Local field-aligned currents in the magnetotail and ionosphere as observed by a Cluster, Double Star, and MIRACLE conjunction

被引:10
作者
Takada, T.
Nakamura, R.
Juusola, L.
Amm, O.
Baumjohann, W.
Volwerk, M.
Matsuoka, A.
Klecker, B.
Snekvik, K.
Owen, C. J.
Fazakerley, A. N.
Frey, H. U.
Reme, H.
Lucek, E. A.
Carr, C.
机构
[1] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2298510, Japan
[2] Finnish Meteorol Inst, FIN-00101 Helsinki, Finland
[3] Austrian Acad Sci, Space Res Inst, A-8042 Graz, Austria
[4] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, London SW7 2BZ, England
[5] UCL, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
[6] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[7] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany
[8] Univ Bergen, Dept Phys & Technol, N-5007 Bergen, Norway
[9] CNRS, CESR, F-31028 Toulouse 4, France
基金
英国科学技术设施理事会;
关键词
D O I
10.1029/2007JA012759
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
During a fortuitous conjunction event observed by Cluster, Double Star TC1, and Magnetometers-Ionospheric Radars-All-Sky Cameras Large Experiment ( MIRACLE) magnetometer stations at almost the same local time, crossings of the plasma sheet boundary layer (PSBL) are observed with a 45-50 s delay between the two spacecraft located approximately 6 RE apart in X. Taking into account the different polarity of BY, Cluster curlometer current density, and the curl of the equivalent current on the ground, the associated current system resembles that of a bubble model, i.e., the propagation of a bursty bulk flow (BBF) with field-aligned currents (FACs) on each side of the flow. The presence of such local FACs associated with BBFs is supported by the time delays of PSBL crossings, corresponding weak auroral brightening, and enhancement of the ionospheric equivalent current pattern. The Cluster observation also shows different signatures between inbound and outbound crossings, i.e., electron beam direction. Such differences are considered to be caused by the relative location of the observation point from the beam ejection region, such as reconnection, and may suggest that the beam ejection region is approaching during the PSBL crossing.
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页数:8
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