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Electron acceleration in solar noise storms View all abstracts by submitter

Prasad Subramanian   Submitted: 2007-03-27 00:38

We present an up-to-date review of the physics of electron acceleration in solar noise storms. We describe the observed characteristics of noise storm emission, emphasizing recent advances in imaging observations. We briefly describe the general method ology of treating particle acceleration problems and apply it to the specific problem of electron acceleration in noise storms. We dwell on the issue of the efficiency of the overall noise storm emission process and outline open problems in this area.

Authors: Prasad Subramanian
Projects: None

Publication Status: Review article, to appear in Asian J. of Physics, 2007
Last Modified: 2007-03-27 12:33
Go to main E-Print page  Generalized Squashing Factors for Covariant Description of Magnetic Connectivity in the Solar Corona  Electron acceleration in a post-flare decimetric continuum source  Edit Entry  Download Preprint  Submitter's Homepage Delete Entry 

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