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

Figure 14. The magnitudes of the geomagnetic field directions
variations (Sp) as a function of the
distance to the center of the Siberian traps for
the time interval of 265-245 Ma. The black
stars, connected by a line, are the
Sp
values average for the intervals of 10-20o.
See Figure 7 for the other symbols.

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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