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Title: Magnetospheric Multiscale Observations of Electron Vortex Magnetic Hole in the Turbulent Magnetosheath Plasma

Journal Article · · Astrophysical Journal Letters
; ; ;  [1]; ;  [2];  [3];  [4]; ; ;  [5];  [6]; ;  [7];  [8];  [9]; ;  [10];  [11];
  1. School of Electronic Information, Wuhan University, Wuhan (China)
  2. Laboratoire de Physique des Plasmas, CNRS-Ecole Polytechnique-UPMC, Palaiseau (France)
  3. School of Earth and Space Sciences, Peking University, Beijing (China)
  4. Key Laboratory of Planetary Sciences, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing (China)
  5. Institute of Space Science and Technology, Nanchang University, Nanchang (China)
  6. Department of Physics and Astronomy, University of California, Los Angeles, CA (United States)
  7. School of Space and Environment, Beihang University, Beijing (China)
  8. Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, Institute of Space Sciences, Shandong University, Weihai (China)
  9. Institut de Recherche and Astrophysique et Planétologie, Université de Toulouse (UPS), Toulouse (France)
  10. NASA, Goddard Space Flight Center, Greenbelt, MD (United States)
  11. University of New Hampshire, Durham, NH (United States)

We report on the observations of an electron vortex magnetic hole corresponding to a new type of coherent structure in the turbulent magnetosheath plasma using the Magnetospheric Multiscale mission data. The magnetic hole is characterized by a magnetic depression, a density peak, a total electron temperature increase (with a parallel temperature decrease but a perpendicular temperature increase), and strong currents carried by the electrons. The current has a dip in the core region and a peak in the outer region of the magnetic hole. The estimated size of the magnetic hole is about 0.23 ρ {sub i} (∼30 ρ {sub e}) in the quasi-circular cross-section perpendicular to its axis, where ρ {sub i} and ρ {sub e} are respectively the proton and electron gyroradius. There are no clear enhancements seen in high-energy electron fluxes. However, there is an enhancement in the perpendicular electron fluxes at 90° pitch angle inside the magnetic hole, implying that the electrons are trapped within it. The variations of the electron velocity components V {sub em} and V {sub en} suggest that an electron vortex is formed by trapping electrons inside the magnetic hole in the cross-section in the M – N plane. These observations demonstrate the existence of a new type of coherent structures behaving as an electron vortex magnetic hole in turbulent space plasmas as predicted by recent kinetic simulations.

OSTI ID:
22654531
Journal Information:
Astrophysical Journal Letters, Vol. 836, Issue 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 2041-8205
Country of Publication:
United States
Language:
English

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