Brightness temperature of solar radio noise storm continua

Details Brightness temperature of solar radio noise storm continua Brightness temperature of solar radio noise storm continua

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...127..132k&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 127, no. 1, Oct. 1983, p. 132-134.

Astronomy and Astrophysics

Astrophysics

14

Brightness Temperature, Noise Temperature, Solar Radio Emission, Solar Storms, Electron Distribution, Electrostatic Waves, Radiative Transfer

Scientific paper

The authors have measured the brightness temperature of 19 noise storms
continua at 169 MHz, chosen among the most intense events. The results
suggest the existence of an upper limit, the value of which is in
agreement with the theoretical predictions of theories involving
generation of Langmuir waves by isotropic electron distributions.

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