Generation of solar type III bursts at the second harmonic

Paul J Kellogg, R. P. Lin

Research output: Contribution to journalArticle

1 Citation (Scopus)

Abstract

Using the data from our experiments on the IMP-6 (Explorer 43) satellite, we have examined over 200 type III bursts at kilometric wavelengths, including 16 bursts which were accompanied by >18 keV electron events with sharp onsets, in a search for the electrostatic waves which, according to theory, should be the primary source of type III bursts. No electrostatic waves of sufficient intensity to generate the type III bursts by any of the wave-wave scattering theories which produce the second harmonic of the plasma frequency, have been found.

Original languageEnglish (US)
Number of pages1
JournalSolar Physics
Volume46
Issue number2
DOIs
StatePublished - Feb 1 1976

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Explorer 43 satellite
bursts
harmonics
electrostatic waves
wave scattering
plasma frequencies
wavelength
plasma
electron
experiment
wavelengths
electrons

Cite this

Generation of solar type III bursts at the second harmonic. / Kellogg, Paul J; Lin, R. P.

In: Solar Physics, Vol. 46, No. 2, 01.02.1976.

Research output: Contribution to journalArticle

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