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Rippled Electron-Scale Structure of a Dipolarization Front

  • Dong Xiao Pan
  • , Yuri V. Khotyaintsev
  • , Daniel B. Graham
  • , Andris Vaivads
  • , Xu Zhi Zhou
  • , Mats André
  • , Per Arne Lindqvist
  • , Robert E. Ergun
  • , Olivier Le Contel
  • , Christopher T. Russell
  • , Roy B. Torbert
  • , Barbara Giles
  • , James L. Burch
  • Tsinghua University
  • Swedish Institute of Space Physics
  • KTH Royal Institute of Technology
  • University of Colorado Boulder
  • Université Paris-Saclay
  • Institute of Geophysics and Planetary Physics, University of California
  • University of New Hampshire Durham
  • NASA Goddard Space Flight Center
  • Southwest Research Institute

Research output: Contribution to journalArticlepeer-review

Abstract

We use the Magnetospheric Multiscale mission to investigate electron-scale structures at a dipolarization front. The four spacecraft are separated by electron scales and observe large differences in plasma and field parameters within the dipolarization front, indicating strong deviation from typically assumed plane or slightly curved front surface. We attribute this to ripples generated by the lower hybrid drift instability (LHDI) with wave number of kρe≃0.4 and maximum wave potential of ∼1 kV ∼kBTe. Power law-like spectra of E with slope of −3 indicates the turbulent cascade of LHDI. LHDI is observed together with bursty high-frequency parallel electric fields, suggesting coupling of LHDI to higher-frequency electrostatic waves.

Original languageEnglish
Pages (from-to)12,116-12,124
JournalGeophysical Research Letters
Volume45
Issue number22
DOIs
Publication statusPublished - 28 Nov 2018
Externally publishedYes

Keywords

  • LHDI
  • MMS
  • dipolarization fronts
  • electron-scale structures
  • ripples
  • turbulence

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