X line distribution determined from earthward and tailward convective bursty flows in the central plasma sheet-Reference-Cited by-同舟云学术

X line distribution determined from earthward and tailward convective bursty flows in the central plasma sheet

Published:2010-06 Issue:A6 Volume:115 Page:n/a-n/a
ISSN:0148-0227
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res.

Author:

Zhang L. Q.¹,Liu Z. X.¹,Ma Z. W.²,Baumjohann W.³,Pu Z. Y.⁴,Dunlop M. W.⁵,Reme H.⁶,Wang J. Y.⁷

Affiliation:

1. State Key Laboratory of Space Weather, Center for Space Science and Applied Research; Chinese Academy of Sciences; Beijing China

2. Institute for Fusion Theory and Simulation; Zhejiang University; Hangzhou China

3. Space Research Institute; Austrian Academy of Sciences; Graz Austria

4. School of Earth and Space Sciences; Peking University; Beijing China

5. Space Sciences Division; Rutherford Appleton Laboratory; Didcot UK

6. Centre d'Etude Spatiale des Rayonnements; CNRS; Toulouse France

7. Information Engineering College; Central University for Nationalities; Beijing China

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Link

http://www.agu.org/journals/ja/ja1006/2009JA014429/2009JA014429.pdf

Reference53 articles.

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2. Statistical characteristics of bursty bulk flow events;Angelopoulos;J. Geophys. Res.,1994

3. Tail reconnection triggering substorm onset;Angelopoulos;Science,2008

4. The neutral line model of substorms: Past results and present view;Baker;J. Geophys. Res.,1996

5. Timing of magnetic reconnection initiation during a global magnetospheric substorm onset;Baker;Geophys. Res. Lett.,2002

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