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Detailed Reference Information |
Winterhalter, D. and Kivelson, M.G. (1988). Observations of the earth’s bow shock under high mach number/high plasma beta solar wind conditions. Geophysical Research Letters 15: doi: 10.1029/88GL03373. issn: 0094-8276. |
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Using 221 observations of the earth's bow shock by ISEE-1 we investigate the magnetic field characteristics of the shock as a function of Mach number and plasma beta. We find that immediately behind the overshoot of the shock large amplitude waves develop preferentially with increasing Alfv¿n Mach number and/or plasma beta. Their probability of occurrence is very high in the parallel regime (&thgr;BN≤10¿), and declines to near zero probability when &thgr;BN reaches 75¿. It is estimated that approximately 10% of the total solar wind energy density is dissipated by these waves. ¿ American Geophysical Union 1988 |
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Abstract |
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Keywords
Space Plasma Physics, Shock waves |
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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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