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Formation of anisotropic distributions of mildly relativistic electrons in flaring loops

Published online by Cambridge University Press:  01 September 2008

Victor F. Melnikov ,
Sergey P. Gorbikov  and
Nikolai P. Pyatakov
Victor F. Melnikov
Affiliation:
Radiophysical Research Institute, B.Pecherskaya 25, 603950, Nizhny Novgorod, Russia email: melnikov@nirfi.sci-nnov.ru
Sergey P. Gorbikov
Affiliation:
Radiophysical Research Institute, B.Pecherskaya 25, 603950, Nizhny Novgorod, Russia email: melnikov@nirfi.sci-nnov.ru
Nikolai P. Pyatakov
Affiliation:
Radiophysical Research Institute, B.Pecherskaya 25, 603950, Nizhny Novgorod, Russia email: melnikov@nirfi.sci-nnov.ru
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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.

Keywords

Sun: flaresSun: radio radiationacceleration of particles

Information

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S257: Universal Heliophysical Processes , September 2008 , pp. 323 - 328
Copyright
Copyright © International Astronomical Union 2009

References

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