RUSSIAN JOURNAL OF EARTH SCIENCES, VOL. 12, ES5001, doi:10.2205/2012ES000520, 2012

Figure 1. Differential spectra of $X$-ray flares of different intensity [Nusinov and Chulankin, 1997]. Due to technical difficulties of measurement in this range is expected in the framework of geophysical monitoring (SHM) to carry on the first $X$-ray flux measurements in the field of 0.05–0.4 nm implemented much easier. This leads to the need to convert the measured flare flows in 0.05–0.4 nm in a flow of 0.1–0.8 nm, which is based on the basis of classification of solar flares and analysis of their effects in the ionosphere and upper atmosphere (see, e.g. [Nusinov and Chulankin, 1997]).

 
Citation: Nusinov A. A., V. V. Katyushina (2012), Classification of solar X-ray flares on X-ray measurements on board geostationary satellites ``Elektro'', Russ. J. Earth Sci., 12, ES5001, doi:10.2205/2012ES000520.
 

Copyright 2012 by the Geophysical Center RAS.

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