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Plasma sheet stretching accompanied by field aligned energetic ion fluxes observed by the NUADU instrument aboard TC-2

  • Li Lu*
  • , S. Mckenna-Lawlor
  • , S. Barabash
  • , Zhen Xing Liu
  • , Jin Bin Cao
  • , J. Balaz
  • , K. Kudela
  • , T. L. Zhang
  • , C. M. Carr
  • *Corresponding author for this work
  • CAS - National Space Science Center
  • Maynooth University
  • Box 537
  • Slovak Academy of Sciences
  • Austrian Academy of Sciences
  • Imperial College London

Research output: Contribution to journalArticlepeer-review

Abstract

The NUADU (NeUtral Atom Detector Unit) instrument aboard TC-2 recorded 4cyrillic letter El solid angle images of charged particles (E >180 keV) spiraling around the magnetic field lines in the near-Earth plasma sheet (at ∼ -7 R E, equatorial dawn-to-night side) during a geomagnetic storm (Dst =-219 nT) on August 24, 2005. Energetic ion beam events characterized by symmetrical, ring-like, solid angle distributions around ambient magnetic field lines were observed during a 34-minute traversal of the plasma sheet by the TC-2 spacecraft. Also, observations during these multiple crossings of the plasma sheet were monitored by the magnetometer experiment (FGM) aboard the same spacecraft. During each crossing, a whistler-mode chorus enhancement was observed in the anisotropic area by the TC-2 low frequency electromagnetic wave detector (LFEW/TC-2) at a frequency just above that of the local lower hybrid wave. A comparison of the ion pitch angle distribution (PAD) map with the ambient magnetic field shows that an enhancement in the field aligned energetic ion flux was accompanied by tailward stretching of the magnetic field lines in the plasma sheet. In contrast, the perpendicular ion-flux enhancement was accompanied by a signature indicating the corresponding shrinkage of the magnetic field lines in the plasma sheet. Since both parallel ion-flux and perpendicular ion-flux enhancements occurred intermittently, the data were interpreted to imply a dynamical, oscillatory process of the magnetic field line (stretching and shrinking) in the near-Earth plasma sheet, which might have acted to help establish an interaction region in this area which would support continuous aurora-substorm triggering during the ongoing magnetic storm. The whistler-mode chorus may have been produced due to ion gyro-resonance during particle pitch angle diffusion after the plasma sheet compression.

Original languageEnglish
Pages (from-to)1719-1723
Number of pages5
JournalChinese Science Bulletin
Volume52
Issue number12
DOIs
StatePublished - Jun 2007
Externally publishedYes

Keywords

  • Energetic ion flux
  • Near-Earth plasma sheet
  • Pitch angle distribution
  • Whistler-mode chorus

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