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Why are solar filaments more extended in extreme-ultraviolet lines than in H alpha?
- 1.0125015 - ASU-R 20020111 RIV US eng J - Journal Article
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
Institutional research plan: CEZ:AV0Z1003909
Keywords : sun * filaments * spectroscopy
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
Impact factor: 5.921, year: 2001
A long solar filament was observed simultaneously in the H aspla line by THEMIS and in EUV lines by CDS/SOHO.
Permanent Link: http://hdl.handle.net/11104/0023274
Number of the records: 1