Two-dimensional structure of a polar coronal hole at solar minimum: New semiempirical methodology for deriving plasma parameters

Astrophysical Journal

Volumn 574, Issue 1 I, 2002, Pages 477-494

  Zangrilli, L ^a,d   Poletto, G ^b   Nicolosi, P ^c   Noci, G ^d   Romoli, M ^d  

^a OSSERVATORIO ASTRONOMICO DI TORINO   (Italy)

^b INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^c UNIVERSITY OF PADOVA   (Italy)

^d UNIVERSITY OF FLORENCE   (Italy)

Author keywords

Solar wind; Sun: corona; Sun: UV radiation

Indexed keywords

EID: 0041730926     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/340942     Document Type: Article

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