Author:
Melnikov Victor F.,Gorbikov Sergey P.,Pyatakov Nikolai P.
Abstract
AbstractIn 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.
Publisher
Cambridge University Press (CUP)
Subject
Astronomy and Astrophysics,Space and Planetary Science
Cited by
4 articles.
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1. Diagnostics of Accelerated Electrons Anisotropy from Solar Hard X-rays;Journal of Physics: Conference Series;2019-11-01
2. Observations and Explanations of MW Emissions in Solar Flaring Loops;Solar Flare Loops: Observations and Interpretations;2018
3. Theory of MW Emissions of Solar Flaring Loops;Solar Flare Loops: Observations and Interpretations;2018
4. Introduction;Solar Flare Loops: Observations and Interpretations;2018