Structure and kinetic properties of slow-mode shocks associated with magnetic reconnection in the near-Earth magnetotail-Reference-Cited by-同舟云学术

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Structure and kinetic properties of slow-mode shocks associated with magnetic reconnection in the near-Earth magnetotail

Published:2011-07 Issue:2 Volume:48 Page:227-239
ISSN:0273-1177
Container-title:Advances in Space Research
language:en
Short-container-title:Advances in Space Research

Author:

Lin Xi,Deng Xiaohua,Yuan Zhigang,Zhou Meng,Li Shiyou,Pang Ye

Publisher

Elsevier BV

Subject

Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics

Reference40 articles.

1. The cluster magnetic field investigation: overview of on-flight performance and initial results;Balogh;Ann. Geophys.,2001

2. Cluster observations of electron holes in association with magnetotail reconnection and comparison to simulations;Cattell;J. Geophys. Res.,2005

3. First results obtained by the Cluster STAFF experiment;Cornilleau-Wehrlin;Ann. Geophys.,2003

4. Laminar wave-train structure of collisionless magnetic slow shocks;Coroniti;Nucl. Fusion,1971

5. Collisionless slow shocks in magnetotail reconnection;Cremer;Geophys. Res. Lett.,1999

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