RUSSIAN JOURNAL OF EARTH SCIENCES VOL. 10, ES3005, doi:10.2205/2007ES000247, 2008

Figure 3. The solar situation during the extreme solar flare of
28 October 2003; upper row, left: the white-light Sun with
sunspot groups (SOHO); upper row, right: the Sun in the extreme
ultraviolet line
l = 195 Å at the flare maximum
(SOHO); lower row, left: coronal mass ejection from the flare
(SOHO C2 coronagraph); lower row, right: the same coronal mass
ejection at a greater distance from the Sun (SOHO C3 coronagraph).

Citation: Ishkov, V. N. (2008), Solar geoeffective phenomena: Impact on the near-Earth space and the opportunity to forecast, Russ. J. Earth Sci., 10, ES3005, doi:10.2205/2007ES000247.
Copyright 2008 by the Russian Journal of Earth Sciences
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