>C<sub>org</sub> negative excursion followed by a positive shift occurs at a slightly younger level, which coincides with a transgression maximum and roughly is coeval with the <em>Oryctocephalus indicus</em> FAD, also proposed as a possible base of the Cambrian Series 3. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>The classical lower-middle Cambrian boundary is approximately equivalent with the boundary of the Cambrian Series 2 and 3, which is now in the process of definition by the International Subcommission on Cambrian Stratigraphy. Currently, there are two oryctocephalid trilobite species first appearance data (FAD) that are suggested as possible markers of this level: Ovatoryctocara granulata Tchernysheva, 1962 and Oryctocephalus indicus (Reed, 1910), respectively. Until now neither of these two species has been recorded in the Mediterranean subprovince or Baltica. As a result, in these regions a level potentially correlating with either the FAD of Ovatoryctocara granulata or Oryctocephalus indicus has to be located using the available bio-, isotope-, and event-stratigraphy data.Carbon isotope signatures reveal global oceanic perturbations adjacent to the Cambrian Series 2 and Series 3 (former lower-middle Cambrian) boundary. This event, first called the Valdemiedes Event (it was defined in Murero, NE Spain; Liñán et al., 1993a), caused a noticeable extinction of trilobites, mostly olenellids and protolenids (which were replaced in some regions by paradoxidids), as well as an almost complete extermination of some other early Cambrian marine animals. Both isotope and palaeontological evidence show that the disappearance of olenellids in Laurentia, protolenids in Siberia and the appearance of the first Acadoparadoxides in Western Gondwana, Baltica, Avalonia, and Siberia, which was formerly thought to be a series of diachronous regional perturbations, were nearly contemporaneous events. Features of a global ecological crisis and faunal replacement being taken together with a pronounced global δ13Corg negative excursion would serve as the best indicator of the lower boundary of the Cambrian Series 3 and Stage 5 in the Mediterranean subprovince and is correlatable with the Ovatoryctocara granulata FAD. Another δ13Corg negative excursion followed by a positive shift occurs at a slightly younger level, which coincides with a transgression maximum and roughly is coeval with the Oryctocephalus indicus FAD, also proposed as a possible base of the Cambrian Series 3. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1327" xmlns="http://purl.org/rss/1.0/"><title>Silurian to Early Devonian organic-walled phytoplankton and miospores from Argentina: biostratigraphy and diversity trends</title><link>http://dx.doi.org/10.1002%2Fgj.1327</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Silurian to Early Devonian organic-walled phytoplankton and miospores from Argentina: biostratigraphy and diversity trends</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Claudia V. Rubinstein</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Victoria J. García Muro</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-11-14T23:53:31.352272-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1327</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1327</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1327</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Special Issue Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>The distribution and diversity of marine palynomorphs, such as acritarchs and chlorophytes, and terrestrial palynomorphs, such as miospores, are controlled mainly by palaeoenvironmental and palaeogeographical conditions. Recently, global patterns of organic-walled phytoplankton were illustrated for the Late Silurian to earliest Devonian based on data from different stratigraphic sections and palaeocontinents. Here, we analyze the Silurian and the Early Devonian diversity in the Argentinean Precordillera, Central Andean, and Chacoparanense basins. The evolution of the diversity is evaluated in a well-constrained biostratigraphic framework, bearing in mind local palaeoenvironmental conditions and changes within each basin. Taking into account recently published and unpublished data from well-dated sections, the biodiversity of Silurian phytoplankton seemingly increases upwards, reaching its maximum peak during the Ludlovian. However, palynomorphs are rarely recorded in Wenlockian strata, and the supposed Pridolian layers are not confidently well constrained. The first record of trilete spores in Argentina is Ludlovian, approximately 30 million years after their first appearance in the Late Ordovician. Palynomorph diversity increases in the Early Devonian, with a higher diversity of miospores than that of the marine phytoplankton. We interpret possible discrepancies in biodiversity trends of organic-walled phytoplankton between Argentina and other regions, as related to the quantitatively and qualitatively disparity of data, as well as the lack of rigorous biostratigraphic and palaeoenvironmental assessments of the Argentinean basins. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>The distribution and diversity of marine palynomorphs, such as acritarchs and chlorophytes, and terrestrial palynomorphs, such as miospores, are controlled mainly by palaeoenvironmental and palaeogeographical conditions. Recently, global patterns of organic-walled phytoplankton were illustrated for the Late Silurian to earliest Devonian based on data from different stratigraphic sections and palaeocontinents. Here, we analyze the Silurian and the Early Devonian diversity in the Argentinean Precordillera, Central Andean, and Chacoparanense basins. The evolution of the diversity is evaluated in a well-constrained biostratigraphic framework, bearing in mind local palaeoenvironmental conditions and changes within each basin. Taking into account recently published and unpublished data from well-dated sections, the biodiversity of Silurian phytoplankton seemingly increases upwards, reaching its maximum peak during the Ludlovian. However, palynomorphs are rarely recorded in Wenlockian strata, and the supposed Pridolian layers are not confidently well constrained. The first record of trilete spores in Argentina is Ludlovian, approximately 30 million years after their first appearance in the Late Ordovician. Palynomorph diversity increases in the Early Devonian, with a higher diversity of miospores than that of the marine phytoplankton. We interpret possible discrepancies in biodiversity trends of organic-walled phytoplankton between Argentina and other regions, as related to the quantitatively and qualitatively disparity of data, as well as the lack of rigorous biostratigraphic and palaeoenvironmental assessments of the Argentinean basins. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1342" xmlns="http://purl.org/rss/1.0/"><title>Engineering geology for tomorrow's cities, edited by M.G. Culshaw, H.J. Reeves, I. Jefferson and T.W. Spink. Geological Society Engineering Geology Special Publication, 22, London, 2009. No. of pages: 303. Price: £95.00. ISBN 978-1-86239-290-8 (hardback).</title><link>http://dx.doi.org/10.1002%2Fgj.1342</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Engineering geology for tomorrow's cities, edited by M.G. Culshaw, H.J. Reeves, I. Jefferson and T.W. Spink. Geological Society Engineering Geology Special Publication, 22, London, 2009. No. of pages: 303. Price: £95.00. ISBN 978-1-86239-290-8 (hardback).</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Will Hughes</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-10-25T06:38:15.614932-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1342</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1342</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1342</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Book review</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[]]></content:encoded><description/></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1333" xmlns="http://purl.org/rss/1.0/"><title>Tectonic framework of southern Bastar Craton, Central India: a study based on different spatial information data sets</title><link>http://dx.doi.org/10.1002%2Fgj.1333</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Tectonic framework of southern Bastar Craton, Central India: a study based on different spatial information data sets</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">T. Yellappa</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">T. R. K. CHETTY</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">M. Santosh</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-10-12T05:50:58.503443-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1333</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1333</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1333</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Special Issue Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>We present here a regional tectonic fabric analysis of the southern margin of the Bastar Craton, Central India, obtained from different spatial data sets that include Shuttle Radar Topographic Mission (SRTM), Landsat ETM<sup>+</sup> (Enhanced Thematic Mapper) and IRS (Indian Remote sensing Satellite) P6-LISS3, integrated with available geological information, as well as field and microscopic observations. The southern margin of the Bastar Craton exhibits large-scale structures, such as regional-scale folds, major shear zones and associated tectonic fabric affected by strong brittle–ductile deformation. The deformational features are related to large-scale thrusting, regional compression, and episodic igneous activity during the Precambrian, and display a major tectonic control on magmatism and the evolution of a shear zone system. The NW–SE to E–W and NE–SW trending brittle to ductile shear zones traversing the craton display both dextral as well as sinistral displacements. Well-developed kinematic indicators include, sheared quartz veins, tension gashes, rotated porphyroblasts, S–C fabrics, pinch-and-swell structures, sigmoidal foliations and riedel fractures that are well preserved in the basement Sukma–Bengpal supracrustals, as well as in the younger granitoids of the Dongargarh Supergroup. Large-scale well-developed NW–SE trending isoclinal folding in the basement gneisses and major folding in mafic intrusions in the south-western margin and tight, upright doubly-plunging large-scale folds in the eastern margins of the craton represent two major tectonic events. These events can be correlated to large-scale thrusts and suggest an initial N–S compression of the craton followed by E–W thrusting at different intervals during the tectonic evolution of the craton. The occurrence of several NW–SE trending mafic dykes parallel to the shear zones indicate that regional-scale tensile stresses were operating during the Proterozoic, associated with a possible continental rift environment in the centre of the craton. The structural pattern obtained, together with the structures mapped with the coherence of remote sensing images, give significant information and an opportunity to reconstruct the timing, style of deformation and its kinematics in the southern part of the Bastar Craton and provide important constraints on the kinematics of the shear zone system and evolution of the craton. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>We present here a regional tectonic fabric analysis of the southern margin of the Bastar Craton, Central India, obtained from different spatial data sets that include Shuttle Radar Topographic Mission (SRTM), Landsat ETM+ (Enhanced Thematic Mapper) and IRS (Indian Remote sensing Satellite) P6-LISS3, integrated with available geological information, as well as field and microscopic observations. The southern margin of the Bastar Craton exhibits large-scale structures, such as regional-scale folds, major shear zones and associated tectonic fabric affected by strong brittle–ductile deformation. The deformational features are related to large-scale thrusting, regional compression, and episodic igneous activity during the Precambrian, and display a major tectonic control on magmatism and the evolution of a shear zone system. The NW–SE to E–W and NE–SW trending brittle to ductile shear zones traversing the craton display both dextral as well as sinistral displacements. Well-developed kinematic indicators include, sheared quartz veins, tension gashes, rotated porphyroblasts, S–C fabrics, pinch-and-swell structures, sigmoidal foliations and riedel fractures that are well preserved in the basement Sukma–Bengpal supracrustals, as well as in the younger granitoids of the Dongargarh Supergroup. Large-scale well-developed NW–SE trending isoclinal folding in the basement gneisses and major folding in mafic intrusions in the south-western margin and tight, upright doubly-plunging large-scale folds in the eastern margins of the craton represent two major tectonic events. These events can be correlated to large-scale thrusts and suggest an initial N–S compression of the craton followed by E–W thrusting at different intervals during the tectonic evolution of the craton. The occurrence of several NW–SE trending mafic dykes parallel to the shear zones indicate that regional-scale tensile stresses were operating during the Proterozoic, associated with a possible continental rift environment in the centre of the craton. The structural pattern obtained, together with the structures mapped with the coherence of remote sensing images, give significant information and an opportunity to reconstruct the timing, style of deformation and its kinematics in the southern part of the Bastar Craton and provide important constraints on the kinematics of the shear zone system and evolution of the craton. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1337" xmlns="http://purl.org/rss/1.0/"><title>A sea without fish: life in the ordovician sea of the cincinnatian region by David L. Meyer and Richard A. Davis. Indiana University Press, Bloomington, 2009. No. of pages: xv+346. Price: US$44.95. ISBN 978-0-253-35198-2 (hardback).</title><link>http://dx.doi.org/10.1002%2Fgj.1337</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">A sea without fish: life in the ordovician sea of the cincinnatian region by David L. Meyer and Richard A. Davis. Indiana University Press, Bloomington, 2009. No. of pages: xv+346. Price: US$44.95. ISBN 978-0-253-35198-2 (hardback).</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Stephen K. Donovan</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-10-12T05:49:34.467847-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1337</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1337</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1337</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Book Review</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[]]></content:encoded><description/></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1338" xmlns="http://purl.org/rss/1.0/"><title>The lie of the land: an under-the-field guide to the british isles by Ian Vince. Boxtree, London, 2010. No. of pages: xiv + 287. Price: UK£14-99. ISBN 978-0-7522-2711-5 (hardback).</title><link>http://dx.doi.org/10.1002%2Fgj.1338</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">The lie of the land: an under-the-field guide to the british isles by Ian Vince. Boxtree, London, 2010. No. of pages: xiv + 287. Price: UK£14-99. ISBN 978-0-7522-2711-5 (hardback).</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Stephen K. Donovan</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-10-12T05:49:18.961452-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1338</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1338</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1338</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Book Review</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[]]></content:encoded><description/></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1341" xmlns="http://purl.org/rss/1.0/"><title>Sedimentary rocks in the field: a practical guide (4th edition), by Maurice E. Tucker. Wiley-Blackwell, Chichester, 2011. No. of pages: xi + 275. Price: UK£22.50. ISBN 978-0-470-68916-5 (paperback)</title><link>http://dx.doi.org/10.1002%2Fgj.1341</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Sedimentary rocks in the field: a practical guide (4th edition), by Maurice E. Tucker. Wiley-Blackwell, Chichester, 2011. No. of pages: xi + 275. Price: UK£22.50. ISBN 978-0-470-68916-5 (paperback)</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Stephen K. Donovan</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-10-04T21:26:30.15648-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1341</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1341</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1341</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Book Review</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[]]></content:encoded><description/></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1340" xmlns="http://purl.org/rss/1.0/"><title>Norfolk's earth heritage - valuing our geodiversity, by Tim Holt-Wilson, design and layout by Su Waldron. Norfolk Geodiversity Partnership, Norwich, 2010. No. of pages: 74. Price: UK£12.00. ISBN 978-1-84754-216-8 (paperback).</title><link>http://dx.doi.org/10.1002%2Fgj.1340</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Norfolk's earth heritage - valuing our geodiversity, by Tim Holt-Wilson, design and layout by Su Waldron. Norfolk Geodiversity Partnership, Norwich, 2010. No. of pages: 74. Price: UK£12.00. ISBN 978-1-84754-216-8 (paperback).</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Stephen K. Donovan</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-10-04T21:23:32.853381-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1340</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1340</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1340</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Book Review</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[]]></content:encoded><description/></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1328" xmlns="http://purl.org/rss/1.0/"><title>Strain localization, granulite formation and geodynamic setting of ‘hot orogens’: a case study from the Eastern Ghats Province, India</title><link>http://dx.doi.org/10.1002%2Fgj.1328</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Strain localization, granulite formation and geodynamic setting of ‘hot orogens’: a case study from the Eastern Ghats Province, India</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Saibal Gupta</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-10-03T22:25:52.019294-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1328</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1328</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1328</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Special Issue Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>The Eastern Ghats Province underwent major orogenic events in the Neoproterozoic–Cambrian period: 980–930, 900–650 and 550–500 Ma. At each time interval, deformation occurred synchronous with high-grade metamorphism. The first event was characterized by distributed strain throughout the entire province, while strain and thermal anomalies during the later orogenies were confined to the province boundaries. In the first case, pre-orogenic rifting caused ultrahigh-temperature metamorphism at the base of the crust, and was closely followed by crustal shortening related to the collision of the granulite belt with the Indian craton. The thermal anomaly persisting from the rifting event, followed by the thermal relaxation associated with crustal shortening led to prolific melt production and transfer of heat producing elements (HPE) into the middle and upper parts of the thick post-collisional crust. Heating and associated melting caused rheological weakening of the crustal section, and explains why strain was distributed across the entire thermally perturbed zone. Erosion removed a substantial portion of the HPE-rich upper crust, and deposited the detritus in cratonic sedimentary basins to the west. Subsequently, the rheologically stronger Eastern Ghats Province crust could effectively transmit stresses and concentrate them along pre-existing zones of weakness near the province boundaries. Progressive thrusting in these domains led to consistent loading of the footwall, even as it underwent thermal relaxation. Since both strain and heating were associated with the footwall of pre-existing discontinuities, the ‘hot orogen’ so formed was also spatially restricted. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>The Eastern Ghats Province underwent major orogenic events in the Neoproterozoic–Cambrian period: 980–930, 900–650 and 550–500 Ma. At each time interval, deformation occurred synchronous with high-grade metamorphism. The first event was characterized by distributed strain throughout the entire province, while strain and thermal anomalies during the later orogenies were confined to the province boundaries. In the first case, pre-orogenic rifting caused ultrahigh-temperature metamorphism at the base of the crust, and was closely followed by crustal shortening related to the collision of the granulite belt with the Indian craton. The thermal anomaly persisting from the rifting event, followed by the thermal relaxation associated with crustal shortening led to prolific melt production and transfer of heat producing elements (HPE) into the middle and upper parts of the thick post-collisional crust. Heating and associated melting caused rheological weakening of the crustal section, and explains why strain was distributed across the entire thermally perturbed zone. Erosion removed a substantial portion of the HPE-rich upper crust, and deposited the detritus in cratonic sedimentary basins to the west. Subsequently, the rheologically stronger Eastern Ghats Province crust could effectively transmit stresses and concentrate them along pre-existing zones of weakness near the province boundaries. Progressive thrusting in these domains led to consistent loading of the footwall, even as it underwent thermal relaxation. Since both strain and heating were associated with the footwall of pre-existing discontinuities, the ‘hot orogen’ so formed was also spatially restricted. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1332" xmlns="http://purl.org/rss/1.0/"><title>Silurian-Devonian coral associations across a sequence stratigraphic boundary in the Argentine Precordillera</title><link>http://dx.doi.org/10.1002%2Fgj.1332</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Silurian-Devonian coral associations across a sequence stratigraphic boundary in the Argentine Precordillera</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Marcelo G. Carrera</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Ezequiel Montoya</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Juan J. Rustán</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Karen Halpern</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-09-27T23:46:49.646496-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1332</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1332</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1332</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Special Issue Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>Silurian and Devonian corals occur abundantly in siliciclastic rocks of the Argentine Precordillera. They are distributed along a Silurian storm-dominated shallow-water platform, a transitional restricted nearshore environment, and a Devonian muddy platform setting. Four main associations of rugose and tabulate corals have been recorded: a Silurian association, a lowermost Devonian and two associations in Lower Devonian rocks. The Silurian shallow-water platform coral association shows abundant colonies of a tabulate pleurodictyform coral. The type and the domical form of corals indicate high-energy environments. The lowermost Devonian coral association shows the abundance of the tabulate coral <em>Argentinella argentina</em>, which could have formed patches in protected low-energy environments. The Lower Devonian coral associations correspond to a muddy platform environment. The first one includes rugose and hemispherical tabulate corals and the second is composed of tabulate corals assigned to <em>Parastriatopora sanjuanina</em>, and <em>Parastriatopora</em> sp. They are long stick-like, fasciculate forms, grouped in apparently life position. Rugose and tabulate corals in the Upper Silurian and Lower Devonian of Argentina constitute low-diversity associations of western Gondwana, developed in mid- to high-latitudes. The morphologies acquired by corals are related to water energy. Laminar or encrusting forms were more competitive in the Silurian shallow-water, high-energy environments. Slender branching forms with a high profile typically inhabited Devonian relatively deeper water or protected settings. The stratigraphic distribution observed partially followed the well- known pattern in which shallow-water faunas disappeared during regressive events and are replaced by new forms in the subsequent transgressive sequence. The turnover pattern detected across the Silurian-Devonian transitional interval is in agreement with that previously recognized on the basis of the accompanying fauna. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>Silurian and Devonian corals occur abundantly in siliciclastic rocks of the Argentine Precordillera. They are distributed along a Silurian storm-dominated shallow-water platform, a transitional restricted nearshore environment, and a Devonian muddy platform setting. Four main associations of rugose and tabulate corals have been recorded: a Silurian association, a lowermost Devonian and two associations in Lower Devonian rocks. The Silurian shallow-water platform coral association shows abundant colonies of a tabulate pleurodictyform coral. The type and the domical form of corals indicate high-energy environments. The lowermost Devonian coral association shows the abundance of the tabulate coral Argentinella argentina, which could have formed patches in protected low-energy environments. The Lower Devonian coral associations correspond to a muddy platform environment. The first one includes rugose and hemispherical tabulate corals and the second is composed of tabulate corals assigned to Parastriatopora sanjuanina, and Parastriatopora sp. They are long stick-like, fasciculate forms, grouped in apparently life position. Rugose and tabulate corals in the Upper Silurian and Lower Devonian of Argentina constitute low-diversity associations of western Gondwana, developed in mid- to high-latitudes. The morphologies acquired by corals are related to water energy. Laminar or encrusting forms were more competitive in the Silurian shallow-water, high-energy environments. Slender branching forms with a high profile typically inhabited Devonian relatively deeper water or protected settings. The stratigraphic distribution observed partially followed the well- known pattern in which shallow-water faunas disappeared during regressive events and are replaced by new forms in the subsequent transgressive sequence. The turnover pattern detected across the Silurian-Devonian transitional interval is in agreement with that previously recognized on the basis of the accompanying fauna. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1321" xmlns="http://purl.org/rss/1.0/"><title>Introduction to coastal processes and geomorphology by Robin Davidson-Arnott. Cambridge University Press, Cambridge, 2010. No. of pages: xiii+442 pp. Price: £29-99. ISBN 978-0-521-69671-5 (paperback).</title><link>http://dx.doi.org/10.1002%2Fgj.1321</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Introduction to coastal processes and geomorphology by Robin Davidson-Arnott. Cambridge University Press, Cambridge, 2010. No. of pages: xiii+442 pp. Price: £29-99. ISBN 978-0-521-69671-5 (paperback).</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Jelmer Cleveringa</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-09-13T09:58:36.294608-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1321</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1321</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1321</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Book Review</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[]]></content:encoded><description/></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1322" xmlns="http://purl.org/rss/1.0/"><title>Our magnetic earth, the science of geomagnetism by R. T. Merrill. University of Chicago Press, Chicago, 2007. No. of pages: xxi + 329. Price: US$25-00. ISBN 978-0-226-51960-9 (hardback).</title><link>http://dx.doi.org/10.1002%2Fgj.1322</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Our magnetic earth, the science of geomagnetism by R. T. Merrill. University of Chicago Press, Chicago, 2007. No. of pages: xxi + 329. Price: US$25-00. ISBN 978-0-226-51960-9 (hardback).</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">C.F. Winkler Prins</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-09-07T03:44:39.238566-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1322</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1322</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1322</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Book Review</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[]]></content:encoded><description/></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1323" xmlns="http://purl.org/rss/1.0/"><title>Fossils from the lower lias of the Dorset coast, edited by Alan R. Lord and Paul G. Davis. The Palaeontological Association, field guide to fossils 13, London, 2010. No. of pages: 436. Price: £18-00. ISBN 978-1-4443-3774-7 (softback)</title><link>http://dx.doi.org/10.1002%2Fgj.1323</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Fossils from the lower lias of the Dorset coast, edited by Alan R. Lord and Paul G. Davis. The Palaeontological Association, field guide to fossils 13, London, 2010. No. of pages: 436. Price: £18-00. ISBN 978-1-4443-3774-7 (softback)</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">David A.T. Harper</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-09-07T03:44:31.530868-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1323</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1323</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1323</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Book Review</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[]]></content:encoded><description/></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1312" xmlns="http://purl.org/rss/1.0/"><title>Geochemical characterization and petrogenesis of Proterozoic Khairagarh volcanics: implication for Precambrian crustal evolution</title><link>http://dx.doi.org/10.1002%2Fgj.1312</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Geochemical characterization and petrogenesis of Proterozoic Khairagarh volcanics: implication for Precambrian crustal evolution</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Kabita C. Longjam</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Talat Ahmad</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-08-05T03:32:54.70952-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1312</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1312</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1312</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Special Issue Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>The Khairagarh volcano-sedimentary sequence is exposed along the Kotri–Dongargarh Belt towards the north-eastern part of the Bastar Craton. This sequence is exposed south of the Central Indian Shear (CIS) and east of the Sakoli Group rocks. The Khairagarh volcanic sequence is represented by low-Ti, intermediate-Ti and high-Ti basalt–basaltic andesite series that probably represent varying degrees of partial melting of an enriched mantle source, thus they appear to be consanguineous. These rocks are associated with a sequence of high magnesium andesitic (HMA) rocks that follow a separate evolutionary trend, thus they appear not to be related to the basalt–basaltic andesite sequence. The presence of the two contrasting sequences probably indicates generation in a hot Andean-type subduction zone for the HMA, and Andean-type back-arc rifting for the basalt–basaltic andesite samples. The possibility of a relatively thick crust around 3.6 Ga in the Bastar Craton and the Amgaon Gneissic Complex, basement for the Khairagarh–Sakoli sequence, probably indicates that it was part of the Supercontinent Ur. The mantle extraction age of about 2.9 to 2.5 Ga, based on the Nd-model ages for the Khairagarh–Sakoli sequence, probably indicate that this part of the Central Indian Shield became part of the Supercontinent Columbia subsequently. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>The Khairagarh volcano-sedimentary sequence is exposed along the Kotri–Dongargarh Belt towards the north-eastern part of the Bastar Craton. This sequence is exposed south of the Central Indian Shear (CIS) and east of the Sakoli Group rocks. The Khairagarh volcanic sequence is represented by low-Ti, intermediate-Ti and high-Ti basalt–basaltic andesite series that probably represent varying degrees of partial melting of an enriched mantle source, thus they appear to be consanguineous. These rocks are associated with a sequence of high magnesium andesitic (HMA) rocks that follow a separate evolutionary trend, thus they appear not to be related to the basalt–basaltic andesite sequence. The presence of the two contrasting sequences probably indicates generation in a hot Andean-type subduction zone for the HMA, and Andean-type back-arc rifting for the basalt–basaltic andesite samples. The possibility of a relatively thick crust around 3.6 Ga in the Bastar Craton and the Amgaon Gneissic Complex, basement for the Khairagarh–Sakoli sequence, probably indicates that it was part of the Supercontinent Ur. The mantle extraction age of about 2.9 to 2.5 Ga, based on the Nd-model ages for the Khairagarh–Sakoli sequence, probably indicate that this part of the Central Indian Shield became part of the Supercontinent Columbia subsequently. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1320" xmlns="http://purl.org/rss/1.0/"><title>Igneous rocks and processes: A practical guide, by Robin Gill. Wiley-Blackwell, Chichester, 2010. No. of pages: ix+428. Price: UK£ 34.95. ISBN 978-0-6320-6377-2 (paperback).</title><link>http://dx.doi.org/10.1002%2Fgj.1320</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Igneous rocks and processes: A practical guide, by Robin Gill. Wiley-Blackwell, Chichester, 2010. No. of pages: ix+428. Price: UK£ 34.95. ISBN 978-0-6320-6377-2 (paperback).</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Trevor A. Jackson</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-07-28T21:53:01.383526-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1320</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1320</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1320</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Book Review</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[]]></content:encoded><description/></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1314" xmlns="http://purl.org/rss/1.0/"><title>A 3.51 Ga bimodal volcanics-BIF-ultramafic succession from Singhbhum Craton: implications for Palaeoarchaean geodynamic processes from the oldest greenstone succession of the Indian subcontinent</title><link>http://dx.doi.org/10.1002%2Fgj.1314</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">A 3.51 Ga bimodal volcanics-BIF-ultramafic succession from Singhbhum Craton: implications for Palaeoarchaean geodynamic processes from the oldest greenstone succession of the Indian subcontinent</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Joydip Mukhopadhyay</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Gautam Ghosh</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Udo Zimmermann</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Susmita Guha</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Titir Mukherjee</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-07-27T05:32:00.493166-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1314</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1314</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1314</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Special Issue Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>The Palaeoarchaean greenstone belt of the southern Iron Ore Group (SIOG) (3.51 Ga) in the Singhbhum Craton, eastern India, includes low-strained and low-greenstone grade bimodal volcanics, Banded Iron Formation (BIF) and chromiferous ultramafics as enclaves within tonalite–trondjhemite–granodiorite (TTG) granitoids, collectively referred to as the Singhbhum Granite (3.4 Ga to 3.1 Ga). The succession comprises, from base to top, a lower unit of massive and pillowed basalt conformably overlain by dacitic lava and pyroclastics which in turn is overlain by a major BIF unit. The ultramafics are juxtaposed with the volcanics-BIF succession along a thrust fault. The lithological association of pillow lava, subaqueous dacitic lava and pyroclastic rocks and BIF collectively, suggests that the entire succession was deposited in a deep-marine depositional setting. The ash-poor dacitic volcanic rock succession with evidences of a transition from suppressed-volatile deep-water lava flow and pyroclastics to more evolved mass-flow deposits with increasing trend of subaqueous flow transformation, records a transition from a deep-water low-height volcanic chain to a shallower subaqueous eruption in an aggradational volcanic chain. Geochemical proxies from the bimodal volcanics and ultramafics showing enrichment of La/Nb, Th/Nb, Th/La, Ba/La, Pb/Ce, depletion in Nb–Ta relative to neighbouring REE, together with tectonic discrimination criteria using Nb, Y, Zr, Ti compositions, suggest an extending oceanic arc–forearc geodynamic setting similar to many of the Phanerozoic supra-subduction zone ophiolites where ophiolite development in the extending upper plate in a relatively short time span is facilitated by slab rollback processes. The positive Eu-anomaly together with high Y/Ho values from the BIFs also suggests their deposition in close proximity to spreading centres that might have developed over a rifted arc. The bimodal volcanic rock-BIF-ultramafic succession of the SIOG with evidence of a convergent margin geodynamic setting is an important example for Palaeoarchaean plate tectonic processes operating on Earth. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>The Palaeoarchaean greenstone belt of the southern Iron Ore Group (SIOG) (3.51 Ga) in the Singhbhum Craton, eastern India, includes low-strained and low-greenstone grade bimodal volcanics, Banded Iron Formation (BIF) and chromiferous ultramafics as enclaves within tonalite–trondjhemite–granodiorite (TTG) granitoids, collectively referred to as the Singhbhum Granite (3.4 Ga to 3.1 Ga). The succession comprises, from base to top, a lower unit of massive and pillowed basalt conformably overlain by dacitic lava and pyroclastics which in turn is overlain by a major BIF unit. The ultramafics are juxtaposed with the volcanics-BIF succession along a thrust fault. The lithological association of pillow lava, subaqueous dacitic lava and pyroclastic rocks and BIF collectively, suggests that the entire succession was deposited in a deep-marine depositional setting. The ash-poor dacitic volcanic rock succession with evidences of a transition from suppressed-volatile deep-water lava flow and pyroclastics to more evolved mass-flow deposits with increasing trend of subaqueous flow transformation, records a transition from a deep-water low-height volcanic chain to a shallower subaqueous eruption in an aggradational volcanic chain. Geochemical proxies from the bimodal volcanics and ultramafics showing enrichment of La/Nb, Th/Nb, Th/La, Ba/La, Pb/Ce, depletion in Nb–Ta relative to neighbouring REE, together with tectonic discrimination criteria using Nb, Y, Zr, Ti compositions, suggest an extending oceanic arc–forearc geodynamic setting similar to many of the Phanerozoic supra-subduction zone ophiolites where ophiolite development in the extending upper plate in a relatively short time span is facilitated by slab rollback processes. The positive Eu-anomaly together with high Y/Ho values from the BIFs also suggests their deposition in close proximity to spreading centres that might have developed over a rifted arc. The bimodal volcanic rock-BIF-ultramafic succession of the SIOG with evidence of a convergent margin geodynamic setting is an important example for Palaeoarchaean plate tectonic processes operating on Earth. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1316" xmlns="http://purl.org/rss/1.0/"><title>Textural developments in chromite deforming under eclogite-facies conditions from the Neoarchaean Sittampundi anorthosite complex, southern India</title><link>http://dx.doi.org/10.1002%2Fgj.1316</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Textural developments in chromite deforming under eclogite-facies conditions from the Neoarchaean Sittampundi anorthosite complex, southern India</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Biswajit Ghosh</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Ritam Konar</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-07-21T01:05:34.413846-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1316</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1316</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1316</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Special Issue Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>We describe the textural evolution of chromites from the Neoarchaean Sittampundi anorthosite complex in southern India. A series of micro-structural developments in chromites with increasing temperature is recorded. The intracrystalline deformation started with a high strain rate at elevated temperature. At higher temperature, crystal plastic deformation like recovery/recrystallization was initiated developing subgrains in chromites. Diffusion processes played a major role during deformation as documented from grain boundary geometry of chromites with adjacent silicates, distribution of silicate inclusions in the host chromites as well as in the new grains, and the development of sector Al–Cr zoning. At the highest temperatures, diffusion might have overstepped the recovery. After deformation stopped, static recrystallization by grain boundary area reduction resulted in grain growth. A high-strain steady-state, heterogeneous deformation, as evidenced from the chromite micro-structures is suggested for the Sittampundi chromites. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>We describe the textural evolution of chromites from the Neoarchaean Sittampundi anorthosite complex in southern India. A series of micro-structural developments in chromites with increasing temperature is recorded. The intracrystalline deformation started with a high strain rate at elevated temperature. At higher temperature, crystal plastic deformation like recovery/recrystallization was initiated developing subgrains in chromites. Diffusion processes played a major role during deformation as documented from grain boundary geometry of chromites with adjacent silicates, distribution of silicate inclusions in the host chromites as well as in the new grains, and the development of sector Al–Cr zoning. At the highest temperatures, diffusion might have overstepped the recovery. After deformation stopped, static recrystallization by grain boundary area reduction resulted in grain growth. A high-strain steady-state, heterogeneous deformation, as evidenced from the chromite micro-structures is suggested for the Sittampundi chromites. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1311" xmlns="http://purl.org/rss/1.0/"><title>Archaean granulite facies metamorphism at the Singhbhum Craton–Eastern Ghats Mobile Belt interface: implication for the Ur supercontinent assembly</title><link>http://dx.doi.org/10.1002%2Fgj.1311</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Archaean granulite facies metamorphism at the Singhbhum Craton–Eastern Ghats Mobile Belt interface: implication for the Ur supercontinent assembly</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">S. N. Mahapatro</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">N. C. Pant</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">S. K. Bhowmik</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">A. K. Tripathy</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">J. K. Nanda</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-07-04T22:51:14.34251-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1311</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1311</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1311</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Special Issue Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>In this study, we investigate the geological significance and the antiquity of lower crustal granulite facies metamorphism from the Rengali Domain, which lies in between the Singhbhum Craton in the north and the Eastern Ghats Mobile Belt in the south. Petrographic, mineral compositional, metamorphic reaction history and geothermobarometric studies of two representative metapelite granulite samples reveal widespread biotite melting at peak granulite facies metamorphic conditions of 7.8 ± 0.13 kbar, 849 ± 31 °C and subsequent melt extraction, producing a mixture of residual granulites and melts in the Rengali Province. Depending on local bulk rock compositional variations, biotite melting produced peak metamorphic assemblages of garnet + cordierite in the more aluminous compositional domain, while garnet + orthopyroxene + cordierite resulted in domains of intermediate alumina. During post-peak cooling, there were localized developments of biotite + sillimanite + quartz symplectites replacing garnet and cordierite and biotite + quartz intergrowths after orthopyroxene. Application of garnet-orthopyroxene and garnet-biotite Fe–Mg exchange thermometers to co-existing garnet rim and symplectitic biotite show the extent of cooling to 610–660 °C. Electron microprobe geochronology of texturally well constrained monazites indicates the timing of peak granulite metamorphism at 3057 ± 17 Ma and its metamorphic reheating at 2781 ± 16 Ma. The present findings when collated with available geological and geophysical data appear to indicate that the studied granulites and the associated granite gneisses, charnockite and enderbite suite of rocks of the Rengali Domain are part of the exhumed lower continental crust of the Singhbhum Craton. The significance of this Neoarchaean orogenesis in the ‘Ur’ supercontinent assembly is discussed. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>In this study, we investigate the geological significance and the antiquity of lower crustal granulite facies metamorphism from the Rengali Domain, which lies in between the Singhbhum Craton in the north and the Eastern Ghats Mobile Belt in the south. Petrographic, mineral compositional, metamorphic reaction history and geothermobarometric studies of two representative metapelite granulite samples reveal widespread biotite melting at peak granulite facies metamorphic conditions of 7.8 ± 0.13 kbar, 849 ± 31 °C and subsequent melt extraction, producing a mixture of residual granulites and melts in the Rengali Province. Depending on local bulk rock compositional variations, biotite melting produced peak metamorphic assemblages of garnet + cordierite in the more aluminous compositional domain, while garnet + orthopyroxene + cordierite resulted in domains of intermediate alumina. During post-peak cooling, there were localized developments of biotite + sillimanite + quartz symplectites replacing garnet and cordierite and biotite + quartz intergrowths after orthopyroxene. Application of garnet-orthopyroxene and garnet-biotite Fe–Mg exchange thermometers to co-existing garnet rim and symplectitic biotite show the extent of cooling to 610–660 °C. Electron microprobe geochronology of texturally well constrained monazites indicates the timing of peak granulite metamorphism at 3057 ± 17 Ma and its metamorphic reheating at 2781 ± 16 Ma. The present findings when collated with available geological and geophysical data appear to indicate that the studied granulites and the associated granite gneisses, charnockite and enderbite suite of rocks of the Rengali Domain are part of the exhumed lower continental crust of the Singhbhum Craton. The significance of this Neoarchaean orogenesis in the ‘Ur’ supercontinent assembly is discussed. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1313" xmlns="http://purl.org/rss/1.0/"><title>Plates vs plumes—a geological controversy by Gillian R. Foulger. Wiley-Blackwell, Chichester, 2010. No. of pages: 328. Price: UK£39-95. ISBN 978-1-4051-6148-0 (paperback).</title><link>http://dx.doi.org/10.1002%2Fgj.1313</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Plates vs plumes—a geological controversy by Gillian R. Foulger. Wiley-Blackwell, Chichester, 2010. No. of pages: 328. Price: UK£39-95. ISBN 978-1-4051-6148-0 (paperback).</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Alan Roberts</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-06-26T21:34:43.65624-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1313</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1313</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1313</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Book Review</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[]]></content:encoded><description/></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1315" xmlns="http://purl.org/rss/1.0/"><title>The fallen sky: An intimate history of shooting stars by Christopher Cokinos. Jeremy P. Tarcher/Penguin, New York, 2009. No. of pages: 517. Price: US$27-95. ISBN 978-1- 58542-720-8 (hardback).</title><link>http://dx.doi.org/10.1002%2Fgj.1315</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">The fallen sky: An intimate history of shooting stars by Christopher Cokinos. Jeremy P. Tarcher/Penguin, New York, 2009. No. of pages: 517. Price: US$27-95. ISBN 978-1- 58542-720-8 (hardback).</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Stephen K. Donovan</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-06-21T03:32:39.529435-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1315</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1315</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1315</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Book Review</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[]]></content:encoded><description/></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1309" xmlns="http://purl.org/rss/1.0/"><title>Origin and diamond prospectivity of Mesoproterozoic kimberlites from the Narayanpet field, Eastern Dharwar Craton, southern India: insights from groundmass mineralogy, bulk-chemistry and perovskite oxybarometry</title><link>http://dx.doi.org/10.1002%2Fgj.1309</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Origin and diamond prospectivity of Mesoproterozoic kimberlites from the Narayanpet field, Eastern Dharwar Craton, southern India: insights from groundmass mineralogy, bulk-chemistry and perovskite oxybarometry</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">N. V. Chalapathi Rao</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">C. Paton</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">B. Lehmann</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-06-10T00:50:59.863333-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1309</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1309</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1309</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Special Issue Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>The Mesoproterozoic Narayanpet Kimberlite Field (NKF) is located ~200 km north of the well-known Wajrakarur Kimberlite Field (WKF) in the Eastern Dharwar Craton, southern India. Whereas a majority of the WKF occurrences are diamondiferous and contain mantle xenoliths and xenocrysts, their paucity is a characteristic feature of the NKF. This has been attributed alternately to the derivation of NKF magmas from a shallower depth, or to variability in thickness of the Sub-Continental Lithospheric Mantle (SCLM) beneath the Eastern Dharwar Craton. Recently, exploration by De Beers resulted in the discovery of a number of new kimberlite occurrences from the NKF, with some of their geochemical features and radiogenic isotope systematics subsequently becoming available. In this paper, we present detailed petrography, groundmass mineral composition and new bulk-rock geochemistry data for a number of NKF rocks and attempt to further constrain their origin. We also investigate the influence of redox conditions on diamond prospectivity by estimating oxygen fugacity (<em>f</em>O<sub>2</sub>) from Fe–Nb oxybarometry on NKF groundmass perovskites. We identify for the first time in the NKF the presence of volcaniclastic (fragmental textured) facies kimberlite belonging to the diatreme portion of the intrusion. Rarity of olivine macrocrysts and the presence of diopside are hallmarks of the NKF kimberlites, in contrast to archetypal kimberlites of southern Africa. Mineral components of the groundmass display features that are characteristic to both archetypal kimberlites and to orangeites, and it is not straight forward to apply conventional mineral-genetic schemes in the nomenclature of the NKF pipes. Low <em>f</em>O<sub>2</sub> of the NKF magma (ΔNNO (nickel–nickel oxide) = −1.9 to −3.2), indistinguishable from that of diamondiferous kimberlites world-wide, indicates that redox conditions were favourable for diamond prospectivity, and that magmatic emplacement could, instead, have played a major role in their low diamond potential. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>The Mesoproterozoic Narayanpet Kimberlite Field (NKF) is located ~200 km north of the well-known Wajrakarur Kimberlite Field (WKF) in the Eastern Dharwar Craton, southern India. Whereas a majority of the WKF occurrences are diamondiferous and contain mantle xenoliths and xenocrysts, their paucity is a characteristic feature of the NKF. This has been attributed alternately to the derivation of NKF magmas from a shallower depth, or to variability in thickness of the Sub-Continental Lithospheric Mantle (SCLM) beneath the Eastern Dharwar Craton. Recently, exploration by De Beers resulted in the discovery of a number of new kimberlite occurrences from the NKF, with some of their geochemical features and radiogenic isotope systematics subsequently becoming available. In this paper, we present detailed petrography, groundmass mineral composition and new bulk-rock geochemistry data for a number of NKF rocks and attempt to further constrain their origin. We also investigate the influence of redox conditions on diamond prospectivity by estimating oxygen fugacity (fO2) from Fe–Nb oxybarometry on NKF groundmass perovskites. We identify for the first time in the NKF the presence of volcaniclastic (fragmental textured) facies kimberlite belonging to the diatreme portion of the intrusion. Rarity of olivine macrocrysts and the presence of diopside are hallmarks of the NKF kimberlites, in contrast to archetypal kimberlites of southern Africa. Mineral components of the groundmass display features that are characteristic to both archetypal kimberlites and to orangeites, and it is not straight forward to apply conventional mineral-genetic schemes in the nomenclature of the NKF pipes. Low fO2 of the NKF magma (ΔNNO (nickel–nickel oxide) = −1.9 to −3.2), indistinguishable from that of diamondiferous kimberlites world-wide, indicates that redox conditions were favourable for diamond prospectivity, and that magmatic emplacement could, instead, have played a major role in their low diamond potential. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1308" xmlns="http://purl.org/rss/1.0/"><title>2.62 Ga high-temperature metamorphism in the central part of the Eastern Dharwar Craton: implications for late Archaean tectonothermal history</title><link>http://dx.doi.org/10.1002%2Fgj.1308</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">2.62 Ga high-temperature metamorphism in the central part of the Eastern Dharwar Craton: implications for late Archaean tectonothermal history</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">M. Jayananda</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">M. Banerjee</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">N. C. Pant</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">S. Dasgupta</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">T. Kano</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">N. Mahesha</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">B. Mahabaleswar</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-05-31T00:55:00.020681-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1308</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1308</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1308</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Special Issue Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>Aluminous metasediments occurring in the central part of the Eastern Dharwar Craton (EDC), southern India, develop contrasting mineral assemblages in closely spaced domains. Detailed petrographic, mineral chemical and geothermobarometry showed ‘peak’ metamorphic conditions of 780–820 °C and ~5 kbar that resulted in partial melting of biotite-bearing protoliths. Initial bulk compositional heterogeneity and different degrees of melt extraction produced diverse restitic mineral assemblages. <em>P–T</em> pseudosections, constructed from effective bulk composition, and consideration of the sequence of mineral reactions, deduced from textural criteria, define a nearly isobaric heating–cooling <em>P–T</em> trajectory. Monazite in the metasediments has a detrital core age of 3161 ± 78 Ma and a metamorphic age of 2625 ± 26 Ma (EPMA chemical age), which is the first record of a pre-2500 Ma high temperature–low pressure metamorphism event in the EDC. Based on age contemporaneity with the 2.7–2.62 Ga hot juvenile magmas of tonalite–trondhjemite–granodiorite (TTG)-greenstone accretion and the deduced <em>P–T</em> history, we conclude that heat advecting from rising TTG magmas and mafic magmas (greenstones) as a consequence of mantle melting, resulted in a hot transient mid-crust during a major late Archaean tectonothermal event in the Eastern Dharwar Craton. All the phenomena are consistent with a recently proposed model involving an arc setting during ridge subduction and consequent opening of a slab window. This study therefore provides new constraints on the thermal evolution of the Eastern Dharwar Craton. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>Aluminous metasediments occurring in the central part of the Eastern Dharwar Craton (EDC), southern India, develop contrasting mineral assemblages in closely spaced domains. Detailed petrographic, mineral chemical and geothermobarometry showed ‘peak’ metamorphic conditions of 780–820 °C and ~5 kbar that resulted in partial melting of biotite-bearing protoliths. Initial bulk compositional heterogeneity and different degrees of melt extraction produced diverse restitic mineral assemblages. P–T pseudosections, constructed from effective bulk composition, and consideration of the sequence of mineral reactions, deduced from textural criteria, define a nearly isobaric heating–cooling P–T trajectory. Monazite in the metasediments has a detrital core age of 3161 ± 78 Ma and a metamorphic age of 2625 ± 26 Ma (EPMA chemical age), which is the first record of a pre-2500 Ma high temperature–low pressure metamorphism event in the EDC. Based on age contemporaneity with the 2.7–2.62 Ga hot juvenile magmas of tonalite–trondhjemite–granodiorite (TTG)-greenstone accretion and the deduced P–T history, we conclude that heat advecting from rising TTG magmas and mafic magmas (greenstones) as a consequence of mantle melting, resulted in a hot transient mid-crust during a major late Archaean tectonothermal event in the Eastern Dharwar Craton. All the phenomena are consistent with a recently proposed model involving an arc setting during ridge subduction and consequent opening of a slab window. This study therefore provides new constraints on the thermal evolution of the Eastern Dharwar Craton. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1307" xmlns="http://purl.org/rss/1.0/"><title>Tracing the Proterozoic continental collision in NW India: a geophysical approach</title><link>http://dx.doi.org/10.1002%2Fgj.1307</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Tracing the Proterozoic continental collision in NW India: a geophysical approach</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">K. Naganjaneyulu</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">M. Santosh</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-05-10T01:56:07.768751-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1307</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1307</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1307</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Special Issue Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>The 800 km-long Aravalli–Delhi Fold Belt (ADFB) in the Aravalli Mountains of Rajasthan defines the largest tectonic feature in the northwestern (NW) Indian shield, situated between the late Proterozoic Marwar Basin in the west and the Vindhyan Basin in the east. The final collision between the Aravalli and Delhi domains defining ocean closure and continental amalgamation is critical in understanding the culmination of the Proterozoic Wilson Cycle in NW India. We present for the first time a regional three-dimensional (3-D) gravity model to evaluate the architecture of the continental collision signature of this region. The deep seismic reflection data along a 400 km-long profile across the ADFB highlights two sets of reflection bands with opposite dips. The prominent west-dipping reflections observed in the central domain, towards the western margin of the Mangalwar Complex could be related to the Palaeoproterozoic subduction of an oceanic lithosphere, and suggest a clear northwestward subduction polarity. The data showing gravity highs, the high elevation features, and the models proposed in the present study, together with the presence of high-density bodies in the deep crust, is interpreted as a signature of magmatic underplating and/or mafic-ultramafic intrusives. The high elevations and corresponding high-density anomalies at depth can also be explained by domal uplift, following the extrusion of metamorphic orogens into the mid crust, as well as the presence of eclogitized material at depth associated with the subduction–collision tectonics and continental amalgamation. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>The 800 km-long Aravalli–Delhi Fold Belt (ADFB) in the Aravalli Mountains of Rajasthan defines the largest tectonic feature in the northwestern (NW) Indian shield, situated between the late Proterozoic Marwar Basin in the west and the Vindhyan Basin in the east. The final collision between the Aravalli and Delhi domains defining ocean closure and continental amalgamation is critical in understanding the culmination of the Proterozoic Wilson Cycle in NW India. We present for the first time a regional three-dimensional (3-D) gravity model to evaluate the architecture of the continental collision signature of this region. The deep seismic reflection data along a 400 km-long profile across the ADFB highlights two sets of reflection bands with opposite dips. The prominent west-dipping reflections observed in the central domain, towards the western margin of the Mangalwar Complex could be related to the Palaeoproterozoic subduction of an oceanic lithosphere, and suggest a clear northwestward subduction polarity. The data showing gravity highs, the high elevation features, and the models proposed in the present study, together with the presence of high-density bodies in the deep crust, is interpreted as a signature of magmatic underplating and/or mafic-ultramafic intrusives. The high elevations and corresponding high-density anomalies at depth can also be explained by domal uplift, following the extrusion of metamorphic orogens into the mid crust, as well as the presence of eclogitized material at depth associated with the subduction–collision tectonics and continental amalgamation. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1305" xmlns="http://purl.org/rss/1.0/"><title>The Second Jurassic Dinosaur Rush: Museums and Paleontology in America at the Turn of the Twentieth Century by Paul D. Brinkman. University of Chicago Press, Chicago, 2010. No. of pages: xiv + 345. Price: US$49.00. ISBN 978-0-226-07472-6 (hardback).</title><link>http://dx.doi.org/10.1002%2Fgj.1305</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">The Second Jurassic Dinosaur Rush: Museums and Paleontology in America at the Turn of the Twentieth Century by Paul D. Brinkman. University of Chicago Press, Chicago, 2010. No. of pages: xiv + 345. Price: US$49.00. ISBN 978-0-226-07472-6 (hardback).</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Stephen K. Donovan</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-04-14T00:31:26.280378-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1305</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1305</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1305</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Book Review</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[]]></content:encoded><description/></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1302" xmlns="http://purl.org/rss/1.0/"><title>Early Precambrian mafic dyke swarms from the Central Archaean Bastar Craton, India: geochemistry, petrogenesis and tectonic implications</title><link>http://dx.doi.org/10.1002%2Fgj.1302</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Early Precambrian mafic dyke swarms from the Central Archaean Bastar Craton, India: geochemistry, petrogenesis and tectonic implications</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Rajesh K. Srivastava</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Gulab C. Gautam</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-04-05T02:20:49.618716-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1302</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1302</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1302</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Special Issue Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3><div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>The Archaean Bastar craton is known for the presence of different generations of mafic dykes. Less studied many NW-SE trending mafic dykes (intruded into the Archaean supracrustal rocks), encountered from the central part of the Bastar craton, are studied for their petrological and geochemical characteristics. There are many geological evidences which suggest emplacement of these mafic dykes in an intracratonic setting. Two distinct types of mafic dykes are recognized. Petrographically it is difficult to discriminate these two types. Many samples show metamorphic textures and amphibolites facies mineral assemblage but a few samples preserved original igneous texture and mineralogy. Major oxides show sub-alkaline thoeliitic basalt/basaltic andesite nature. High-Fe and high-Mg contents classify them as high-iron and high-magnesium tholeiites. They fall in the gabbronorite field on R1-R2 plot. Geochemical characteristics, particularly high-field strength and rare-earth elements, clearly distinguished them into two types: Group 1 and Group 2 mafic dykes. When compared with well-studied mafic dyke swarms of the Southern Bastar craton, the Group 1 is recognized as Meso-Neoarchaean sub-alkaline mafic dykes (BD1-CBC) and the Group 2 as Neoarchaean-Palaeoproterozoic boninite–norite mafic dykes (BN-CBC). The boninite–norite nature of the second group is also corroborated through immobile trace element ratios. BD1-CBC dykes are characterized by a relatively higher concentration of HFSE and REE in comparison to BN-CBC dykes. Some extent of crustal contamination is observed in BN-CBC dykes but BD1-CBC dykes do not show any indication of crustal contamination. Trace element modelling suggest that BD1-CBC mafic dykes are derived from a melt originated through ∼20% melting of a depleted mantle source, whereas BN-CBC mafic dykes are probably derived from a high-Mg magma generated through ∼25% melting of a refractory mantle source. Both melts have undergone 30–40% olivine fractionation before the emplacement. Geochemistry also points out involvement of a plume in the genesis of these mafic dykes. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>The Archaean Bastar craton is known for the presence of different generations of mafic dykes. Less studied many NW-SE trending mafic dykes (intruded into the Archaean supracrustal rocks), encountered from the central part of the Bastar craton, are studied for their petrological and geochemical characteristics. There are many geological evidences which suggest emplacement of these mafic dykes in an intracratonic setting. Two distinct types of mafic dykes are recognized. Petrographically it is difficult to discriminate these two types. Many samples show metamorphic textures and amphibolites facies mineral assemblage but a few samples preserved original igneous texture and mineralogy. Major oxides show sub-alkaline thoeliitic basalt/basaltic andesite nature. High-Fe and high-Mg contents classify them as high-iron and high-magnesium tholeiites. They fall in the gabbronorite field on R1-R2 plot. Geochemical characteristics, particularly high-field strength and rare-earth elements, clearly distinguished them into two types: Group 1 and Group 2 mafic dykes. When compared with well-studied mafic dyke swarms of the Southern Bastar craton, the Group 1 is recognized as Meso-Neoarchaean sub-alkaline mafic dykes (BD1-CBC) and the Group 2 as Neoarchaean-Palaeoproterozoic boninite–norite mafic dykes (BN-CBC). The boninite–norite nature of the second group is also corroborated through immobile trace element ratios. BD1-CBC dykes are characterized by a relatively higher concentration of HFSE and REE in comparison to BN-CBC dykes. Some extent of crustal contamination is observed in BN-CBC dykes but BD1-CBC dykes do not show any indication of crustal contamination. Trace element modelling suggest that BD1-CBC mafic dykes are derived from a melt originated through ∼20% melting of a depleted mantle source, whereas BN-CBC mafic dykes are probably derived from a high-Mg magma generated through ∼25% melting of a refractory mantle source. Both melts have undergone 30–40% olivine fractionation before the emplacement. Geochemistry also points out involvement of a plume in the genesis of these mafic dykes. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1300" xmlns="http://purl.org/rss/1.0/"><title>U-Pb zircon geochronology of granites and charnockite from southern India: implications for magmatic pulses associated with plate tectonic cycles within a Precambrian suture zone</title><link>http://dx.doi.org/10.1002%2Fgj.1300</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">U-Pb zircon geochronology of granites and charnockite from southern India: implications for magmatic pulses associated with plate tectonic cycles within a Precambrian suture zone</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Kei Sato</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">M. Santosh</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">T. R. K. Chetty</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Takafumi Hirata</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-04-05T02:14:45.605356-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1300</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1300</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1300</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Special Issue Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3><div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>The Palghat–Cauvery Suture Zone (PCSZ) in southern India marks the trace along which continental blocks were sutured during the Precambrian. We report here U-Pb geochronological data based on laser ablation ICP mass spectrometry for zircons in two granite plutons and an associated charnockite from within the PCSZ. The weighted mean of <sup>206</sup>Pb/<sup>238</sup>U ages for a rapakivi granite from the southern part of the PCSZ yields 819 ± 26 Ma (error: 2<em>σ</em>; <em>N</em> = 13). On the other hand, a metamorphosed A-type granite and a charnockite from the central part of the PCSZ yield a markedly older upper intercept age of 2468 ± 36 Ma (error: 2<em>σ</em>) and a lower intercept age of 588 ± 36 Ma (error: 2<em>σ</em>). Our results provide important constraints on the Precambrian crustal evolution in the PCSZ and demonstrate: (1) Neoarchaean to early Palaeoproterozoic magmatism, generating A-type granites which we correlate with a major global crustal formation event; (2) mid Neoproterozoic magmatism, and generation of the rapakivi granite, probably associated with the subduction of the Mozambique Ocean floor; and (3) latest Neoproterozoic high-grade metamorphism (generating the charnockite) associated with the collisional amalgamation of the Gondwana supercontinent. Together with the previous geochronological data from the PCSZ and adjacent crustal blocks, our results provide information on magmatic pulses associated with the Archaean cratonization event, as well as the Neoproterozoic Wilson Cycle of the Mozambique Ocean culminating in continent-continent collision. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>The Palghat–Cauvery Suture Zone (PCSZ) in southern India marks the trace along which continental blocks were sutured during the Precambrian. We report here U-Pb geochronological data based on laser ablation ICP mass spectrometry for zircons in two granite plutons and an associated charnockite from within the PCSZ. The weighted mean of 206Pb/238U ages for a rapakivi granite from the southern part of the PCSZ yields 819 ± 26 Ma (error: 2σ; N = 13). On the other hand, a metamorphosed A-type granite and a charnockite from the central part of the PCSZ yield a markedly older upper intercept age of 2468 ± 36 Ma (error: 2σ) and a lower intercept age of 588 ± 36 Ma (error: 2σ). Our results provide important constraints on the Precambrian crustal evolution in the PCSZ and demonstrate: (1) Neoarchaean to early Palaeoproterozoic magmatism, generating A-type granites which we correlate with a major global crustal formation event; (2) mid Neoproterozoic magmatism, and generation of the rapakivi granite, probably associated with the subduction of the Mozambique Ocean floor; and (3) latest Neoproterozoic high-grade metamorphism (generating the charnockite) associated with the collisional amalgamation of the Gondwana supercontinent. Together with the previous geochronological data from the PCSZ and adjacent crustal blocks, our results provide information on magmatic pulses associated with the Archaean cratonization event, as well as the Neoproterozoic Wilson Cycle of the Mozambique Ocean culminating in continent-continent collision. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1297" xmlns="http://purl.org/rss/1.0/"><title>The terrestrialization process: Modelling complex interactions at the biosphere–geosphere interface, edited by M. Vecoli, G. Clément, &amp; B. Meyer-Berthaud. Geological Society Special Publications, 339, 2010. No. of pages: 187. ISBN 978-1-86239-309-7 (hardback)</title><link>http://dx.doi.org/10.1002%2Fgj.1297</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">The terrestrialization process: Modelling complex interactions at the biosphere–geosphere interface, edited by M. Vecoli, G. Clément, &amp; B. Meyer-Berthaud. Geological Society Special Publications, 339, 2010. No. of pages: 187. ISBN 978-1-86239-309-7 (hardback)</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">J.H.A. van Konijnenburg-van Cittert</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2011-03-01T23:00:20.429983-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1297</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1297</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1297</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Book Review</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[]]></content:encoded><description/></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1324" xmlns="http://purl.org/rss/1.0/"><title>Trace fossils and palaeoenvironments of the Middle Devonian Caherbla Group, Dingle Peninsula, southwest Ireland</title><link>http://dx.doi.org/10.1002%2Fgj.1324</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Trace fossils and palaeoenvironments of the Middle Devonian Caherbla Group, Dingle Peninsula, southwest Ireland</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Lance B. Morrissey</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Simon Braddy</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Chris Dodd</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Kenneth T. Higgs</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Brian P. J. Williams</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-01-01T00:00:00-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1324</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1324</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1324</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Research Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">29</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>Trace fossils from the Middle Devonian Caherbla Group of the Dingle Peninsula, southwest Ireland, record a diverse arthropod fauna inhabiting a hot-arid intracontinental rift setting. Aeolian dunefield and coeval fluvial interdune deposits interfinger spatially and temporally with alluvial fan sedimentary rocks. Three distinct trace fossil assemblages are recognized. The <em>Taenidium-Scoyenia</em> ichnocoenosis occurs in alluvial fan and fluvial channel deposits, and includes the large backfilled burrow <em>Taenidium</em>, interpreted as eoarthropleurid aestivation chambers. The <em>Rusophycu</em>s-<em>Protichnites</em> ichnocoenosis, composed of arthropod trackways and surface pits, occurs in an interdune ponded area that was susceptible to ephemeral fluvial flow, with <em>Rusophycus</em> showing preferred orientation into the oncoming palaeocurrent. Both the <em>Taenidium-Scoyenia</em> and <em>Rusophycu</em>s-<em>Protichnites</em> ichnocoenoses are assignable to the globally recurring continental <em>Scoyenia</em> ichnofacies. They are clearly substrate-controlled and moisture-related due to the ephemeral nature of the fluvial system. The <em>Palmichnium-Entradichnus</em> ichnocoenosis occurs in aeolian dune deposits, and includes <em>Palmichnium</em>, attributed to large stylonurid eurypterids, and <em>Diplichnites</em>, attributed to eoarthropleurids. These trackways represent the activities of dune pioneers that left their fluvial habitat to forage for detritus. Interface burrows (<em>Entradichnus</em>, <em>Palaeophycus</em>) were also constructed by arthropods moving just under the sand surface and vertical burrows (<em>Cylindricum</em>, <em>Pustulichnus</em>) were made by arthropods digging downward. Trace preservation in the aeolian environment was probably enhanced by heavy nocturnal dew-fall or light rain. The <em>Palmichnium-Entradichnus</em> ichnocoenosis is assigned to the globally recurring aeolian <em>Octopodichnus-Entradichnus</em> ichnofacies. This aeolian facies, and associated ichnofauna described herein, represents the oldest development of a unique erg system in the Old Red Sandstone (Devonian) of the southern British Isles, and one of the oldest and most diverse aeolian ichnofaunas to be reported worldwide. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>Trace fossils from the Middle Devonian Caherbla Group of the Dingle Peninsula, southwest Ireland, record a diverse arthropod fauna inhabiting a hot-arid intracontinental rift setting. Aeolian dunefield and coeval fluvial interdune deposits interfinger spatially and temporally with alluvial fan sedimentary rocks. Three distinct trace fossil assemblages are recognized. The Taenidium-Scoyenia ichnocoenosis occurs in alluvial fan and fluvial channel deposits, and includes the large backfilled burrow Taenidium, interpreted as eoarthropleurid aestivation chambers. The Rusophycus-Protichnites ichnocoenosis, composed of arthropod trackways and surface pits, occurs in an interdune ponded area that was susceptible to ephemeral fluvial flow, with Rusophycus showing preferred orientation into the oncoming palaeocurrent. Both the Taenidium-Scoyenia and Rusophycus-Protichnites ichnocoenoses are assignable to the globally recurring continental Scoyenia ichnofacies. They are clearly substrate-controlled and moisture-related due to the ephemeral nature of the fluvial system. The Palmichnium-Entradichnus ichnocoenosis occurs in aeolian dune deposits, and includes Palmichnium, attributed to large stylonurid eurypterids, and Diplichnites, attributed to eoarthropleurids. These trackways represent the activities of dune pioneers that left their fluvial habitat to forage for detritus. Interface burrows (Entradichnus, Palaeophycus) were also constructed by arthropods moving just under the sand surface and vertical burrows (Cylindricum, Pustulichnus) were made by arthropods digging downward. Trace preservation in the aeolian environment was probably enhanced by heavy nocturnal dew-fall or light rain. The Palmichnium-Entradichnus ichnocoenosis is assigned to the globally recurring aeolian Octopodichnus-Entradichnus ichnofacies. This aeolian facies, and associated ichnofauna described herein, represents the oldest development of a unique erg system in the Old Red Sandstone (Devonian) of the southern British Isles, and one of the oldest and most diverse aeolian ichnofaunas to be reported worldwide. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1329" xmlns="http://purl.org/rss/1.0/"><title>Geomorphologic assessment of relative tectonic activity in the Maharlou Lake Basin, Zagros Mountains of Iran</title><link>http://dx.doi.org/10.1002%2Fgj.1329</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Geomorphologic assessment of relative tectonic activity in the Maharlou Lake Basin, Zagros Mountains of Iran</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Ali Faghih</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Babak Samani</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Timothy Kusky</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Saman Khabazi</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Reihaneh Roshanak</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-01-01T00:00:00-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1329</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1329</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1329</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Research Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">30</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">40</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>Spatial differences of Quaternary deformation and intensity of tectonic activity are assessed through a detailed quantitative geomorphic study of the fault-generated mountain fronts and alluvial/fluvial systems around the Maharlou Lake Basin in the Zagros Fold–Thrust Belt of Iran. The Maharlou Lake Basin is defined as an approximately northwest–southeast trending, linear, topographic depression located in the central Zagros Mountains of Iran. The lake is located in a tectonically active area delineated by the Ghareh and Maharlou faults. Combined geomorphic and morphometric data reveal differences between the Ghareh and Maharlou mountain front faults indicating different levels of tectonic activity along each mountain front. Geomorphic indices show a relatively high degree of tectonic activity along the Ghareh Mountain Front in the southwest, in contrast with less tectonic activity along the Ahmadi Mountain Front northeast of the lake which is consistent with field evidence and seismotectonic data for the study area. A ramp valley tectonic setting is proposed to explain the tectonosedimentary evolution of the lake. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>Spatial differences of Quaternary deformation and intensity of tectonic activity are assessed through a detailed quantitative geomorphic study of the fault-generated mountain fronts and alluvial/fluvial systems around the Maharlou Lake Basin in the Zagros Fold–Thrust Belt of Iran. The Maharlou Lake Basin is defined as an approximately northwest–southeast trending, linear, topographic depression located in the central Zagros Mountains of Iran. The lake is located in a tectonically active area delineated by the Ghareh and Maharlou faults. Combined geomorphic and morphometric data reveal differences between the Ghareh and Maharlou mountain front faults indicating different levels of tectonic activity along each mountain front. Geomorphic indices show a relatively high degree of tectonic activity along the Ghareh Mountain Front in the southwest, in contrast with less tectonic activity along the Ahmadi Mountain Front northeast of the lake which is consistent with field evidence and seismotectonic data for the study area. A ramp valley tectonic setting is proposed to explain the tectonosedimentary evolution of the lake. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1331" xmlns="http://purl.org/rss/1.0/"><title>Electron microprobe monazite geochronology of granitic intrusions from the Montes de Toledo batholith (central Spain)</title><link>http://dx.doi.org/10.1002%2Fgj.1331</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Electron microprobe monazite geochronology of granitic intrusions from the Montes de Toledo batholith (central Spain)</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">David Orejana</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Enrique Merino</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Carlos Villaseca</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Cecilia Pérez-Soba</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Andrés Cuesta</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-01-01T00:00:00-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1331</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1331</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1331</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Research Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">41</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">58</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>U–Th–Pb monazite dating by electron microprobe has been applied to three peraluminous granitic intrusions of the western Montes de Toledo batholith (MTB). Back scattered electron images of monazite crystals reveal a variety of internal textures: patchy zoning, overgrowths around older cores and unzoned crystals. On the basis of their zoning pattern and chemical composition, two monazite domains can be distinguished: (1) corroded cores and crystals with patchy zoning, exhibiting relatively constant Th/U ratios and broadly older ages, and (2) unzoned grains and monazite rims, with variable Th/U ratios and younger ages. The first monazite group represents inherited domains from metamorphic sources, which accounts for pre-magmatic monazite growth events. Two average ages from Torrico and Belvís de Monroy granites (333 ± 18 and 333 ± 5 Ma, respectively) relate these cores to a Viséan extensional deformation phase. The second group represents igneous monazites which have provided the following crystallization ages for the host granite: 298 ± 11 Ma (Villar del Pedroso), 303 ± 6 Ma (Torrico) and 314 ± 3 Ma (Belvís de Monroy). Two main magmatic pulses, the first about 314 Ma and the second at the end of the Carboniferous (303–298 Ma), might be envisaged in the western MTB. While Belvís de Monroy leucogranite is likely a syn- to late-tectonic intrusion, the Villar del Pedroso and Torrico plutons represent post-tectonic magmas with emplacement ages similar to those of equivalent intrusions from nearby Variscan magmatic sectors. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>U–Th–Pb monazite dating by electron microprobe has been applied to three peraluminous granitic intrusions of the western Montes de Toledo batholith (MTB). Back scattered electron images of monazite crystals reveal a variety of internal textures: patchy zoning, overgrowths around older cores and unzoned crystals. On the basis of their zoning pattern and chemical composition, two monazite domains can be distinguished: (1) corroded cores and crystals with patchy zoning, exhibiting relatively constant Th/U ratios and broadly older ages, and (2) unzoned grains and monazite rims, with variable Th/U ratios and younger ages. The first monazite group represents inherited domains from metamorphic sources, which accounts for pre-magmatic monazite growth events. Two average ages from Torrico and Belvís de Monroy granites (333 ± 18 and 333 ± 5 Ma, respectively) relate these cores to a Viséan extensional deformation phase. The second group represents igneous monazites which have provided the following crystallization ages for the host granite: 298 ± 11 Ma (Villar del Pedroso), 303 ± 6 Ma (Torrico) and 314 ± 3 Ma (Belvís de Monroy). Two main magmatic pulses, the first about 314 Ma and the second at the end of the Carboniferous (303–298 Ma), might be envisaged in the western MTB. While Belvís de Monroy leucogranite is likely a syn- to late-tectonic intrusion, the Villar del Pedroso and Torrico plutons represent post-tectonic magmas with emplacement ages similar to those of equivalent intrusions from nearby Variscan magmatic sectors. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1336" xmlns="http://purl.org/rss/1.0/"><title>Trace element geochemistry of primary mantle minerals in spinel-peridotites from polygenetic MOR–SSZ suites of SW Turkey: constraints from an LA-ICP-MS study and implications for mantle metasomatism</title><link>http://dx.doi.org/10.1002%2Fgj.1336</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Trace element geochemistry of primary mantle minerals in spinel-peridotites from polygenetic MOR–SSZ suites of SW Turkey: constraints from an LA-ICP-MS study and implications for mantle metasomatism</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">E. Aldanmaz</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-01-01T00:00:00-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1336</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1336</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1336</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Research Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">59</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">76</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>Ophiolites exposed across the western Tauride Belt in SW Turkey represent tectonically emplaced fragments of oceanic lithosphere incorporated into continental margin following the closure of the Neotethys Ocean during the Late Cretaceous. The mantle sections of the ophiolites contain peridotites with diverse suites of geochemical signatures indicative of residual origin by melt depletion in both mid-ocean ridge (MOR) and supra-subduction zone (SSZ) settings. This study uses a laser-ablation inductively-coupled plasma-mass spectrometry (LA-ICP-MS) for <em>in situ</em> measurements of trace elements in primary mantle phases in order to identify the upper mantle petrogenetic processes effective during variable stage of melt extraction in these discrete tectonic settings and to discriminate between the effects of reaction with chemically distinct mantle melts migrating through the solid residues. Trace element signatures in pyroxenes suggest small-length scales of compositional variations which may be interpreted to be a result of post-melting petrogenetic processes. Relative distribution of rare earth elements and Li between coexisting orthopyroxene-clinopyroxene pairs in the peridotites suggests compositional disequilibrium in sub-solidus conditions, which possibly reflects differential effects of diffusive exchange during melting and melt transport or interaction with subduction melts/fluids. On the basis of Ga abundances and Ga–Ti–Fe<sup>+3</sup># [Fe<sup>+3</sup>/(Fe<sup>+3</sup> + Cr + Al)] relationships of chrome-spinels it is documented that the peridotites have experienced the combined effects of partial melting and variable extent of melt-solid interaction. The MOR peridotites have spinels with geochemical signatures indicative of melt-depleted residual origin with subsequent incompatible element enrichment through melt impregnation, while the Ga–Ti–Fe<sup>+3</sup># relationships of chrome-spinels in SSZ peridotites indicate that these highly depleted peridotites are not simple melt residues, but have been subject to significant compositional modification by interaction with subduction related melts/fluids. The observed compositional variations, which are related to long-term tectonic reorganisation of oceanic lithosphere, provide evidence for a time integrated evolution from a mid-ocean ridge to a supra-subduction zone setting and may be a possible analogue to explain the coexistence of geochemically diverse MOR–SSZ suites in other Tethyan ophiolites. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>Ophiolites exposed across the western Tauride Belt in SW Turkey represent tectonically emplaced fragments of oceanic lithosphere incorporated into continental margin following the closure of the Neotethys Ocean during the Late Cretaceous. The mantle sections of the ophiolites contain peridotites with diverse suites of geochemical signatures indicative of residual origin by melt depletion in both mid-ocean ridge (MOR) and supra-subduction zone (SSZ) settings. This study uses a laser-ablation inductively-coupled plasma-mass spectrometry (LA-ICP-MS) for in situ measurements of trace elements in primary mantle phases in order to identify the upper mantle petrogenetic processes effective during variable stage of melt extraction in these discrete tectonic settings and to discriminate between the effects of reaction with chemically distinct mantle melts migrating through the solid residues. Trace element signatures in pyroxenes suggest small-length scales of compositional variations which may be interpreted to be a result of post-melting petrogenetic processes. Relative distribution of rare earth elements and Li between coexisting orthopyroxene-clinopyroxene pairs in the peridotites suggests compositional disequilibrium in sub-solidus conditions, which possibly reflects differential effects of diffusive exchange during melting and melt transport or interaction with subduction melts/fluids. On the basis of Ga abundances and Ga–Ti–Fe+3# [Fe+3/(Fe+3 + Cr + Al)] relationships of chrome-spinels it is documented that the peridotites have experienced the combined effects of partial melting and variable extent of melt-solid interaction. The MOR peridotites have spinels with geochemical signatures indicative of melt-depleted residual origin with subsequent incompatible element enrichment through melt impregnation, while the Ga–Ti–Fe+3# relationships of chrome-spinels in SSZ peridotites indicate that these highly depleted peridotites are not simple melt residues, but have been subject to significant compositional modification by interaction with subduction related melts/fluids. The observed compositional variations, which are related to long-term tectonic reorganisation of oceanic lithosphere, provide evidence for a time integrated evolution from a mid-ocean ridge to a supra-subduction zone setting and may be a possible analogue to explain the coexistence of geochemically diverse MOR–SSZ suites in other Tethyan ophiolites. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1335" xmlns="http://purl.org/rss/1.0/"><title>The provenance of Western Irish Namurian Basin sedimentary strata inferred using detrital zircon U–Pb LA-ICP-MS geochronology</title><link>http://dx.doi.org/10.1002%2Fgj.1335</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">The provenance of Western Irish Namurian Basin sedimentary strata inferred using detrital zircon U–Pb LA-ICP-MS geochronology</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Michael A. Pointon</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Robert A. Cliff</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">David M. Chew</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-01-01T00:00:00-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1335</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1335</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1335</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Research Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">77</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">98</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>The Western Irish Namurian Basin (WINB) preserves classic examples of basin floor sequences through to slope deposits and deltaic cyclothems. Despite over 50 years of research into the WINB, its sediment provenance remains highly contested. Sedimentological arguments, including palaeocurrent vectors and palaeoslope indicators have been invoked to propose a sediment source from the NW or the west (i.e. from within Laurentia). These same indicators have been subsequently reinterpreted to reflect a southern provenance. It is not clear from sedimentological arguments alone which interpretation more accurately reflects the infilling of the WINB. Regional-scale constraints on WINB provenance may be obtained with detrital zircon U–Pb geochronology.</p></div><div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>U–Pb LA-ICP-MS detrital zircon analysis was undertaken on samples from three sandstone units at different stratigraphic levels within the WINB siliciclastic sedimentary fill (Ross Formation, Tullig Sandstone, Doonlicky Sandstone). The samples are dominated by 500–700 Ma zircons, which can be correlated with Cadomian–Avalonian orogenic activity within terranes to the south of the WINB (Avalonia/Ganderia, Armorica and Iberia). In contrast, Eastern Laurentia, to the north of the WINB, was devoid of orogenic activity at this time. WINB samples also yield age populations younger than 500 Ma, and older than 700 Ma. These are not diagnostic of a particular source terrane and thus could be derived from terranes north and/or south of the WINB. WINB detrital zircon age spectra can be reconciled by an Avalonian or combined Avalonian–Laurentian provenance for WINB sedimentary strata. Further research is required in order to distinguish between these two possibilities. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>The Western Irish Namurian Basin (WINB) preserves classic examples of basin floor sequences through to slope deposits and deltaic cyclothems. Despite over 50 years of research into the WINB, its sediment provenance remains highly contested. Sedimentological arguments, including palaeocurrent vectors and palaeoslope indicators have been invoked to propose a sediment source from the NW or the west (i.e. from within Laurentia). These same indicators have been subsequently reinterpreted to reflect a southern provenance. It is not clear from sedimentological arguments alone which interpretation more accurately reflects the infilling of the WINB. Regional-scale constraints on WINB provenance may be obtained with detrital zircon U–Pb geochronology.U–Pb LA-ICP-MS detrital zircon analysis was undertaken on samples from three sandstone units at different stratigraphic levels within the WINB siliciclastic sedimentary fill (Ross Formation, Tullig Sandstone, Doonlicky Sandstone). The samples are dominated by 500–700 Ma zircons, which can be correlated with Cadomian–Avalonian orogenic activity within terranes to the south of the WINB (Avalonia/Ganderia, Armorica and Iberia). In contrast, Eastern Laurentia, to the north of the WINB, was devoid of orogenic activity at this time. WINB samples also yield age populations younger than 500 Ma, and older than 700 Ma. These are not diagnostic of a particular source terrane and thus could be derived from terranes north and/or south of the WINB. WINB detrital zircon age spectra can be reconciled by an Avalonian or combined Avalonian–Laurentian provenance for WINB sedimentary strata. Further research is required in order to distinguish between these two possibilities. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://dx.doi.org/10.1002%2Fgj.1346" xmlns="http://purl.org/rss/1.0/"><title>Usage of strain and vorticity analyses to interpret large-scale fold mechanisms along the Sanandaj–Sirjan HP-LT metamorphic belt, SW Iran</title><link>http://dx.doi.org/10.1002%2Fgj.1346</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Usage of strain and vorticity analyses to interpret large-scale fold mechanisms along the Sanandaj–Sirjan HP-LT metamorphic belt, SW Iran</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Khalil Sarkarinejad</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Abdolreza Partabian</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Ali Faghih</dc:creator><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Timothy M. Kusky</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-01-01T00:00:00-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/gj.1346</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/gj.1346</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://dx.doi.org/10.1002%2Fgj.1346</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Research Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">99</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">110</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p>3D finite strain analyses and kinematic vorticity measurements were carried out on the Loghon Anticline within the HP-LT Sanandaj–Sirjan metamorphic belt (Neyriz area, SW Iran). <em>Rƒ/φ</em> and Fry methods were used on the strain markers (e.g. deformed fossils) to interpret geometric relationships between the fold axis, strain ellipsoid axes and shear zone boundaries. The results indicate the predominance of prolate strain in the anticline. Quantitative kinematic analyses show that the W<sub>k</sub> parameter is 0. 67 ± 0. 06 (i.e. pure-shear dominated non-coaxial flow). This study quantitatively supports the establishment of a dextral transpressive system, which is responsible for the development of the large-scale right-lateral shear zones that strike sub-parallel to the major folds. Flexural shear combined with regional dextral-shear is suggested to be the most common mechanism of folding in this area. Copyright © 2011 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>3D finite strain analyses and kinematic vorticity measurements were carried out on the Loghon Anticline within the HP-LT Sanandaj–Sirjan metamorphic belt (Neyriz area, SW Iran). Rƒ/φ and Fry methods were used on the strain markers (e.g. deformed fossils) to interpret geometric relationships between the fold axis, strain ellipsoid axes and shear zone boundaries. The results indicate the predominance of prolate strain in the anticline. Quantitative kinematic analyses show that the Wk parameter is 0. 67 ± 0. 06 (i.e. pure-shear dominated non-coaxial flow). This study quantitatively supports the establishment of a dextral transpressive system, which is responsible for the development of the large-scale right-lateral shear zones that strike sub-parallel to the major folds. Flexural shear combined with regional dextral-shear is suggested to be the most common mechanism of folding in this area. Copyright © 2011 John Wiley &amp; Sons, Ltd.</description></item></rdf:RDF>
