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Variation of the Solar Flare Energy Spectrum Over the 11-Year Activity Cycle

Published online by Cambridge University Press:  27 September 2017

V.V. Kasinsky  and
R.T. Sotnikova
V.V. Kasinsky
Affiliation:
SibIZMIRAN, Irkutsk, 664033, USSR

Abstract

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Based on X-ray (1-8 Å) flux data for 1977-1987, the integral spectra of solar flare energy were computed. The energy spectra were approximated by a power law N(E) α; E~n, with N being the number of flares with energy in excess of E. It is shown that the spectral index (β) varies systematically with the 11-year cycle phase.

Type
Session II: Solar Flares
Information
International Astronomical Union Colloquium , Volume 104 , Issue 2: Solar and Stellar Flares , 1989 , pp. 255 - 258
Copyright
Copyright © Kluwer 1989

References

1. Krasnobabtsev, V.I., Gershberg, R. E.: 1975, Izv. Krymsk. Astrofiz. Obs., 73, 131.Google Scholar
2. Gershberg, R. E.: 1988 XXXII Congresso della Soc. Astron Ital., 4-7 May 1988, Catania Preprint No. 9/1988.Google Scholar
3. Gershberg, R. E., Magilevsky, E. I., Obridko, V. N.: 1987, Kinematika i Fizika Nebesnykh Tel. 3, No. 5, 3.Google Scholar
4. Hudson, H.S.: 1978 Solar Phys. 57, 237.Google Scholar