Literature DB >> 22026861

Jet deflection by very weak guide fields during magnetic reconnection.

M V Goldman1, G Lapenta, D L Newman, S Markidis, H Che.   

Abstract

Previous 2D simulations of reconnection using a standard model of initially antiparallel magnetic fields have detected electron jets outflowing from the x point into the ion outflow exhausts. Associated with these jets are extended "outer electron diffusion regions." New PIC simulations with an ion to electron mass ratio as large as 1836 (an H(+) plasma) now show that the jets are strongly deflected and the outer electron diffusion region is broken up by a very weak out-of-plane magnetic guide field, even though the diffusion rate itself is unchanged. Jet outflow and deflection are interpreted in terms of electron dynamics and are compared to recent measurements of jets in the presence of a small guide field in Earth's magnetosheath.

Year:  2011        PMID: 22026861     DOI: 10.1103/PhysRevLett.107.135001

Source DB:  PubMed          Journal:  Phys Rev Lett        ISSN: 0031-9007            Impact factor:   9.161


  2 in total

1.  Direct evidence for kinetic effects associated with solar wind reconnection.

Authors:  Xiaojun Xu; Yi Wang; Fengsi Wei; Xueshang Feng; Xiaohua Deng; Yonghui Ma; Meng Zhou; Ye Pang; Hon-Cheng Wong
Journal:  Sci Rep       Date:  2015-01-28       Impact factor: 4.379

2.  Structure of the Current Sheet in the 11 July 2017 Electron Diffusion Region Event.

Authors:  Rumi Nakamura; Kevin J Genestreti; Takuma Nakamura; Wolfgang Baumjohann; Ali Varsani; Tsugunobu Nagai; Naoki Bessho; James L Burch; Richard E Denton; Jonathan P Eastwood; Robert E Ergun; Daniel J Gershman; Barbara L Giles; Hiroshi Hasegawa; Michael Hesse; Per-Arne Lindqvist; Christopher T Russell; Julia E Stawarz; Robert J Strangeway; Roy B Torbert
Journal:  J Geophys Res Space Phys       Date:  2019-02-27       Impact factor: 2.811

  2 in total

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