Coronal Langmuir turbulence and the quasi-stable accelerating sources

Details Coronal Langmuir turbulence and the quasi-stable accelerating sources Coronal Langmuir turbulence and the quasi-stable accelerating sources

Mar 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980acasn..21...20s&link_type=abstract

Acta Astronomica Sinica, vol. 21, Mar. 1980, p. 20-26. In Chinese, with abstract in English.

Astronomy and Astrophysics

Astronomy

3

Microwave Emission, Particle Acceleration, Plasma Turbulence, Solar Corona, Solar Radio Bursts, Energetic Particles, High Energy Interactions, Plasma-Particle Interactions, Turbulence Effects, Very High Frequencies

Scientific paper

It is suggested that there may be quasi-stable Langmuir turbulence in
the corona in an active region. It is suggested that the enhanced radio
emission meter-wave type I bursts would be the electromagnetic emission
produced by this turbulence. The acceleration of particles caused by
such turbulence and some phenomena of observation are discussed.

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