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Detailed Reference Information |
Kainer, S. and MacDowall, R.J. (1996). A ring beam mechanism for radio wave emission in the interplanetary medium. Journal of Geophysical Research 101: doi: 10.1029/95JA02026. issn: 0148-0227. |
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Radio wave emission sources in the interplanetary medium (IPM) include type II and type III radio bursts and emission from planetary bow shock regions. The presence of electron beams in a range of energies suggests the possibility of a ring beam-plasma interaction as a mechanism for the generation of radio waves at both the fundamental and the second harmonic of the background electron plasma frequency. In this paper, ring beam-plasma interactions are simulated for the conditions of the IPM, &ohgr;e/&OHgr;e=100 to 200. In these simulations, the ring beam-plasma interaction couples the electrostatic Langmuir waves at the fundamental plasma frequency to electromagnetic waves; harmonic radiation is produced by an electrostatic trapped electron instability. Mode conversion processes permit the Z mode radiation generated through these instabilities to be converted to the X mode. Examination of both theory and observations suggests the ring beam-plasma interaction as a candidate for many of the radio phenomena in the IPM. ¿ American Geophysical Union 1996 |
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Abstract |
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Keywords
Interplanetary Physics, Planetary bow shocks, Interplanetary Physics, Plasma waves and turbulence, Solar Physics, Astrophysics, and Astronomy, Radio emissions, Space Plasma Physics, Waves and instabilities |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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