Kinetic models of solar wind current sheet

T. Neukirch, I. Vasko, A. Artemyev, O. Allanson

Research output: Contribution to conference (unpublished)Paper

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Abstract

Current sheets in the collisionless solar wind usually have kinetic spatial scales. In-situ measurements show that these current sheets are often approximately force-free, i.e. the directions
of their current density and magnetic field are aligned, despite the fact that the plasma beta
is found to be of the order of one. The measurements also often show systematic asymmetric spatial variations of the plasma density and temperature across the current sheets, whilst
the plasma pressure is approximately uniform. Neukirch et al. (2020) found exact equilibrium
models of force-free collisionless current sheets which allowed for asymmetric plasma density
and temperature gradients. These models assumed that the form of the distribution function for
electrons and ions is the same. In this contribution we generalise this approach to current sheets
with static ions. As a consequence the force-free condition is only satisfied approximately and
quasi-neutrality requires the presence of a nonvanishing electric potential.
Original languageEnglish
Publication statusPublished - Jul 2022
Event48th European Physical Society Conference on Plasma Physics - Virtual, Online
Duration: 27 Jun 20221 Jul 2022
https://indico.fusenet.eu/event/28/ (Conference in online conference environment)

Conference

Conference48th European Physical Society Conference on Plasma Physics
Abbreviated titleEPS 2022
CityVirtual, Online
Period27/06/221/07/22
Internet address

Bibliographical note

Funding Information:
TN acknowledges financial support by the Science and Technology Facilities Council (STFC) via Consolidated Grant ST/W001195/1. OA acknowledges financial support by Natural Environment Research Council (NERC) Independent Research Fellowship NE/ V013963/1.

ASJC Scopus subject areas

  • Atomic and Molecular Physics, and Optics

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