Literature DB >> 30224858

Strongly localized magnetic reconnection by the super-Alfvénic shear flow.

Yi-Hsin Liu1, M Hesse2,3, F Guo4, H Li4, T K M Nakamura5.   

Abstract

We demonstrate that the dragging of the magnetic field by the super-Alfvénic shear flows out of the reconnection plane can strongly localize the reconnection x-line in collisionless pair plasmas, reversing the current direction at the x-line. Reconnection with this new morphology, which is impossible in resistive-magnetohydrodynamics, is enabled by the particle inertia. Surprisingly, the quasi-steady reconnection rate remains of order 0.1 even though the aspect ratio of the local x-line geometry is larger than unity, which completely excludes the role of tearing physics. We explain this by examining the transport of the reconnected magnetic flux and the opening angle ma de by the upstream magnetic field, concluding that the reconnection rate is still limited by the constraint imposed at the inflow region. Based on these findings, we propose that this often observed fast rate value of order 0.1 itself, in general, is an upper bound value determined by the upstream constraint, independent of the localization mechanism and dissipation therein.

Entities:  

Year:  2018        PMID: 30224858      PMCID: PMC6137741          DOI: 10.1063/1.5042539

Source DB:  PubMed          Journal:  Phys Plasmas        ISSN: 1070-664X            Impact factor:   2.023


  9 in total

1.  Role of dispersive waves in collisionless magnetic reconnection.

Authors:  B N Rogers; R E Denton; J F Drake; M A Shay
Journal:  Phys Rev Lett       Date:  2001-10-22       Impact factor: 9.161

2.  Magnetic reconnection in the two-dimensional Kelvin-Helmholtz instability.

Authors:  D A Knoll; L Chacón
Journal:  Phys Rev Lett       Date:  2002-05-13       Impact factor: 9.161

3.  Collisionless reconnection in an electron-positron plasma.

Authors:  N Bessho; A Bhattacharjee
Journal:  Phys Rev Lett       Date:  2005-12-05       Impact factor: 9.161

4.  Formation of plasmoid chains in magnetic reconnection.

Authors:  R Samtaney; N F Loureiro; D A Uzdensky; A A Schekochihin; S C Cowley
Journal:  Phys Rev Lett       Date:  2009-09-04       Impact factor: 9.161

5.  New measure of the dissipation region in collisionless magnetic reconnection.

Authors:  Seiji Zenitani; Michael Hesse; Alex Klimas; Masha Kuznetsova
Journal:  Phys Rev Lett       Date:  2011-05-11       Impact factor: 9.161

6.  Fast magnetic reconnection in the plasmoid-dominated regime.

Authors:  D A Uzdensky; N F Loureiro; A A Schekochihin
Journal:  Phys Rev Lett       Date:  2010-12-01       Impact factor: 9.161

7.  Formation of hard power laws in the energetic particle spectra resulting from relativistic magnetic reconnection.

Authors:  Fan Guo; Hui Li; William Daughton; Yi-Hsin Liu
Journal:  Phys Rev Lett       Date:  2014-10-08       Impact factor: 9.161

8.  Why does Steady-State Magnetic Reconnection have a Maximum Local Rate of Order 0.1?

Authors:  Yi-Hsin Liu; M Hesse; F Guo; W Daughton; H Li; P A Cassak; M A Shay
Journal:  Phys Rev Lett       Date:  2017-02-21       Impact factor: 9.161

9.  Turbulent mass transfer caused by vortex induced reconnection in collisionless magnetospheric plasmas.

Authors:  T K M Nakamura; H Hasegawa; W Daughton; S Eriksson; W Y Li; R Nakamura
Journal:  Nat Commun       Date:  2017-11-17       Impact factor: 14.919

  9 in total
  2 in total

Review 1.  PIC methods in astrophysics: simulations of relativistic jets and kinetic physics in astrophysical systems.

Authors:  Kenichi Nishikawa; Ioana Duţan; Christoph Köhn; Yosuke Mizuno
Journal:  Living Rev Comput Astrophys       Date:  2021-07-08

2.  Decay of Kelvin-Helmholtz Vortices at the Earth's Magnetopause Under Pure Southward IMF Conditions.

Authors:  T K M Nakamura; F Plaschke; H Hasegawa; Y-H Liu; K-J Hwang; K A Blasl; R Nakamura
Journal:  Geophys Res Lett       Date:  2020-06-29       Impact factor: 4.720

  2 in total

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