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Well-resolved observations by ISEE 2 of ion dispersion in the magnetospheric cusp

Journal Article · · Journal of Geophysical Research
DOI:https://doi.org/10.1029/93JA00631· OSTI ID:96494
; ; ; ;  [1];  [2]
  1. Los Alamos National Lab., NM (United States)
  2. Univ. of New Hampshire, Durham, NH (United States)
During a prolonged period of southward interplanetary magnetic field on October 30, 1978, the ISEE 2 spacecraft observed an unusually prolonged and distinct region of ion energy-time dispersion in the dayside, dawn magnetosphere. Observed plasma features included the (1) presence of magnetosheath electrons and initial absence of magnetosheath ions and (2) subsequent arrival and energy-time dispersion of magnetosheath ions as the spacecraft transited outbound from 6.03 to 7.66 Earth radii. The authors use ISEE 2 ion measurements to illustrate these dispersive time-of-flight effects and to support their interpretation of a location in the North magnetospheric cusp. Ion energy dispersion, well documented at lower altitudes but generally only observable for a few minutes due to rapid cusp crossings by the spacecraft, in this case persists for {approximately}35 min and includes well-resolved sequences of magnetosheath and magnetospheric ion distributions. The authors focus primarily on observations and time-of-flight analysis of ions from the magnetosheath, which are observed simultaneously entering and exiting the cusp at different energies. They discuss the observational support and shortcomings of various ion injection locations and durations and conclude that quasi-steady merging at the dayside magnetopause, with ion dispersion caused by spacecraft motion away from the last closed field line, is the most likely scenario. 24 refs., 9 figs.
Sponsoring Organization:
USDOE
OSTI ID:
96494
Journal Information:
Journal of Geophysical Research, Journal Name: Journal of Geophysical Research Journal Issue: A8 Vol. 98; ISSN JGREA2; ISSN 0148-0227
Country of Publication:
United States
Language:
English

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