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A simple test of the induced nature of the Martian tail

  • C. T. Russell*
  • , T. Mulligan
  • , M. Delva
  • , T. L. Zhang
  • , K. Schwingenschuh
  • *Corresponding author for this work
  • University of California at Los Angeles
  • Austrian Academy of Sciences

Research output: Contribution to journalArticlepeer-review

Abstract

The cross tail component of the magnetic field in the Mars wake allows a simple test of the contribution of the intrinsic planetary magnetic field to the observed magnetic field. If the magnetic tail is entirely induced, then the direction of this cross tail component should be highly correlated with the direction of the interplanetary magnetic field. It is found that the direction of the cross tail magnetic field is so highly correlated with the direction of the cross flow interplanetary magnetic field that there can be little intrinsic contribution to the Martian magnetotail. This in turn implies that the upper limit to the Martian magnetic moment is about 4 × 1011 Tm3.

Original languageEnglish
Pages (from-to)875-879
Number of pages5
JournalPlanetary and Space Science
Volume43
Issue number7
DOIs
StatePublished - Jul 1995
Externally publishedYes

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