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

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.

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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