Formation of a transient front structure near reconnection point in 3-D PIC simulations-Reference-Cited by-同舟云学术

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Formation of a transient front structure near reconnection point in 3-D PIC simulations

Published:2013-04 Issue:4 Volume:118 Page:1435-1449
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Vapirev A.E.¹²,Lapenta G.¹,Divin A.³,Markidis S.⁴,Henri P.⁵,Goldman M.⁶,Newman D.⁶

Affiliation:

1. Centre for Plasma Astrophysics; Katholieke Universiteit Leuven; Belgium

2. Intel ExaScience Laboratory; Leuven Belgium

3. Swedish Institute of Space Physics; Uppsala; Sweden

4. PDC Centre; KTH Royal Institute of Technology; Stockholm Sweden

5. Dipartimento Fisica; Universita di Pisa; Pisa Italy

6. Center for Integrated Plasma Studies; University of Colorado; Boulder Colorado USA

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/jgra.50136/fullpdf

Reference55 articles.

1. The development of the auroral substorm;Akasofu;Planet. Space Sci.,1964

2. Bursty bulk flows in the inner plasma sheet;Angelopoulos;J. Geophys. Res.,1992

3. The THEMIS fluxgate magnetometer;Auster;Space Sci. Rev.,2008

4. Reconnection, substorms and solar flares;Axford;Phys. Chem. Earth C,1999

5. Neutral line model of substorms: Past results and present view;Baker;J. Geophys. Res.,1996

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