How does large flaring activity from the same active region produce oppositely directed magnetic clouds?

Solar Physics

Volumn 244, Issue 1-2, 2007, Pages 95-114

  Harra, Louise K ^a   Crooker, Nancy U ^b   Mandrini, Cristina H ^c   Van Driel Gesztelyi, Lidia ^a,d,e   Dasso, Sergio ^c,g   Wang, Jingxiu ^f   Elliott, Heather ^h   Attrill, Gemma ^a   Jackson, Bernard V ⁱ   Bisi, Mario M ⁱ  

^a UNIVERSITY COLLEGE LONDON   (United Kingdom)

^b BOSTON UNIVERSITY   (United States)

^c INSTITUTO DE ASTRONOMÍA Y FÍSICA DEL ESPACIO   (Argentina)

^d OBSERVATOIRE DE PARIS   (France)

^e INSTITUTE OF EXPERIMENTAL MEDICINE   (Hungary)

^f INSTITUTE OF GEOLOGY AND GEOPHYSICS   (China)

^g UNIVERSIDAD DE BUENOS AIRES   (Argentina)

^h SOUTHWEST RESEARCH INSTITUTE   (United States)

ⁱ UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 35248859207     PISSN: 00380938     EISSN: 1573093X     Source Type: Journal    
DOI: 10.1007/s11207-007-9002-x     Document Type: Article

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