Refilling of geosynchronous flux tubes as observed at the equator by GEOS 2
Author(s) -
Sojka J. J.,
Wrenn G. L.
Publication year - 1985
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/ja090ia07p06379
Subject(s) - plasmasphere , geosynchronous orbit , physics , earth's magnetic field , flux (metallurgy) , equator , plasma , electron density , population , flux tube , geophysics , van allen radiation belt , atmospheric sciences , satellite , magnetosphere , magnetic flux , astronomy , magnetic field , materials science , latitude , demography , quantum mechanics , sociology , metallurgy
During periods of extended quiet geomagnetic activity the geosynchronous satellite orbit lies inside the plasmasphere. Five such periods were observed by the GEOS 2 satellite. During the initial 48 hours of such periods the equatorial plasma flux tube density increases at 30 to 50 cm −3 /day. However, on reaching ∼100 cm −3 the refilling rate decreases, and refilling is limited. Only when the density reaches ∼100 cm −3 do the plasma characteristics and fluctuations appear to be plasmaspheric and the flow predominantly corotational. The “hot outer zone” of the plasmasphere is highly structured in density and temperature when viewed from a corotating satellite. This region also has a relatively dense population of warm subkilovolt electrons. These warm electrons whose density is ∼1% to 50% of the cold plasma may be the heat source for the hot outer zone ions.
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