Externally driven bifurcation of current sheet: A particle-in-cell simulation
Source abstract
Abstract
A current sheet is a confined layer of electric current in the presence of a strong magnetic gradient, which exists ubiquitously in space and the universe. Magnetic energy is stored in current sheets and then potentially released through processes such as magnetic reconnection. Spacecraft observations show that some current sheets in Earth’s magnetotail are bifurcated with a double-peak current density profile. The cause of this bifurcation, however, is still unclear. Here, using a particle-in-cell simulation, we show the bifurcation is formed when the current sheet is thinned by an external driver. In this process, an electron pressure anisotropy (pe⊥ > pe∥) is formed at the center of the current sheet, which decreases the current density at the center, leading to the bifurcated profile of the current density.
Source: crossref · Quality: baseline
Research context
OpenAlex topics: Ionosphere and magnetosphere dynamics · Solar and Space Plasma Dynamics · Earthquake Detection and Analysis
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Department of Electric and Computer Engineering, State University of New York-Binghamton 1 , Binghamton, New York 13902, USA
Department of Earth, Planetary, and Space Sciences, University of California 2 , Los Angeles, California 90095, USA
Funding
National Aeronautics and Space Administration
References (32)
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