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Detailed Reference Information |
Gomberoff, L., Gnavi, G. and Gratton, F.T. (1996). Minor heavy ion electromagnetic beam–plasma interactions in the solar wind. Journal of Geophysical Research 101: doi: 10.1029/96JA00546. issn: 0148-0227. |
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It is shown that the velocity threshold of the right-hand-polarized ion-ion resonant instability decreases with decreasing gyrofrequency values of the beam ions, and also, the system can become unstable for very small beam concentrations. In order to illustrate the results, a plasma consisting of a proton background and a very tenuous O+ ion beam is considered. It is shown that for an ion beam of nO+/np=10-4, the threshold velocity is VO+~1.36VA (VA is the Alfv¿n velocity), and the maximum growth rate is of the order of 10-3&OHgr;p (&OHgr;p is the proton gyrofrequency). We apply these results to high-speed solar-wind-type plasmas consisting of a proton background, an alpha particle beam, and a beam of O+ ions. It is also shown that the presence of alpha particles reduces the velocity instability threshold of the O+-p resonant instability. ¿ American Geophysical Union 1996 |
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Abstract |
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Keywords
Space Plasma Physics, Waves and instabilities, Interplanetary Physics, Solar wind plasma |
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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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