Ion Reflection by a Rippled Perpendicular Shock

Fuente: arXiv
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Auteurs principaux: Khotyaintsev, Yuri V., Graham, Daniel B., Johlander, Andreas
Format: Preprint
Publié: 2023
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author Khotyaintsev, Yuri V.
Graham, Daniel B.
Johlander, Andreas
author_facet Khotyaintsev, Yuri V.
Graham, Daniel B.
Johlander, Andreas
contents We use multi-spacecraft Magnetospheric Multiscale (MMS) observations to investigate electric fields and ion reflection at a non-stationary collisionless perpendicular plasma shock. We identify sub-proton scale (5-10 electron inertial lengths) large-amplitude normal electric fields, balanced by the Hall term ($\mathbf{J} \times \mathbf{B}/ne$), as a transient feature of the shock ramp related to non-stationarity (rippling). The associated electrostatic potential, comparable to the energy of the incident solar wind protons, decelerates incident ions and reflects a significant fraction of protons, resulting in more efficient shock-drift acceleration than a stationary planar shock.
format Preprint
id arxiv_https___arxiv_org_abs_2312_14736
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Ion Reflection by a Rippled Perpendicular Shock
Khotyaintsev, Yuri V.
Graham, Daniel B.
Johlander, Andreas
Space Physics
Plasma Physics
We use multi-spacecraft Magnetospheric Multiscale (MMS) observations to investigate electric fields and ion reflection at a non-stationary collisionless perpendicular plasma shock. We identify sub-proton scale (5-10 electron inertial lengths) large-amplitude normal electric fields, balanced by the Hall term ($\mathbf{J} \times \mathbf{B}/ne$), as a transient feature of the shock ramp related to non-stationarity (rippling). The associated electrostatic potential, comparable to the energy of the incident solar wind protons, decelerates incident ions and reflects a significant fraction of protons, resulting in more efficient shock-drift acceleration than a stationary planar shock.
title Ion Reflection by a Rippled Perpendicular Shock
topic Space Physics
Plasma Physics
url https://arxiv.org/abs/2312.14736