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Detailed Reference Information |
Mozer, F.S., Hayakawa, H., Kokubun, S., Nakamura, M., Okada, T., Yamamoto, T. and Tsuruda, K. (1994). Direct entry of dense flowing plasmas into the distant tail lobes. Geophysical Research Letters 21: doi: 10.1029/94GL01610. issn: 0094-8276. |
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Electric field, magnetic field, and spacecraft potential measurements on the Geotail satellite have confirmed earlier observations of relatively dense flowing plasmas in the magnetotail lobes. Within these flowing plasmas, density discontinuities of factors of 2 to 4 were observed. At least 15 of the 18 magnetopause crossings that occurred during a 24-hour interval when the spacecraft was at GSM coordinates near X=-140 Re, Y=0, and Z=15 Re, were rotational discontinuities across which the magnetosheath plasma had direct entry into the tail lobes. Within the lobes near the rotational discontinuities, the spacecraft typically crossed a second boundary at which the plasma density decreased from its magnetosheath value by a typical factor of 1.5 to 3 while the magnetic field strength and flow speed increased. Equatorward of this density discontinuity, the plasma density and flow remained appreciable. At least 2 of the 18 magnetopause crossings may have been tangential discontinuities across which the density and magnetic field strength both changed. Within the lobes near these tangential discontinuities, significant densities of flowing plasma were observed. Since 11 of the 18 discontinuities were crossed within a time interval of less than 7 seconds, the boundary current layer was well-defined and very thin. ¿American Geophysical Union 1994 |
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BACKGROUND DATA FILES |
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Abstract |
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Keywords
Magnetospheric Physics, Electric fields, Magnetospheric Physics, Magnetopause, cusp, and boundary layers |
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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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