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Why are solar filaments more extended in extreme-ultraviolet lines than in H alpha?
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SYSNO 0125015 Title Why are solar filaments more extended in extreme-ultraviolet lines than in H alpha? Author(s) Heinzel, Petr (ASU-R) RID, ORCID
Schmieder, B. (FR)
Tziotziou, K. (FR)Source Title Astrophysical Journal. Roč. 561, č. 2 (2001), s. L223-L227 Document Type Článek v odborném periodiku Grant IAA3003902 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR) IBS1003006 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR) CEZ AV0Z1003909 - ASU-R Language eng Country US Keywords sun * filaments * spectroscopy Permanent Link http://hdl.handle.net/11104/0023274
Number of the records: 1