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2D radiative-magnetohydrostatic model of a prominence observed by Hinode, SoHO/SUMER and Meudon/MSDP
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SYSNO ASEP 0365396 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title 2D radiative-magnetohydrostatic model of a prominence observed by Hinode, SoHO/SUMER and Meudon/MSDP Author(s) Berlicki, Arkadiusz (ASU-R) RID
Gunár, Stanislav (ASU-R) RID, ORCID
Heinzel, Petr (ASU-R) RID, ORCID
Schmieder, B. (FR)
Schwartz, Pavol (ASU-R) RIDNumber of authors 5 Source Title Astronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
Roč. 530, May (2011), A143/1-A143/13Number of pages 13 s. Language eng - English Country FR - France Keywords Sun ; atmosphere ; filaments Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics R&D Projects GAP209/10/1680 GA ČR - Czech Science Foundation (CSF) GP205/09/P554 GA ČR - Czech Science Foundation (CSF) GAP209/10/1706 GA ČR - Czech Science Foundation (CSF) CEZ AV0Z10030501 - ASU-R (2005-2011) UT WOS 000291027400143 DOI 10.1051/0004-6361/201015896 Annotation Prominences observed by Hinode show very dynamical and intriguing structures. To understand the mechanisms that are responsible for these moving structures, it is important to know the physical conditions that prevail in fine-structure threads. In the present work we analyse a quiescent prominence with fine structures, which exhibits dynamic behaviour, which was observed in the hydrogen Hα line with Hinode/SOT, Meudon/MSDP and Ondˇrejov/HSFA2, and simultaneously in hydrogen Lyman lines with SoHO/SUMER during a coordinated campaign. We derive the fine-structure physical parameters of this prominence and also address the questions of the role of the magnetic dips and of the interpretation of the flows. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2012
Number of the records: 1