Pitch angle distribution of electrons generating hard X-ray emission in flare loops

Details Pitch angle distribution of electrons generating hard X-ray emission in flare loops Pitch angle distribution of electrons generating hard X-ray emission in flare loops

Feb 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976azh....53..215m&link_type=abstract

Astronomicheskii Zhurnal, vol. 53, no. 1, 1976, p. 215-217. In Russian.

Astronomy and Astrophysics

Astronomy

1

Angular Distribution, Electron Distribution, Plasma Interactions, Solar Flares, Solar Magnetic Field, Solar X-Rays, Electrostatic Waves, Magnetic Field Configurations, Plasma Oscillations

Scientific paper

The author examines the nonlinear interaction of Langmuir oscillations with magnetic field fluctuations in flare loops in order to shed light on the possible electron pitch angle distribution of electrons whose braking may account for the hard X-ray emission detected during the early stage of solar flares. In the case of an anisotropic pitch angle distribution, the interaction can lead to a considerable increase in the amplitude of magnetic field fluctuations, an effect which could be observed with current instruments. The interaction is absent when the pitch angle distribution is isotropic.

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