Revised and updated paleomagnetic results from Costa Rica
Article first published online: 3 SEP 2013
©2013. American Geophysical Union. All Rights Reserved.
Geochemistry, Geophysics, Geosystems
Volume 14, Issue 9, pages 3379–3388, September 2013
How to Cite
2013), Revised and updated paleomagnetic results from Costa Rica, Geochem. Geophys. Geosyst., 14, 3379–3388, doi:10.1002/ggge.20199., , , , and (
- Issue published online: 24 OCT 2013
- Article first published online: 3 SEP 2013
- Accepted manuscript online: 26 JUN 2013 01:50AM EST
- Manuscript Accepted: 7 JUN 2013
- Manuscript Received: 12 MAR 2013
- National Science Foundation . Grant Numbers: EAR1141840 , EAR0809709
- Costa Rica;
- paleosecular variation;
 Paleomagnetic results from globally distributed lava flows have been collected and analyzed under the time-averaged field initiative (TAFI), a multi-institutional collaboration started in 1996 and designed to improve the geographic and temporal coverage of the 0–5 Ma paleomagnetic database for studying both the time-averaged field and its very long-term secular variations. Paleomagnetic samples were collected from 35 volcanic units, either lava flows or ignimbrites, in Costa Rica in December 1998 and February 2000 from the Cordilleras Central and Guanacaste, the underlying Canas, Liberia and Bagaces formations and from Volcano Arenal. Age estimates range from approximately 40 ka to slightly over 6 Ma. Although initial results from these sites were used in a global synthesis of TAFI data by Johnson et al. (2008), a full description of methodology was not presented. This paper documents the definitive collection of results comprising 28 paleomagnetic directions (24 normal, 4 reversed), with enhanced precision and new geological interpretations, adding two paleointensity estimates and 19 correlated 40Ar/39Ar radiometric ages. The average field direction is consistent with that of a geocentric axial dipole and dispersion of virtual geomagnetic poles (17.3 ± 4.6°) is in general agreement with predictions from several statistical paleosecular variation models. Paleointensity estimates from two sites give an average field strength of 26.3 μT and a virtual axial dipole moment of 65 ZAm2. The definitive results provide a useful augmentation of the global database for the longer term goal of developing new statistical descriptions of paleomagnetic field behavior.