Formation of anisotropic distributions of mildly relativistic electrons in flaring loops

Details Formation of anisotropic distributions of mildly relativistic electrons in flaring loops Formation of anisotropic distributions of mildly relativistic electrons in flaring loops

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009iaus..257..323m&link_type=abstract

Universal Heliophysical Processes, Proceedings of the International Astronomical Union, IAU Symposium, Volume 257, p. 323-328

Astronomy and Astrophysics

Astronomy

Sun: Flares, Sun: Radio Radiation, Acceleration Of Particles

Scientific paper

In this paper we show that different locations of acceleration/injection sites in flaring loops may produce very different types of pitch-angle distributions of accelerated electrons and, as a consequence, different spatial, spectral and polarization properties of the loop microwave emission. It is shown that these properties can be detected using spatially resolved microwave observations of specific flaring loops and be used to choose the most suitable electron acceleration model.

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