Could the collision of CMEs in the heliosphere be super-elastic? Validation through three-dimensional simulations-Reference-Cited by-同舟云学术

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Could the collision of CMEs in the heliosphere be super-elastic? Validation through three-dimensional simulations

Published:2013-04-28 Issue:8 Volume:40 Page:1457-1461
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophys. Res. Lett.

Author:

Shen Fang¹,Shen Chenglong²,Wang Yuming²,Feng Xueshang¹,Xiang Changqing¹

Affiliation:

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

2. CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences; University of Science and Technology of China; Hefei Anhui China

Funder

973 key projects

CAS Knowledge Innovation Program

NFSC

ublic Science and Technology Research Funds Projects of Ocean

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/grl.50336/fullpdf

Reference26 articles.

1. On the effect of the initial magnetic polarity and of the background wind on the evolution of CME shocks;Chané;Astron. & Astrophys.,2005

2. Evolutionary signatures in complex ejecta and their driven shocks;Farrugia;Ann. Geophys.,2004

3. A class of TVD type combined numerical scheme for MHD equations with a survey about numerical methods in solar wind simulations;Feng;Space Sci. Rev.,2003

4. A comparative study on 3-D solar wind structure observed by Ulysses and MHD simulation;Feng;Chinese Sci. Bull.,2005

5. Magnetohydrodynamic simulations of the solar corona and solar wind using a boundary treatment to limit solar wind mass flux;Hayashi;Astrophys. J.,2005

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3. Propagation characteristics of coronal mass ejections (CMEs) in the corona and interplanetary space;Reviews of Modern Plasma Physics;2022-04-02

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