Plasma diagnostics of the solar corona using decimetric radio waves (review)

Details Plasma diagnostics of the solar corona using decimetric radio waves (review) Plasma diagnostics of the solar corona using decimetric radio waves (review)

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994r%26qe...37..525b&link_type=abstract

Radiophysics and Quantum Electronics, Volume 37, Issue 7, pp.525-532

Physics

Scientific paper

The solar corona is a very dynamic plasma on time scales down to a few tens of microseconds. The various emissions at decimetric wavelength are briefly reviewed. Several of them seem to be caused by energetic (non-thermal) electrons accelerated in flares or flare-like processes releasing free magnetic energy. The use of decimetric radiation as diagnostics of the acceleration process, the ambient plasma, and the non-thermal particles requires a solid understanding of the emission process. Although we are still far from this in most cases, some information can already be derived from the observations.

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