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On Special Features of Non-Thermal Solar X Radiation above 10 keV

Published online by Cambridge University Press:  12 April 2016

G. Elwert  and
E. Haug
G. Elwert
Affiliation:
Lehrstuhl für Theoretische Astrophysik, Tübingen, Germany
E. Haug
Affiliation:
Lehrstuhl für Theoretische Astrophysik, Tübingen, Germany

Extract

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The polarization and angular distribution of solar hard X radiation above 10 keV was calculated under the assumption that the X rays originate as bremsstrahlung from energetic electrons moving in a preferred direction. The source electrons are supposed to have a power-law spectrum. These conditions are to be expected in the impulsive phase of an X-ray burst. The spiral orbits of the electrons around the magnetic field lines are taken into account.

Type
Section V / The Solar Flare Plasma
Information
International Astronomical Union Colloquium , Volume 14: Special Issue: Ultraviolet and X-Ray Spectroscopy of Astrophysical and Laboratory Plasmas , November 1972 , pp. 761 - 762
Copyright
Copyright © Reidel 1972

References

Tindo, P. J., Ivanov, V. D., Mandel’ stam, S. L., and Shuryghin, A. J.: 1970, Solar Phys. 14, 204.CrossRefGoogle Scholar