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- W1642920203 abstract "The structure of the plasma sheet under northward IMF is studied by data from the Geotail spacecraft. The plasma sheet is known to become cold and dense (T < 2 keV, n > 1 cm-3) during extended northward IMF periods. We show that such cold-dense ions (CDIs) appear at itYgsm>10 Re, that is, 10Reoff the tail axis to both flanks. CDIs on the dawnside have higher temperatures and some reach the upper-limit of 2 keV that we use to select CDIs. These CDIs having the highest temperature are distributed at the dawnside plasma sheet inner-edge (R < 15 Re) and is connected to the hot-dense ions (HDIs: T >2 keV, n >1 cm-3) in the further inner region. A survey shows that HDIs under nominal solar wind dynamic pressure appear mostly in the dawnside inner-magnetosphere during extended northward IMF intervals. Both results point to the idea that HDIs are the inner-magnetosphere extension of dawnside CDIs, while such a partner to the duskside CDIs cannot be identified. This structure of the plasma sheet suggests that there is significant dawn-dusk asymmetry in heating and transport in the magnetotail under northward IMF." @default.
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- W1642920203 date "2005-01-01" @default.
- W1642920203 modified "2023-10-18" @default.
- W1642920203 title "The Structure of the Plasma Sheet Under Northward IMF" @default.
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- W1642920203 doi "https://doi.org/10.1016/s0964-2749(05)80004-6" @default.
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