Abstract
An analysis of the August 20, 2002 flare using RHESSI, Hα, and radio observations is presented. Radio data in the decimetric frequency range showed a type IIId (relativistic) burst at the time of the X-ray maximum. At this time a very flat (γphot = 1.8) X-ray spectrum was measured. Fitted double power-law spectra in the thick-target model revealed an increase of the low energy cuto in the electron spectrum that rose to as high as 81 keV. This cutoff evolution is interpreted as a possible gap in energies of electrons injected into the X-ray thick-target source and those of the background plasma. Fast changes of Ha intensities were found to be located away from the X-ray sources in the beginning of the Ha flare.
This paper is a short version of Kašparová et al. (2004)
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Kašparová, J., Karlický, M., Schwartz, R., Dennis, B. (2005). X-Ray and HαEmission of the 20 Aug 2002 Flare*. In: Hanslmeier, A., Veronig, A., Messerotti, M. (eds) Solar Magnetic Phenomena. Astrophysics and Space Science Library, vol 320. Springer, Dordrecht. https://doi.org/10.1007/1-4020-2962-4_12
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DOI: https://doi.org/10.1007/1-4020-2962-4_12
Publisher Name: Springer, Dordrecht
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