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Detailed Reference Information |
Terasawa, T., Kasaba, Y., Tsubouchi, K., Mukai, T., Saito, Y., Frank, L.A., Paterson, W.R., Ackerson, K., Matsumoto, H., Kojima, H., Matsui, H., Larson, D., Lin, R., Phan, T., Steinberg, J., McComas, D., Skoug, R., Fujimoto, M., Hoshino, M. and Nishida, A. (2000). GEOTAIL observations of anomalously low density plasma in the magnetosheath. Geophysical Research Letters 27: doi: 10.1029/2000GL000087. issn: 0094-8276. |
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During the anomalously low density solar wind interval of May 1999, GEOTAIL was in the magnetosheath for ~37 hours after making an inbound crossing of the expanding bow shock at ~80 RE upstream of its nominal position. Comparison among data sets obtained from GEOTAIL (magnetosheath), WIND (near upstream-bow shock), and ACE (far upstream) reveals several unique features: Firstly, during the interval of 1430--1530 UT on 11 May, we observed both in the solar wind and magnetosheath double-peaked protons with a peak separation of 250--300 km/s, which was close to the local Alfv¿n velocity during the event. Secondly, we observed extremely strong strahl electrons both in the solar wind and magnetosheath during the interval of 0600--2100 UT on 11 May 1999. We present an overview of the GEOTAIL observations, and discuss their physical significance. ¿ 2000 American Geophysical Union |
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Abstract |
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Keywords
Interplanetary Physics, Solar wind plasma, Magnetospheric Physics, Solar wind/magnetosphere interactions |
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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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