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

Figure 12. The magnitudes of geomagnetic field direction
variations (Sp) as a function of the distance
to the center of the Siberian traps for the time
interval of 285-270 Ma. The black stars
connected by a line are the
Sp values
averaged over the intervals of 10-20o. See
Figure 7 for the other explanations.

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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