Analysis of the physical conditions in a strong X-ray flare |
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| Authors: | B. Sylwester J. Sylwester |
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| Affiliation: | Space Research Centre, Polish Academy of Sciences, Wroclaw, Poland;Astronomical Institute, Wroclaw University, Wroclaw, Poland;Astronomical Institute of the Czechoslovak Academy of Sciences, Ond?ejov Observatory, Czechoslovakia |
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| Abstract: | ![]()
The temperature distribution of the hot plasma emission measure in a large but slowly developing flare has been investigated using the following data obtained from the INTERCOSMOS 4 satellite: (1) the X - ray spectra in the range 1.7 – 1.9 Å, (2) the hard X - ray fluxes in the range 10 – 40 keV. It has been found that all the data can be explained by a consistent thermal model of the emitting region. |
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