Volume 415, Number 1, February III 2004
|Page(s)||377 - 389|
|Published online||03 February 2004|
Solar impulsive soft X–ray brightenings and their connection with footpoint hard X–ray emission sources
Astronomical Institute, University of Wrocław, ul. Kopernika 11, 51-622 Wrocław, Poland
Corresponding author: T. Mrozek, firstname.lastname@example.org
Accepted: 5 September 2003
We have investigated 46 solar flares showing impulsive soft X–ray brightenings in footpoints. To obtain their main observational characteristics we used the Yohkoh/SXT images. The results are presented in the form of normalized histograms showing the distribution of the characteristics. For 18 flares it has been possible to make a quantitative comparison between the footpoint response in soft X–ray images and in hard X–ray images. The latter have been derived from the Yohkoh/HXT and reconstructed using the MEM procedure. The evident correlation between these two kinds of response, as well as between the deposited energies, strongly supports a common physical cause, namely non-thermal electron beams. We present evidence that in the impulsive phase the chromospheric evaporation is driven mainly by low-energy non-thermal electrons. We show that the low-energy cut-off energy in hard X–ray photon fluxes may vary from flare to flare and may even vary during a given flare.
Key words: Sun: corona / flares / X–rays, gamma rays
© ESO, 2004
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