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Flux-Rope Structure of Coronal Mass EjectionsThis Topical Issue (TI) of Solar Physics, devoted to the study of flux-rope structure in coronal mass ejections (CMEs), is based on two Coordinated Data Analysis Workshops (CDAWs) held in 2010 (20-23 September in Dan Diego, California, USA) and 2011 (5-9 September in Alcala, Spain). The primary purpose of the CDAWs was to address the question whether all CMEs have a flux rope structure. Each CDAW was attended by about 50 scientists interested in the origin, propagation, and interplanetary manifestation of CME phenomena.
Document ID
20150019869
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1007/s11207-013-0280-1
Authors
Gopalswamy, N. (NASA Goddard Space Flight Center Greenbelt, MD United States)
Nieves-Chinchilla, T. (Catholic Univ. of America Washington, DC, United States)
Hidalgo, M. (Alcala de Henares Univ. Madrid, Spain)
Zhang, J. (George Mason Univ. Fairfax, VA, United States)
Riley, P. (Predictive Science, Inc. San Diego, CA, United States)
van Driel-Gesztelyi, L. (Observatoire de Paris-Meudon France)
Mandrini, C. H. (Instituto de Astronomia y Fisica del Espacio Buenos Aires, Argentina)
Date Acquired
October 29, 2015
Publication Date
April 4, 2013
Publication Information
Publication: Solar Physics
Publisher: Springer
Volume: 284
Issue: 1
Subject Category
Solar Physics
Report/Patent Number
GSFC-E-DAA-TN26682
Funding Number(s)
CONTRACT_GRANT: NNG11PL10A
Distribution Limits
Public
Copyright
Other
Keywords
flux-rope

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