X-Ray and HαEmission of the 20 Aug 2002 Flare*

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Solar Magnetic Phenomena

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 320))

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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