Physics
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3219t&link_type=abstract
Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I
Physics
1
Scientific paper
We have studied the formation of 2.223 MeV gamma-line, arising of solar flare neutron captures on hydrogen in the photosphere and lower levels. Applying the results of calculations to the 1988 December 16 solar flare (exactly, to its third, last gamma-emission peak) enable us to deduce the enhanced density in the whole thickness of photosphere in the period of this flare like it was previously found for two other flares [6]. We also conclude that the charged particle spectrum evolve during the decay phase of corresponding charged particles acceleration process. The spectral index αT in Bessel representation changes from 0.005 up to 0.1 with the meaning 0.03 for the best approximation of whole the peak. Character of ion spectral evolution confirms previous result found by another method [1].
Gan Weiqun
Kuzhevskij Boris M.
Miroshnichenko Leonty I.
sTroitskaia Evgenya V.
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