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Evidence for Secondary Flux Rope Generated by the Electron Kelvin-Helmholtz Instability in a Magnetic Reconnection Diffusion Region.
Zhong, Z H; Tang, R X; Zhou, M; Deng, X H; Pang, Y; Paterson, W R; Giles, B L; Burch, J L; Tobert, R B; Ergun, R E; Khotyaintsev, Y V; Lindquist, P-A.
Afiliação
  • Zhong ZH; Department of Physics, School of Science, Nanchang University, Nanchang 330031, People's Republic of China.
  • Tang RX; Institute of Space Science and Technology, Nanchang University, Nanchang 330031, People's Republic of China.
  • Zhou M; School of Resources Environmental and Chemical Engineering, Nanchang University, Nanchang 330031, People's Republic of China.
  • Deng XH; Department of Physics, School of Science, Nanchang University, Nanchang 330031, People's Republic of China.
  • Pang Y; Institute of Space Science and Technology, Nanchang University, Nanchang 330031, People's Republic of China.
  • Paterson WR; Institute of Space Science and Technology, Nanchang University, Nanchang 330031, People's Republic of China.
  • Giles BL; Department of Physics and Astronomy, University of California, Los Angeles, California 90095, USA.
  • Burch JL; Institute of Space Science and Technology, Nanchang University, Nanchang 330031, People's Republic of China.
  • Tobert RB; Institute of Space Science and Technology, Nanchang University, Nanchang 330031, People's Republic of China.
  • Ergun RE; NASA, Goddard Space Flight Center, Greenbelt, Maryland 20771, USA.
  • Khotyaintsev YV; NASA, Goddard Space Flight Center, Greenbelt, Maryland 20771, USA.
  • Lindquist PA; Southwest Research Institute, San Antonio Texas 78238, USA.
Phys Rev Lett ; 120(7): 075101, 2018 Feb 16.
Article em En | MEDLINE | ID: mdl-29542938
ABSTRACT
Secondary flux ropes are suggested to play important roles in energy dissipation and particle acceleration during magnetic reconnection. However, their generation mechanism is not fully understood. In this Letter, we present the first direct evidence that a secondary flux rope was generated due to the evolution of an electron vortex, which was driven by the electron Kelvin-Helmholtz instability in an ion diffusion region as observed by the Magnetospheric Multiscale mission. The subion scale (less than the ion inertial length) flux rope was embedded within the electron vortex, which contained a secondary electron diffusion region at the trailing edge of the flux rope. We propose that intense electron shear flow produced by reconnection generated the electron Kelvin-Helmholtz vortex, which induced a secondary reconnection in the exhaust of the primary X line and then led to the formation of the flux rope. This result strongly suggests that secondary electron Kelvin-Helmholtz instability is important for reconnection dynamics.

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2018 Tipo de documento: Article

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2018 Tipo de documento: Article