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Statistical comparison of the observed and synthetic hydrogen Lyman line profiles in solar prominences
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SYSNO ASEP 0354498 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title Statistical comparison of the observed and synthetic hydrogen Lyman line profiles in solar prominences Author(s) Gunár, Stanislav (ASU-R) RID, ORCID
Schwartz, Pavol (ASU-R) RID
Schmieder, B. (FR)
Heinzel, Petr (ASU-R) RID, ORCID
Anzer, U. (DE)Source Title Astronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
Roč. 514, May (2010), A43/1-A43/11Number of pages 11 s. Language eng - English Country FR - France Keywords Sun filaments ; prominences ; radiative transfer Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics R&D Projects GP205/09/P554 GA ČR - Czech Science Foundation (CSF) GA205/07/1100 GA ČR - Czech Science Foundation (CSF) 1QS300120506 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR) CEZ AV0Z10030501 - ASU-R (2005-2011) UT WOS 000280504800010 DOI 10.1051/0004-6361/200913411 Annotation 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. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2011
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