Can spontaneously emitted Langmuir waves account for type III solar radio bursts

Details Can spontaneously emitted Langmuir waves account for type III solar radio bursts Can spontaneously emitted Langmuir waves account for type III solar radio bursts

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976pasau...3...43m&link_type=abstract

(Astronomical Society of Australia, Annual General Meeting, 10th, Sydney, Australia, May 12-14, 1976.) Astronomical Society of A

Astronomy and Astrophysics

Astronomy

1

Electrostatic Waves, Magnetohydrodynamic Stability, Spontaneous Emission, Type 3 Bursts, Harmonic Radiation, Infrared Spectra, Plasma Dynamics, Ubv Spectra, Wave Amplification

Scientific paper

It is assumed that two-stream instability does not develop in the solar atmosphere and that the only Langmuir waves generated by the stream are those generated through spontaneous emission. The question whether the observed radio emission (type III bursts) can be accounted for in terms of the spontaneously emitted Langmuir waves is examined. It is concluded that the Langmuir waves probably cannot account for type III emission, and that this inadequacy is due to the relative inefficiency of their conversion into transverse waves.

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