Arguments for fundamental emission by the parametric process L → T + S in interplanetary type III bursts.

Details Arguments for fundamental emission by the parametric process L → T + S in interplanetary type III bursts. Arguments for fundamental emission by the parametric process L → T + S in interplanetary type III bursts.

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.217..281c&link_type=abstract

ESA Spec. Publ., ESA SP-207, p. 281 - 284

Physics

Interplanetary Plasma:Solar Radio Bursts, Solar Radio Bursts:Interplanetary Plasma

Scientific paper

Recent observations of low frequency ion acoustic-like waves associated with Langmuir waves present during interplanetary type III bursts lead the author to consider plasma emission mechanisms and wave processes involving ion acoustic waves. He concludes that the parametric process L → T + S may be the important emission process for the fundamental radiation of interplanetary type III bursts.

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