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On Two Mechanisms of X-Ray Generation in Comets

Published online by Cambridge University Press:  12 April 2016

S. Ibadov
S. Ibadov*
Affiliation:
Institute of Astrophysics, 734670 Dushanbe USSR

Abstract

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The intensity of solar X-radiation scattered by a comet is calculated and compared to the proper X-radiation of the comet due to impacts of cometary and interplanetary dust particles. Detection of X-radiation of dusty comets at small heliocentric distances (R ≤ 1 a.u.) is found to be an indicator of high-temperature plasma generation as result of grain collisions.

Type
VI. Dust – Plasma Interactions
Information
International Astronomical Union Colloquium , Volume 85: Properties and Interactions of Interplanetary Dust , 1985 , pp. 365 - 368
Copyright
Copyright © Reidel 1985

References

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