Literature DB >> 30364510

Orientation and Stability of Asymmetric Magnetic Reconnection X Line.

Yi-Hsin Liu1, M Hesse2,3, T C Li1, M Kuznetsova4, A Le5.   

Abstract

The orientation and stability of the reconnection x line in asymmetric geometry is studied using three-dimensional (3-D) particle-in-cell simulations. We initiate reconnection at the center of a large simulation domain to minimize the boundary effect. The resulting x line has sufficient freedom to develop along an optimal orientation, and it remains laminar. Companion 2-D simulations indicate that this x line orientation maximizes the reconnection rate. The divergence of the nongyrotropic pressure tensor breaks the frozen-in condition, consistent with its 2-D counterpart. We then design 3-D simulations with one dimension being short to fix the x line orientation but long enough to allow the growth of the fastest growing oblique tearing modes. This numerical experiment suggests that reconnection tends to radiate secondary oblique tearing modes if it is externally (globally) forced to proceed along an orientation not favored by the local physics. The development of oblique structure easily leads to turbulence inside small periodic systems.

Year:  2018        PMID: 30364510      PMCID: PMC6196328          DOI: 10.1029/2018JA025410

Source DB:  PubMed          Journal:  J Geophys Res Space Phys        ISSN: 2169-9380            Impact factor:   2.811


  10 in total

1.  In situ observations of a secondary magnetic island in an ion diffusion region and associated energetic electrons.

Authors:  Rongsheng Wang; Quanming Lu; Aimin Du; Shui Wang
Journal:  Phys Rev Lett       Date:  2010-04-29       Impact factor: 9.161

2.  A magnetic reconnection X-line extending more than 390 Earth radii in the solar wind.

Authors:  T D Phan; J T Gosling; M S Davis; R M Skoug; M Øieroset; R P Lin; R P Lepping; D J McComas; C W Smith; H Reme; A Balogh
Journal:  Nature       Date:  2006-01-12       Impact factor: 49.962

3.  Bifurcated structure of the electron diffusion region in three-dimensional magnetic reconnection.

Authors:  Yi-Hsin Liu; W Daughton; H Karimabadi; H Li; V Roytershteyn
Journal:  Phys Rev Lett       Date:  2013-06-25       Impact factor: 9.161

4.  A current filamentation mechanism for breaking magnetic field lines during reconnection.

Authors:  H Che; J F Drake; M Swisdak
Journal:  Nature       Date:  2011-06-01       Impact factor: 49.962

5.  Extended magnetic reconnection across the dayside magnetopause.

Authors:  M W Dunlop; Q-H Zhang; Y V Bogdanova; M Lockwood; Z Pu; H Hasegawa; J Wang; M G G T Taylor; J Berchem; B Lavraud; J Eastwood; M Volwerk; C Shen; J-K Shi; D Constantinescu; H Frey; A N Fazakerley; D Sibeck; P Escoubet; J A Wild; Z-X Liu
Journal:  Phys Rev Lett       Date:  2011-07-06       Impact factor: 9.161

6.  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

7.  Magnetospheric Multiscale Satellites Observations of Parallel Electric Fields Associated with Magnetic Reconnection.

Authors:  R E Ergun; K A Goodrich; F D Wilder; J C Holmes; J E Stawarz; S Eriksson; A P Sturner; D M Malaspina; M E Usanova; R B Torbert; P-A Lindqvist; Y Khotyaintsev; J L Burch; R J Strangeway; C T Russell; C J Pollock; B L Giles; M Hesse; L J Chen; G Lapenta; M V Goldman; D L Newman; S J Schwartz; J P Eastwood; T D Phan; F S Mozer; J Drake; M A Shay; P A Cassak; R Nakamura; G Marklund
Journal:  Phys Rev Lett       Date:  2016-06-10       Impact factor: 9.161

8.  Electron-scale measurements of magnetic reconnection in space.

Authors:  J L Burch; R B Torbert; T D Phan; L-J Chen; T E Moore; R E Ergun; J P Eastwood; D J Gershman; P A Cassak; M R Argall; S Wang; M Hesse; C J Pollock; B L Giles; R Nakamura; B H Mauk; S A Fuselier; C T Russell; R J Strangeway; J F Drake; M A Shay; Yu V Khotyaintsev; P-A Lindqvist; G Marklund; F D Wilder; D T Young; K Torkar; J Goldstein; J C Dorelli; L A Avanov; M Oka; D N Baker; A N Jaynes; K A Goodrich; I J Cohen; D L Turner; J F Fennell; J B Blake; J Clemmons; M Goldman; D Newman; S M Petrinec; K J Trattner; B Lavraud; P H Reiff; W Baumjohann; W Magnes; M Steller; W Lewis; Y Saito; V Coffey; M Chandler
Journal:  Science       Date:  2016-05-12       Impact factor: 47.728

9.  On the Collisionless Asymmetric Magnetic Reconnection Rate.

Authors:  Yi-Hsin Liu; M Hesse; P A Cassak; M A Shay; S Wang; L-J Chen
Journal:  Geophys Res Lett       Date:  2018-03-06       Impact factor: 4.720

10.  Electron Crescent Distributions as a Manifestation of Diamagnetic Drift in an Electron-Scale Current Sheet: Magnetospheric Multiscale Observations Using New 7.5 ms Fast Plasma Investigation Moments.

Authors:  A C Rager; J C Dorelli; D J Gershman; V Uritsky; L A Avanov; R B Torbert; J L Burch; R E Ergun; J Egedal; C Schiff; J R Shuster; B L Giles; W R Paterson; C J Pollock; R J Strangeway; C T Russell; B Lavraud; V N Coffey; Y Saito
Journal:  Geophys Res Lett       Date:  2018-01-30       Impact factor: 4.720

  10 in total

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