In situ observation at L = 2.3-5 by the Akebono satellite of the plasmaspheric depletion during the September 1998 magnetic storm

Hideaki Kawano, P. J. Chi, A. Kumamoto, A. Morioka

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Abstract

From ground-based observations at L = 2.07 of the field line resonance (FLR) during an intense magnetic storm on 25 September 1998, Chi et al. (2000) estimated that the equatorial plasma density at L = 2.07 dropped to 25% of the prestorm value. Such depletion very close to the Earth is unusual. Two possible interpretations of the result are: (1) the plasmapause moved inward past L = 2.07, and (2) the plasmapause remained outside L = 2.07, but the density within the plasmasphere decreased. To distinguish between these possibilities, we examine in situ observations of the electron density made by the Akebono satellite at I = 2.3-5 on four passes during the same storm. The electron density measured by Akebono at a reference L shell of L ∼2.5 changed with time in a manner consistent with the FLR-based estimates. On three of these passes, the plasmapause was located at L > 3, and if the plasmaspheric L profile of the Akebono density data is extrapolated inward, for each pass, its value at L = 2.07 matches the FLR-based estimates. However, on the pass at 2323-2351 UT on 25 September that corresponded to the severe density decrease detected at L = 2.07, Akebono did not detect a plasmapause in the L range (>2.3) for which the electron density data were available. For the same pass, inward extrapolation of the density measured at L > 2.3 was a factor of ∼5 smaller than the FLR-based estimate. This implies that there was a sharp density inward gradient (the plasmapause) at 2.07 < L < 2.3, supporting the second interpretation.

Original languageEnglish
Article numberA04204
JournalJournal of Geophysical Research: Space Physics
Volume111
Issue number4
DOIs
Publication statusPublished - Apr 1 2006

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EXOS-D satellite
plasmapause
magnetic storms
depletion
resonance lines
Satellites
Carrier concentration
electron density
estimates
Plasma density
plasmasphere
electrons
Extrapolation
Earth (planet)
plasma density
extrapolation
in situ
gradients
shell
plasma

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  • Geophysics
  • Forestry
  • Oceanography
  • Aquatic Science
  • Ecology
  • Water Science and Technology
  • Soil Science
  • Geochemistry and Petrology
  • Earth-Surface Processes
  • Atmospheric Science
  • Earth and Planetary Sciences (miscellaneous)
  • Space and Planetary Science
  • Palaeontology

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In situ observation at L = 2.3-5 by the Akebono satellite of the plasmaspheric depletion during the September 1998 magnetic storm. / Kawano, Hideaki; Chi, P. J.; Kumamoto, A.; Morioka, A.

In: Journal of Geophysical Research: Space Physics, Vol. 111, No. 4, A04204, 01.04.2006.

Research output: Contribution to journalArticle

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