Observations of Whistler Waves Correlated with Electron-scale Coherent Structures in the Magnetosheath Turbulent Plasma

  • S. Y. Huang
  • , F. Sahraoui
  • , Z. G. Yuan
  • , O. Le Contel
  • , H. Breuillard
  • , J. S. He
  • , J. S. Zhao
  • , H. S. Fu
  • , M. Zhou
  • , X. H. Deng
  • , X. Y. Wang
  • , J. W. Du
  • , X. D. Yu
  • , D. D. Wang
  • , C. J. Pollock
  • , R. B. Torbert
  • , J. L. Burch

Research output: Contribution to journalArticlepeer-review

Abstract

A new type of electron-scale coherent structure, referred to as electron vortex magnetic holes, was identified recently in the Earth's magnetosheath turbulent plasma. These electron-scale magnetic holes are characterized by magnetic field strength depression, electron density enhancement, temperature and temperature anisotropy increase (a significant increase in perpendicular temperature and a decrease in parallel temperature), and an electron vortex formed by the trapped electrons. The strong increase of electron temperature indicates that these magnetic holes have a strong connection with the energization of electrons. Here, using high time resolution in situ measurements from the MMS mission, it is further shown that electron-scale whistler waves coexist with electron-scale magnetic holes. These whistler waves were found not propagating from remote regions, but generated locally due to electron temperature anisotropy (T eperp;/T e∥) inside the magnetic holes. This study provides new insights into the electron-scale plasma dynamics in turbulent plasmas.

Original languageEnglish
Article number29
JournalAstrophysical Journal
Volume861
Issue number1
DOIs
Publication statusPublished - 1 Jul 2018

Keywords

  • Turbulence
  • planets and satellites: magnetic fields
  • planets and satellites: physical evolution
  • plasmas
  • waves

Fingerprint

Dive into the research topics of 'Observations of Whistler Waves Correlated with Electron-scale Coherent Structures in the Magnetosheath Turbulent Plasma'. Together they form a unique fingerprint.

Cite this