Solar wind control of density and temperature in the near-Earth plasma sheet: WIND/GEOTAIL collaboration

被引:241
作者
Terasawa, T
Fujimoto, M
Mukai, T
Shinohara, I
Saito, Y
Yamamoto, T
Machida, S
Kokubun, S
Lazarus, AJ
Steinberg, JT
Lepping, RP
机构
[1] TOKYO INST TECHNOL,DEPT EARTH & PLANETARY SCI,MEGURO KU,TOKYO 152,JAPAN
[2] INST SPACE & ASTRONAUT SCI,SAGAMIHARA,KANAGAWA 229,JAPAN
[3] KYOTO UNIV,DEPT GEOPHYS,SAKYO KU,KYOTO 606,JAPAN
[4] MIT,CTR SPACE RES,CAMBRIDGE,MA 02139
[5] NASA,GODDARD SPACE FLIGHT CTR,EXTRATERR PHYS LAB,GREENBELT,MD 20771
[6] NAGOYA UNIV,SOLAR TERR ENVIRONM LAB,TOYOKAWA,AICHI 442,JAPAN
关键词
D O I
10.1029/96GL04018
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
A statistical survey of GEOTAIL observations reveals the following. properties of the near-Earth plasma sheet (-15 < X-GSM' < -50 Re): During the periods when the northward IMF dominates, (1) the plasma sheet becomes significantly cold and dense, (2) the best correlations between the plasma, sheet and the IMF parameters occur when the latter quantities are averaged over 9(-4)(+3) hours prior to the plasma sheet observations, and (3) temperatures diminish and densities increase near the dawn and dusk flanks of the plasma sheet. We suggest that during prolonged northward IMF periods (similar to several hours) there is a slow diffusive transport of the plasma from the solar wind into the plasma, sheet through the the magnetotail flanks.
引用
收藏
页码:935 / 938
页数:4
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