The hyperfine time structure of the microwave emission of the solar flare on March 12, 1989

Details The hyperfine time structure of the microwave emission of the solar flare on March 12, 1989 The hyperfine time structure of the microwave emission of the solar flare on March 12, 1989

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pazh...16..247s&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 16, March 1990, p. 247-252. In Russian. In Russian.

Astronomy and Astrophysics

Astrophysics

5

Microwave Emission, Solar Flares, Solar Radio Bursts, Brightness Temperature, Electrostatic Waves, Temporal Distribution

Scientific paper

An analysis of the hyperfine time structure of the March 12, 1989 solar radio burst is presented using observations from the 2.85-GHz radiometer at the Crimean Astrophysical Observatory. It is shown that the characteristics of the millisecond spikes can be explained in terms of nonlinear plasma emission. The Langmuir wave turbulence level is found to be W/nT = 4 x 10 to the -7th, and the electron density in the emission source is shown to be 2.5 x 10 to the 10th/cu cm.

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