Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1764189 | Advances in Space Research | 2015 | 4 Pages |
Abstract
The peculiarities of time delays between the peaks of hard X-ray and microwave emissions within the framework of the trap-plus-precipitation model are studied. Using the continuity equation it has been shown that time delays strongly depend on the chromospheric evaporation in the case of the Coulomb pitch angle diffusion of trapped electrons into the loss-cone. Based on the obtained results the origin of time delays as well as the role of Coulomb collisions in flare coronal loops are discussed.
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Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Yuriy T. Tsap, Yulia G. Kopylova, Alexander V. Stepanov,