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Bidirectional electron anisotropies in the distant tail: ISEE-3 observations of polar rain

Conference ·
OSTI ID:6281232

A detailed observational treatment of bidirectional electrons (50 approx.500 eV) in the distant magnetotail (r greater than or equal to 100 R/sub E/) is presented. It is found that electrons in this energy range commonly exhibit strong, field-aligned anisotropies in the tail lobes. Because of large tail motions, the ISEE-3 data provide extensive sampling of both the north and south lobes in rapid succession, demonstrating directly the strong asymmetries that exist between the north and south lobes at any one time. The bidirectional fluxes are found to occur predominantly in the lobe directly connected to the sunward IMF in the open magnetosphere model (north lobe for away sectors and south lobe for toward sectors). Electron anisotropy and magnetic field data are presented which show the transition from unidirectional (sheath) electron populations to bidirectional (lobe) populations. Taken together, the present evidence suggests that the bidirectional electrons that we observe in the distant tail are closely related to the polar rain electrons observed previously at lower altitudes. Furthermore, these data provide strong evidence that the distant tail is comprised largely of open magnetic field lines in contradistinction to some recently advanced models.

Research Organization:
Los Alamos National Lab., NM (USA); Jet Propulsion Lab., Pasadena, CA (USA)
DOE Contract Number:
W-7405-ENG-36
OSTI ID:
6281232
Report Number(s):
LA-UR-85-4310; CONF-8510254-1; ON: DE86004737
Country of Publication:
United States
Language:
English