RUSSIAN JOURNAL OF EARTH SCIENCES VOL. 8, ES1004, doi:10.2205/2006ES000191, 2006

2006ES000191-fig17.html
Figure 17. The magnitudes of the geomagnetic field direction variations (Sp) as a function of the distances to the centers of the world magnetic anomalies (WMA) [Pechersky, 2001], shown by red stars; same to the epicenters of the modern active plumes (45-50 Ma) [Pechersky, 2001], shown by violet squares; same to the epicenter of the Greenland plume (73-82 Ma) [Pechersky and Garbuzenko, 2005] shown by green triangles; same to the epicenter of the Deccan plume (95-110 Ma) [Pechersky and Garbuzenko, 2005], shown by blue triangles; same to the epicenter of the Siberian plume (270-285 Ma and 290-300 Ma) [this paper], shown by red and brown circles. These data were averaged over the interval ranging from 10o to 20o.

RJES

Citation: Pechersky, D. M. (2006), Geomagnetic field in the vicinity of the Paleozoic-Mesozoic boundary and the Siberian superplume, Russ. J. Earth Sci., 8, ES1004, doi:10.2205/2006ES000191.

Copyright 2006 by the Russian Journal of Earth Sciences
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