Physics
Scientific paper
Jun 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979soph...62..359s&link_type=abstract
Solar Physics, vol. 62, June 1979, p. 359-373.
Physics
11
Energy Transfer, Plasma Diagnostics, Plasma Turbulence, Solar Flares, Integral Equations, Plasma Acceleration, Plasma Waves, Stellar Models, Wave Equations
Scientific paper
The possibility is investigated that the plasma turbulence used in many recent models of the primary energy release and acceleration in solar flares should be detectable by radiation near the fundamental and second harmonic of the plasma frequency. Formulae are derived for fundamental emission due to the combination of ion-acoustic and Langmuir plasma turbulence and for second harmonic emission due to the combination of two Langmuir waves. These results are applied to recent primary energy release and acceleration models which shows that either such radiation should be detectable and possibly distinguishable with suitable microwave interferometers or that its absence places fairly stringent constraints on the possible level of Langmuir or Langmuir and ion-acoustic waves in these models.
Smith Donelson F.
Spicer Daniel S.
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