Numerical MHD Simulations of the 3D Morphology and Kinematics of the 2017 September 10 CME-driven Shock from the Sun to Earth-Reference-Cited by-同舟云学术

Numerical MHD Simulations of the 3D Morphology and Kinematics of the 2017 September 10 CME-driven Shock from the Sun to Earth

Published:2021-09-01 Issue:1 Volume:918 Page:31
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Yang Liping^ORCID,Wang Haopeng,Feng Xueshang^ORCID,Xiong Ming^ORCID,Zhang Man^ORCID,Zhu Bei,Li Huichao^ORCID,Zhou Yufen,Shen Fang^ORCID,Zhao Xinhua^ORCID,Liu Xiaojing

Funder

NSFC

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ac0ef7/pdf

Reference76 articles.

1. Characterizing and predicting the magnetic environment leading to solar eruptions

2. Coronal Mass Ejection: Initiation, Magnetic Helicity, and Flux Ropes. I. Boundary Motion–driven Evolution

3. Parametric Study of ICME Properties Related to Space Weather Disturbances via a Series of Three-Dimensional MHD Simulations

4. FIRST COMPLETE DETERMINATION OF PLASMA PHYSICAL PARAMETERS ACROSS A CORONAL MASS EJECTION-DRIVEN SHOCK

5. The Large Angle Spectroscopic Coronagraph (LASCO)

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