Reid, H. A. S. and Ratcliffe, H. (2014) A review of solar type III radio bursts. Research in Astronomy and Astrophysics, 14(7), pp. 773-804. (doi: 10.1088/1674-4527/14/7/003)
Full text not currently available from Enlighten.
Publisher's URL: http://dx.doi.org/10.1088/1674-4527/14/7/003
Abstract
Solar type III radio bursts are an important diagnostic tool in the understanding of solar accelerated electron beams. They are a signature of propagating beams of nonthermal electrons in the solar atmosphere and the solar system. Consequently, they provide information on electron acceleration and transport, and the conditions of the background ambient plasma they travel through. We review the observational properties of type III bursts with an emphasis on recent results and how each property can help identify attributes of electron beams and the ambient background plasma. We also review some of the theoretical aspects of type III radio bursts and cover a number of numerical efforts that simulate electron beam transport through the solar corona and the heliosphere.
Item Type: | Articles |
---|---|
Status: | Published |
Refereed: | Yes |
Glasgow Author(s) Enlighten ID: | Ratcliffe, Miss Heather and Reid, Dr Hamish |
Authors: | Reid, H. A. S., and Ratcliffe, H. |
College/School: | College of Science and Engineering > School of Physics and Astronomy |
Journal Name: | Research in Astronomy and Astrophysics |
Publisher: | IOP Publishing |
ISSN: | 1674-4527 |
University Staff: Request a correction | Enlighten Editors: Update this record