Why are halo coronal mass ejections faster?

Research in Astronomy and Astrophysics

Volumn 10, Issue 5, 2010, Pages 461-472

  Zhang, Qing Min ^a   Guo, Yang ^a   Chen, Peng Fei ^a,b   Ding, Ming De ^a,b   Fang, Cheng ^a,b  

^a NANJING UNIVERSITY   (China)

^b BEIJING UNIVERSITY OF POSTS AND TELECOMMUNICATIONS   (China)

Author keywords

Methods: numerical; Solar terrestrial relations; Sun: activity; Sun: coronal mass ejections (CMEs)

Indexed keywords

EID: 77951520827     PISSN: 16744527     EISSN: None     Source Type: Journal    
DOI: 10.1088/1674-4527/10/5/006     Document Type: Article

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