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Ion Nongyrotropy in Solar Wind Discontinuities

  • Authors: Anton V. Artemyev, Vassilis Angelopoulos, Ivan Y. Vasko, and Lev M. Zelenyi

2020 The Astrophysical Journal Letters 889 L23.

  • Provider: AAS Journals

Caption: Figure 2.

Two discontinuities captured by ARTEMIS P2: (a) magnetic field in local coordinates, (b) ion spectrum and mean energy (black dashed line), (c) variations of vl, ﹩{v}_{{\rm{A}}}^{* }={v}_{{\rm{A}}}\sqrt{1-{{\rm{\Lambda }}}_{e}}﹩, and a nondiagonal ion pressure component Πln, (d) current density (top panels) the inserted panels show current density spatial distributions; the coordinate is normalized to the proton inertial length, di), (bottom panels) two cross sections of ion distribution before and after discontinuity crossings (see the text for details).

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