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Electron densities in quiescent prominences derived from eclipse observations
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SYSNO ASEP 0322311 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title Electron densities in quiescent prominences derived from eclipse observations Title Elektronové hustoty v klidných protuberancích odvozené z pozorování během zatmění Author(s) Jejčič, S. (SI)
Heinzel, Petr (ASU-R) RID, ORCIDSource Title Solar Physics. - : Springer - ISSN 0038-0938
Roč. 254, č. 1 (2009), s. 89-100Number of pages 12 s. Language eng - English Country NL - Netherlands Keywords prominences quiescent ; eclipse observations ; visible spectrum Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics CEZ AV0Z10030501 - ASU-R (2005-2011) UT WOS 000261577100006 DOI 10.1007/s11207-008-9289-2 Annotation Eclipse observations in white light were used to derive the elektron densities in solar prominences. Theoretical metod was developed using the set of NLTE prominence models. The nature of prominence pink color seen during the total eclipse is discussed. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2009
Number of the records: 1