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Electrons and X-Ray Emission of Solar Flares

Published online by Cambridge University Press:  19 July 2016

V. G. Kurt
V. G. Kurt*
Affiliation:
Institute of Nuclear Pnysics Moscow State University P. B. 119899 Leninskie Gory, Moscow, USSR

Abstract

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A statistical analysis of solar flare X-rays and interplanetary particle fluxes, measured onboard VENERA-13, 14 Spacecraft, was performed. The correlation of fluences for different manifestations of solar flares is strong, especially for fast electrons and hard and soft X-ray emissions. Frequency dependence on fluence value ϵi for practically all Kinds of solar flare emission can be described by power law ν (ϵ > ϵO) ∼ ϵ−0.45±0.15 which does not change significantly with solar activity. For different Hα flare importances the values of ϵi were obtained. It is proposed that appearance of certain energy flare frequency is strongly dependent on some scale factor.

Type
VIII. Solar Flares
Information
Symposium - International Astronomical Union , Volume 142: Basic Plasma Processes on the Sun , 1990 , pp. 409 - 413
Copyright
Copyright © Kluwer 1990 

References

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