Why are solar filaments more extended in extreme-ultraviolet lines than in Hα?

Astrophysical Journal

Volumn 561, Issue 2 PART II, 2001, Pages

  Heinzel, P ^a   Schmieder, B ^b,c   Tziotziou, K ^b  

^a ASTRONOMICAL INSTITUTE   (Czech Republic)

^b OBSERVATOIRE DE PARIS   (France)

^c UNIVERSITY OF OSLO   (Norway)

Author keywords

Sun: Filaments; Techniques: Spectroscopic

Indexed keywords

EID: 15544366345     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/324755     Document Type: Article

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