Three‐Dimensional X‐line Spreading in Asymmetric Magnetic Reconnection
نویسندگان
چکیده
منابع مشابه
New electric field in asymmetric magnetic reconnection.
We present a theory and numerical evidence for the existence of a previously unexplored in-plane electric field in collisionless asymmetric magnetic reconnection. This electric field, dubbed the "Larmor electric field," is associated with finite Larmor radius effects and is distinct from the known Hall electric field. Potentially, it could be an important indicator for the upcoming Magnetospher...
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[1] The scaling of the reconnection rate and ion and electron outflow speeds with upstream magnetic field strengths and plasma mass densities during asymmetric collisionless (Hall) reconnection without a guide field is studied using two-dimensional two-fluid simulations. The results agree with a recent theory by Cassak and Shay (2007). It is found that the normalized reconnection rate is on the...
متن کاملScaling of asymmetric magnetic reconnection: Kinetic particle‐in‐cell simulations
[1] Recently, Cassak and Shay (2007) applied a generalized Sweet‐Parker analysis to derive scaling laws for gross properties of asymmetric magnetic reconnection, including the reconnection rate, outflow speed, and outflow density. This study presents the first comprehensive test of this scaling theory using fully electromagnetic particle‐in‐cell simulations of antiparallel asymmetric magnetic r...
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Realistic models of magnetic reconnection in the solar chromosphere must take into account that the plasma is partially ionized and that plasma conditions within any two magnetic flux bundles undergoing reconnection may not be the same. Asymmetric reconnection in the chromosphere may occur when newly emerged flux interacts with pre-existing, overlying flux. We present 2.5D simulations of asymme...
متن کاملScaling of asymmetric magnetic reconnection: General theory and collisional simulations
A Sweet-Parker-type scaling analysis for asymmetric antiparallel reconnection in which the reconnecting magnetic field strengths and plasma densities are different on opposite sides of the dissipation region is performed. Scaling laws for the reconnection rate, outflow speed, the density of the outflow, and the structure of the dissipation region are derived from first principles. These results...
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ژورنال
عنوان ژورنال: Journal of Geophysical Research: Space Physics
سال: 2020
ISSN: 2169-9380,2169-9402
DOI: 10.1029/2019ja027094