LARGE SCALE PLASMA SHEET STRUCTURE- A STATISTICAL APPROACH

机译：大型等离子板结构-一种统计方法

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When Cluster crosses the magnetotail, the boundaryrnbetween the lobe and the plasma sheet is clearly definedrnby a distinct change in the ion flux. The identification ofrnthis boundary has, combined with calculations of thernneutral sheet location at the time of boundary crossings,rnbeen used to estimate the half thickness of the plasmarnsheet. A method, based on the variation in the dipole tiltrnangle, has been used to estimate the neutral sheetrnposition relative to the GSM xy-plane for magnetic localrntimes (MLT) near midnight. The plasma sheet thicknessrnwas then divided into geomagnetically active anrnnon-active periods and compared with 7 solar windrnparameters.

机译：当团簇穿过磁尾时，通过离子通量的明显变化清楚地限定了波瓣和等离子体片之间的边界。对该边界的识别与边界穿越时的中性板位置的计算相结合，用于估计等离子板的一半厚度。一种基于偶极子倾斜角变化的方法，已被用于估计午夜附近的磁性局部时间（MLT）相对于GSM xy平面的中性薄片位置。然后将等离子片的厚度分为地磁活跃和非活跃时期，并与7个太阳风参数进行比较。

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《Cluster and double star symposium》|2005年|1-5|共5页
会议地点 Noordwijk(NL);Noordwijk(NL)
作者
E. Osmundsen; A. Pedersen; E. Lucek; H. Rème;
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Dep. Of Physics, University of Oslo, P.O.Box 1048Blindern, N-0316 Oslo, Norway, e.h.osmundsen@fys.uio.no;

Dep. Of Physics, University of Oslo, P.O.Box 1048Blindern, N-0316 Oslo, Norway, arne.pedersen@fys.uio.no;

Space and Atmospheric Physic, Imperial College London, London, SW7 2BZ, UK, e.lucek@ic.ac.uk;

CESR/CNES, BP 4346, Toulouse, France, henri.reme@cesr.fr;

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LARGE SCALE PLASMA SHEET STRUCTURE- A STATISTICAL APPROACH

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