Počet záznamů: 1
2D radiative-magnetohydrostatic model of a prominence observed by Hinode, SoHO/SUMER and Meudon/MSDP
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SYSNO ASEP 0365396 Druh ASEP J - Článek v odborném periodiku Zařazení RIV J - Článek v odborném periodiku Poddruh J Článek ve WOS Název 2D radiative-magnetohydrostatic model of a prominence observed by Hinode, SoHO/SUMER and Meudon/MSDP Tvůrce(i) Berlicki, Arkadiusz (ASU-R) RID
Gunár, Stanislav (ASU-R) RID, ORCID
Heinzel, Petr (ASU-R) RID, ORCID
Schmieder, B. (FR)
Schwartz, Pavol (ASU-R) RIDCelkový počet autorů 5 Zdroj.dok. Astronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
Roč. 530, May (2011), A143/1-A143/13Poč.str. 13 s. Jazyk dok. eng - angličtina Země vyd. FR - Francie Klíč. slova Sun ; atmosphere ; filaments Vědní obor RIV BN - Astronomie a nebeská mechanika, astrofyzika CEP GAP209/10/1680 GA ČR - Grantová agentura ČR GP205/09/P554 GA ČR - Grantová agentura ČR GAP209/10/1706 GA ČR - Grantová agentura ČR CEZ AV0Z10030501 - ASU-R (2005-2011) UT WOS 000291027400143 DOI 10.1051/0004-6361/201015896 Anotace 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. Pracoviště Astronomický ústav Kontakt Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Rok sběru 2012
Počet záznamů: 1