Statistical comparison of the observed and synthetic hydrogen Lyman line profiles in solar prominences

0354498 - ASÚ 2011 RIV FR eng J - Článek v odborném periodiku
Gunár, Stanislav - Schwartz, Pavol - Schmieder, B. - Heinzel, Petr - Anzer, U.
Statistical comparison of the observed and synthetic hydrogen Lyman line profiles in solar prominences.
Astronomy & Astrophysics. Roč. 514, May (2010), A43/1-A43/11. ISSN 0004-6361. E-ISSN 1432-0746
Grant CEP: GA ČR GP205/09/P554; GA ČR GA205/07/1100; GA AV ČR 1QS300120506
Grant ostatní: ESA(XE) ESA-PECS project No. 98030
Výzkumný záměr: CEZ:AV0Z10030501
Klíčová slova: Sun filaments * prominences * radiative transfer
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
Impakt faktor: 4.410, rok: 2010

Quiescent solar prominences consist of a large number of moving small-scale plasma structures. These are regularly observed in UV by space-based spectrographs. This is the first statistical comparison of the Lyman spectra observed by SOHO/SUMER with synthetic spectra obtained by 2D multi-thread prominence fine-structure models.
Trvalý link: http://hdl.handle.net/11104/0193485