Cluster observations of earthward flowing plasmoid in the tail

被引:137
|
作者
Zong, QG [1 ]
Fritz, TA
Pu, ZY
Fu, SY
Baker, DN
Zhang, H
Lui, AT
Vogiatzis, I
Glassmeier, KH
Korth, A
Daly, PW
Balogh, A
Reme, H
机构
[1] Boston Univ, Ctr Space Phys, Boston, MA 02215 USA
[2] Univ Colorado, Atmospher & Space Phys Lab, Boulder, CO 80303 USA
[3] Peking Univ, ISPAT, Beijing 100871, Peoples R China
[4] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
[5] Tech Univ Braunschweig, Inst Geophys & Extraterr Phys, D-3300 Braunschweig, Germany
[6] Max Planck Inst Aeron, D-37191 Katlenburg Lindau, Germany
[7] Univ London Imperial Coll Sci Technol & Med, Space & Atmospher Phys Grp, London SW7 2BW, England
[8] Ctr Etud Spatiale Rayonnements, Toulouse 4, France
关键词
D O I
10.1029/2004GL020692
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
The energetic electrons and ions embedded in Earthward-moving plasmoid structures have been observed. These plasmoids are associated with a rotational local B-z component (bi-polar) signature. Energetic electrons are found to be confined in a smaller spatial region than ions inside the plasmoid. Energetic ions and electrons seem to be a good indicator for the structure boundary. The fleet of Cluster spacecraft cross the plasmoid structure in a "first entry, last out'' order (Note: when spacecraft cross a planar discontinuity, e.g. magnetopause, they will be in "first entry, first out'' order). This documents the fact that the plasmoid has a non-planar nested structure. The large separation distance (around 1 R-E) of the Cluster satellites in October 2002 is an advantage to provide constraints on the size and shape of the plasmoid structure of interest. In addition, the plasmoid (with closed field lines) should preserve the ion composition information where it is formed. The ion composition observed in the plasmoid shows significantly lower O and He than in the ambient plasma. This implies few heavy ions are involved in the reconnection process where the plasmoid is formed. Multiple flux ropes/plasmoids observation presented in this paper can be interpreted as strong evidence for multiple X-lines.
引用
收藏
页码:L188031 / 4
页数:4
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