Number of the records: 1  

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

  1. 1.
    Heinzel, Petr - Schmieder, B. - Tziotziou, K.
    Why are solar filaments more extended in extreme-ultraviolet lines than in H alpha?
    Astrophysical Journal. Roč. 561, č. 2 (2001), s. L223-L227. ISSN 0004-637X. E-ISSN 1538-4357
    R&D Projects: GA AV ČR IAA3003902; GA AV ČR IBS1003006
    Impact factor: 5.921, year: 2001
    http://hdl.handle.net/11104/0023274

Number of the records: 1  

  This site uses cookies to make them easier to browse. Learn more about how we use cookies.