On the 3-D structure and dissipation of reconnection-driven flow bursts-Reference-Cited by-同舟云学术

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On the 3-D structure and dissipation of reconnection-driven flow bursts

Published:2014-06-03 Issue:11 Volume:41 Page:3710-3716
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophys. Res. Lett.

Author:

Drake J. F.¹,Swisdak M.²,Cassak P. A.³,Phan T. D.⁴

Affiliation:

1. Department of Physics and the Institute for Physical Sciences and Technology; University of Maryland; College Park Maryland USA

2. Institute for Research in Electronics and Applied Physics; University of Maryland; College Park Maryland USA

3. Department of Physics and Astronomy; West Virginia University; Morgantown West Virginia USA

4. Space Science Laboratory; University of California; Berkeley California USA

Funder

NSF

NASA

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/2014GL060249/fullpdf

Reference24 articles.

1. Magnetotail flow bursts: Association to global magnetospheric circulation, relationship to ionospheric activity and direct evidence for localization;Angelopoulos;Geophys. Res. Lett.,1997

2. Electromagnetic energy conversion at reconnection fronts;Angelopoulos;Science,2013

3. On the propagation of bubbles in the geomagnetic tail;Birn;Ann. Geophys.,2004

4. On the cause of supra-arcade downflows;Cassak;Astrophys. J. Lett.,2013

5. Direct evidence for magnetic reconnection in the solar wind near 1 AU;Gosling;Geophys. Res. Lett.,2005

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