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Short large-amplitude magnetic structures (SLAMS) at Venus

  • G. A. Collinson*
  • , L. B. Wilson
  • , D. G. Sibeck
  • , N. Shane
  • , T. L. Zhang
  • , T. E. Moore
  • , A. J. Coates
  • , S. Barabash
  • *Corresponding author for this work
  • NASA Goddard Space Flight Center
  • University College London
  • Center for Planetary Sciences, University College London/Birkbeck
  • Austrian Academy of Sciences
  • Swedish Institute of Space Physics

Research output: Contribution to journalArticlepeer-review

Abstract

We present the first observation of magnetic fluctuations consistent with short large-amplitude magnetic structures (SLAMS) in the foreshock of the planet Venus. Three monolithic magnetic field spikes were observed by the Venus Express on 11 April 2009. The structures were ∼1.5-11s in duration, had magnetic compression ratios between ∼3 and 6, and exhibited elliptical polarization. These characteristics are consistent with the SLAMS observed at Earth, Jupiter, and Comet Giacobini-Zinner, and thus we hypothesize that it is possible SLAMS may be found at any celestial body with a foreshock.

Original languageEnglish
Article numberA10221
JournalJournal of Geophysical Research: Space Physics
Volume117
Issue number10
DOIs
StatePublished - 2012
Externally publishedYes

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