A quantitative method to optimise magnetic field line fitting of observed coronal loops

Solar Physics

Volumn 218, Issue 1-2, 2003, Pages 29-40

  Carcedo, L ^a   Brown, D S ^a   Hood, A W ^a   Neukirch, T ^a   Wiegelmann, T ^a,b  

^a UNIVERSITY OF ST ANDREWS   (United Kingdom)

^b MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 3543100874     PISSN: 00380938     EISSN: None     Source Type: Journal    
DOI: 10.1023/b:sola.0000013045.65499.da     Document Type: Article

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