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Figure S1. Part of the CCD image centred in the −5 mag Orionid (SPMN021006) recorded from (a) Montseny and (b) Folgueroles (under a partially cloudy sky). (c) Apparent trajectory of the meteor from both stations. (d) Atmospheric trajectory and its projection on the ground. (e) The heliocentric orbit of the meteoroid projected on the ecliptic plane, where the orbits of Jupiter (J) and Saturn (S) are shown for comparison. Figure S2. Composition of the Orionid meteors imaged from Ankara (Turkey) with a Canon EOS 300D digital SLR at ISO 1600 and a 10-mm f/3.5 wide-angle lens. A total of 130 1-min shots of about the same part of sky were taken between 2035 and 2235 UTC. The radiant (marked as a white circle) is clearly consistent with that derived from astrometric measurements from Spanish CCD images (for more details see the text and Fig. 3). Please note: Blackwell Publishing is not responsible for the content or functionality of any supplementary materials supplied by the authors. Any queries (other than missing material) should be directed to the corresponding author for the article.

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MNR_11966_sm_FigureS1.jpg210KSupporting info item
MNR_11966_sm_FigureS2.jpg188KSupporting info item

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