Postburst increase of solar brightness temperature at decameter wavelengths

Details Postburst increase of solar brightness temperature at decameter wavelengths Postburst increase of solar brightness temperature at decameter wavelengths

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kfnt....6...87b&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 6, Jan.-Feb. 1990, p. 87-89. In Russian.

Physics

Brightness Temperature, High Energy Electrons, Plasma Turbulence, Solar Corona, Solar Flares, Decametric Waves, Isotropic Turbulence

Scientific paper

It is shown that, after a high energy electron beam passes through the
solar corona, an elevated level of isotropic plasma turbulence arises.
It is suggested that this may explain the large variations of brightness
temperature observed at decameter wavelengths during periods of high
solar activity.

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