• Volume/Page
  • Keyword
  • DOI
  • Citation
  • Advanced
   
 
 
 

Flickr Twitter iResearch App Facebook

Phys. Plasmas 17, 110701 (2010); http://dx.doi.org/10.1063/1.3493627 (4 pages)

Magnetic vortex growth in the transition layer of a mildly relativistic plasma shock

G. C. Murphy, M. E. Dieckmann, and L. O’C. Drury

Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2, Ireland

View MapView Map

(Received 9 April 2010; accepted 7 September 2010; published online 2 November 2010)

A two-dimensional particle simulation models the collision of two electron-ion plasma clouds along a quasiparallel magnetic field. The collision speed is 0.9c and the density ratio, 10. A current sheet forms at the front of the dense cloud, in which the electrons and the magnetic field reach energy equipartition with the ions. A structure composed of a solenoidal and a toroidal magnetic field grows in this sheet. It resembles the cross-section of the torus of a spheromak, which may provide the coherent magnetic fields in gamma-ray burst jets needed for their prompt emissions.

© 2010 American Institute of Physics

RELATED DATABASES

To view database links for this article, you need to log in.

KEYWORDS and PACS

PACS

ARTICLE DATA

PUBLICATION DATA

ISSN

1070-664X (print)  
1089-7674 (online)

For access to fully linked references, you need to log in.

    References

    T. Piran, Rev. Mod. Phys. 76, 1143 (2005).

    N. Bessho and Y. Ohsawa, Phys. Plasmas 6, 3076 (1999)PHPAEN000006000008003076000001.

    J. M. Dawson, Rev. Mod. Phys. 55, 403 (1983).

    M. Cerchez, R. Jung, J. Osterholz, T. Toncian, O. Willi, P. Mulser, and H. Ruhl, Phys. Rev. Lett. 100, 245001 (2008), P. Mulser, D. Bauer, and H. Ruhl, ibid. 101, 225002 (2008).

    A. Bret and M. E. Dieckmann, Phys. Plasmas 17, 032109 (2010)PHPAEN000017000003032109000001.

    J. B. Taylor, Rev. Mod. Phys. 58, 741 (1986).


Access to article objects (figures, tables, multimedia) requires a subscription; log in to view available files.
(Access to supplementary files, where available, is free for this journal.)

Access to article objects (figures, tables, multimedia) requires a subscription; log in to view available files.
(Access to supplementary files, where available, is free for this journal.)



Close
Google Calendar
ADVERTISEMENT

close