Dependence of coronal mass ejections on the morphology and toroidal flux of their source magnetic flux ropes

被引：0

作者：

Guo, J.H. ^{[1
,2
]}

Linan, L. ^{[1
]}

Poedts, S. ^{[1
,3
]}

Guo, Y. ^{[2
]}

Schmieder, B. ^{[1
,4
]}

Lani, A. ^{[1
]}

Ni, Y.W. ^{[2
]}

Brchnelova, M. ^{[1
]}

Perri, B. ^{[1
,5
]}

Baratashvili, T. ^{[1
]}

Li, S.T. ^{[6
,7
]}

Chen, P.F. ^{[2
]}

机构：

[1] Centre for Mathematical Plasma Astrophysics, Department of Mathematics, Ku Leuven, Celestijnenlaan 200B, Leuven,B-3001, Belgium

[2] School of Astronomy and Space Science, Key Laboratory of Modern Astronomy and Astrophysics, Nanjing University, Nanjing,210023, China

[3] Institute of Physics, University of Maria Curie-Sklodowska, ul. Marii Curie-Sklodowskiej 1, Lublin,20-031, Poland

[4] Lesia, Observatoire de Paris, Cnrs, Upmc, Université Paris Diderot, 5 place Jules Janssen, Meudon,92190, France

[5] AIM/DAp - Cea Paris-Saclay, Université Paris-Saclay, Université Paris-Cité, Gif-sur-Yvette, France

[6] Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing,210023, China

[7] Inaf - Turin Astrophysical Observatory, Via Osservatorio 20, (TO), Pino Torinese,10025, Italy

来源：

Astronomy and Astrophysics | 1600年 / 690卷

关键词：

96;

D O I：

暂无

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摘要：

Journal article (JA)

引用

共 50 条

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