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Detailed Reference Information |
Moses, S.L., Coroniti, F.V., Kennel, C.F., Kurth, W.S. and Gurnett, D.A. (1990). Comparison of plasma wave measurements in the bow shocks at Earth, Jupiter, Saturn, Uranus and Neptune. Geophysical Research Letters 17: doi: 10.1029/90GL00612. issn: 0094-8276. |
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We present plasma wave measurements from the Voyager 2 crossing of Neptune's bow shock and compare them with measurements from the bow shocks of Earth, Jupiter, Saturn and Uranus. The wave amplitudes above 0.01fp, when normalized to the solar wind ion thermal energy density at each planet, are significantly higher at the outer planets than at Earth. Despite the differences in amplitude the shock specta of all the planets can be fitted to curves of similar form in this frequency range. The total normalized electric field energy densities exhibit an exponential dependence on ion thermal Mach number. Magnetosheath wave energies are comparable at all of the planets when normalized to the downstream plasma pressure. ¿American Geophysical Union 1990 |
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Abstract |
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Keywords
Ionosphere, Plasma waves and instabilities, Interplanetary Physics, Planetary bow shocks |
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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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