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


Figure 2. The dependence of the flow in the ``long wave'' (0.1–0.8 nm) band of the flux in the ``short'' (0.05–0.4 nm) GOES satellite data for February 1992. Along the coordinate axes on a logarithmic scale flow units are shown above W m$^{-2}$.


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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.


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