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Timescale for the formation of the cold‐dense plasma sheet: A case study
Author(s) -
Wing Simon,
Johnson Jay R.,
Fujimoto Masaki
Publication year - 2006
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/2006gl027110
Subject(s) - plasma sheet , geology , plasma , atmospheric sciences , climatology , environmental science , geophysics , meteorology , physics , magnetosphere , nuclear physics
The timescale for the formation of cold‐dense plasma sheet ions was investigated with an event in which the interplanetary magnetic field (IMF) was northward for almost one day. The plasma sheet dawn and dusk flanks appear to reach cold dense states (n > 1 cm −3 ; T < 2 keV) within a few hours after IMF northward turning. Closer to the center (midnight meridian), the ion temperatures reach < 2 keV within a few hours of IMF northward turning, but the ion densities do not reach above 1 cm −3 for at least ∼8 hours after IMF northward turning. The connection between solar wind ions and plasma sheet cold‐component ions is demonstrated. The plasma sheet dawn flank ions appear to lag the solar wind ions by about 3 hours. This study confirms the previous statistical results: (a) the densification of the plasma sheet can be attributed to the influx of the cold‐component (magnetosheath/solar wind origin) ions; and (b) the cooling of the plasma sheet can be attributed not only to the influx of the solar wind ions, but also to the cooling of the hot components. Order of magnitude calculations of the plasma sheet filling rate from reconnection and diffusion suggest that both entry mechanisms could result in roughly comparable filling rates. Hence, the dawn‐dusk asymmetries would be key in distinguishing the roles of the various proposed entry mechanisms.