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Magnetospheric boundary shapes and internal structures

Conference · · Adv. Space Res.; (United States)
OSTI ID:5023686
ISEE data, together with previously known results, are used to identify magnetospheric plasma regimes and their boundaries. The bow shock and its asymmetric foreshock is the first magnetospheric boundary, the entire magnetosphere being tilted by 5-10 deg (close to the earth) because of its intrinsic asymmetry. Although the magnetopause limits the magnetosheath, magnetospheric phenomena are observed outside it. At high latitudes along the magnetopause, the entry layer and the plasma mantle whose properties are somewhat influenced by the IMF are found. A flowing plasma is observed in the tail which originates from the polar ionospheric regions and makes an important contribution to the magnetospheric plasma from a source other than the solar wind.
Research Organization:
ESA, Space Science Dept., Noordwijk, Netherlands
OSTI ID:
5023686
Report Number(s):
CONF-8006190-
Conference Information:
Journal Name: Adv. Space Res.; (United States) Journal Volume: 1:1
Country of Publication:
United States
Language:
English