Physical structure of a coronal streamer in the closed-field region as observed from UVCS/SOHO and SXT/YOHKOH

Astrophysical Journal

Volumn 506, Issue 1 PART I, 1998, Pages 431-438

  Li, J ^a,b   Raymond, J C ^b,c   Acton, L W ^a,e   Kohl, J L ^a,d   Romoli, M ^a,c   Noci, G ^b,c,d   Naletto, G ^c,d  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b MONTANA STATE UNIVERSITY   (United States)

^c UNIVERSITY OF FLORENCE   (Italy)

^d UNIVERSITY OF PADOVA   (Italy)

^e SMITHSONIAN ASTROPHYSICAL OBSERVATORY   (United States)

Author keywords

Sun: corona; Sun: fundamental parameters; Sun: magnetic fields; Sun: X rays, gamma rays

Indexed keywords

EID: 22444456021     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/306244     Document Type: Article

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