On the heliocentric distance dependence of plasmon emission in type III bursts

Details On the heliocentric distance dependence of plasmon emission in type III bursts On the heliocentric distance dependence of plasmon emission in type III bursts

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....94..219d&link_type=abstract

Astronomy and Astrophysics, vol. 94, no. 2, Feb. 1981, p. 219-225.

Astronomy and Astrophysics

Astrophysics

4

Plasma-Particle Interactions, Plasmons, Solar Wind, Type 3 Bursts, Astronomical Models, Electron Clouds, Random Processes, Wave Interaction

Scientific paper

The paper reports on the space and time dependence of plasmon emission in type III solar radio bursts. This dependence is inferred from four one-dimensional models of wave-particle interaction: free-streaming beam (homogeneous plasma); effects of random density fluctuations of the background plasma; quasi-linear beam relaxation; beam stabilization by nonlinear wave-wave interactions. The plasma wave energy density is shown in every case to become negligibly small as the heliocentric distance increases. Implications for low-frequency type III bursts of this result are discussed as a function of the beam characteristic parameters.

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