RUSSIAN JOURNAL OF EARTH SCIENCES VOL. 9, ES3004, doi:10.2205/2007ES000276, 2007

2007ES000276-fig05.html
Figure 5. The dependence of the background (without flares) X-ray radiation spectra of active regions on the sunspot number illustrating the magnetic heating of the solar atmosphere in October 2003, correspondingly at the beginning (1, 3, and 5 October), in the middle (11, 14, and 17 October), and at the end (24, 30, and 31 October). The X-ray spectrometer RPS-1.

RJES

Citation: Kuznetsov, V. D. (2007), From the geophysical to heliophysical year: The results of the CORONAS-F project, Russ. J. Earth Sci., 9, ES3004, doi:10.2205/2007ES000276.

Copyright 2007 by the Russian Journal of Earth Sciences
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