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Formation of anisotropic distributions of mildly relativistic electrons in flaring loops
Published online by Cambridge University Press: 01 September 2008
Abstract
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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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- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 4 , Symposium S257: Universal Heliophysical Processes , September 2008 , pp. 323 - 328
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- Copyright © International Astronomical Union 2009
References
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