Bimodal size of Jupiter's magnetosphere

D. J. McComas, F. Bagenal, R. W. Ebert

Research output: Contribution to journalArticle

11 Scopus citations

Abstract

Observations of Jovian magnetopause crossing by a number of different spacecraft have established that Jupiter's magnetosphere has a generally bimodal size distribution, with typical standoff distances at the nose of ∼63 and ∼92 RJ. Here we examine both the external solar wind structure and time constants and the internal magnetospheric time constants for shedding and refilling material in the Jovian plasma disk. We show that these latter time constants are ∼ hours to ∼10 h, comparable to the compression time of the magnetopause, but shorter than the typically several day expansion time when the solar wind dynamic pressure decreases. Together, we show that it is the well-developed compressions and rarefactions in the solar wind at ∼5 AU that produced the generally bimodally structured solar wind dynamic pressure and hence Jovian magnetospheric size.

Original languageEnglish (US)
Pages (from-to)1523-1529
Number of pages7
JournalJournal of Geophysical Research: Space Physics
Volume119
Issue number3
DOIs
StatePublished - Mar 2014

All Science Journal Classification (ASJC) codes

  • 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

Keywords

  • Jovian magnetosphere
  • Jupiter-solar wind interaction
  • corotating interaction regions
  • magnetopause standoff distance

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