Radio Spectral Diagnostics

Gary, Dale E.; Hurford, G. J.

doi:10.1007/1-4020-2814-8_4

Radio Spectral Diagnostics

Dale E. Gary²⁵ &
G. J. Hurford²⁶

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Part of the Astrophysics and Space Science Library book series (ASSL,volume 314)

Abstract

We review solar radio emission from the perspective of imaging spectroscopy. Radio emission mechanisms differ in their spectral properties, which can be used to determine parameters of the emitting particles and the ambient solar atmosphere in the emitting volume. After generation, the propagation of radiation in the solar atmosphere leads to changes in the spectrum that can be exploited to gain further information about the atmospheric parameters along the line of sight.

Keywords

Radio Emission
Imaging Spectroscopy
Solar Atmosphere
Solar Radio Emission
Gyrosynchrotron Emission

These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Authors and Affiliations

Center for Solar-Terrestrial Research, New Jersey Institute of Technology, Newark, NJ, 07102, USA
Dale E. Gary
Space Sciences Laboratory, University of California, Berkeley, CA, 94720
G. J. Hurford

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Dale E. Gary
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G. J. Hurford
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Editors and Affiliations

Center for Solar-Terrestrial Research, New Jersey Institute of Technology, Newark, N.J., USA
Dale E. Gary
National Solar Observatory, Tucson, AZ, USA
Christoph U. Keller

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Gary, D.E., Hurford, G.J. (2004). Radio Spectral Diagnostics. In: Gary, D.E., Keller, C.U. (eds) Solar and Space Weather Radiophysics. Astrophysics and Space Science Library, vol 314. Springer, Dordrecht. https://doi.org/10.1007/1-4020-2814-8_4

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DOI: https://doi.org/10.1007/1-4020-2814-8_4
Publisher Name: Springer, Dordrecht
Print ISBN: 978-1-4020-2813-7
Online ISBN: 978-1-4020-2814-4
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