Diamagnetic and expansion effects on the observable properties of the slow solar wind in a coronal streamer

Astrophysical Journal

Volumn 633, Issue 1 I, 2005, Pages 474-488

  Rappazzo, A F ^a,d   Velli, M ^b,e   Einaudi, G ^a,f   Dahlburg, R B ^c  

^a UNIVERSITY OF PISA   (Italy)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c NAVAL RESEARCH LABORATORY   (United States)

^d Università di Firenze ^*

^e UNIVERSITY OF FLORENCE   (Italy)

^f GEORGE MASON UNIVERSITY   (United States)

Author keywords

MHD; Solar wind; Sun: corona; Sun: magnetic fields

Indexed keywords

EID: 29144480221     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/431916     Document Type: Article

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