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May 4, 1998 storm: Observations of energetic ion composition by POLAR
Author(s) -
Chen Jiasheng,
Fritz Theodore A.
Publication year - 1999
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 - 10.1029/1999gl003582
Subject(s) - magnetosheath , magnetosphere , physics , van allen radiation belt , ion , polar , magnetopause , flux (metallurgy) , geophysics , geomagnetic storm , cusp (singularity) , solar wind , astrophysics , atmospheric sciences , astronomy , plasma , materials science , nuclear physics , geometry , mathematics , quantum mechanics , metallurgy
A major geomagnetic storm occurred at 5:00–12:05 UT on May 4, 1998. During this period, the magnetosphere was compressed and eroded; POLAR traveled in its outbound orbit from the equatorial radiation belt to the cusp and crossed the magnetopause into the magnetosheath. Two CEP‐like (Cusp Energetic Particle) events with two to three orders of magnitudes enhancements of MeV ion fluxes were measured. The first event had a peak flux higher than that of the intense outer radiation belt in the equatorial plane. The shape of the measured energy spectra (in the unit of keV/e) were ion species dependent. For He + /He + + ratio at 18–269 keV/e, the difference between the radiation belt and the magnetosheath can be by a factor of as large as 62. In the magnetosheath, the 18–269 keV/e ion composition are variable, indicating a mass dependent acceleration process. These MeV ions may be energized by a mechanism in the cusp responsible for the CEP events previously reported.