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3D Coronal Structures and Magnetic Field During the Total Solar Eclipse of 29 March 2006
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SYSNO ASEP 0333718 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title 3D Coronal Structures and Magnetic Field During the Total Solar Eclipse of 29 March 2006 Author(s) Ambrož, Pavel (ASU-R) RID, ORCID
Druckmüller, M. (CZ)
Galal, A.A. (EG)
Hamid, R.H. (EG)Source Title Solar Physics. - : Springer - ISSN 0038-0938
Roč. 258, č. 2 (2009), s. 243-265Number of pages 13 s. Language eng - English Country NL - Netherlands Keywords Sun ; eclipse observations ; corona Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics R&D Projects IAA300030506 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR) IAA300030808 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR) CEZ AV0Z10030501 - ASU-R (2005-2011) UT WOS 000269008700005 DOI 10.1007/s11207-009-9413-y Annotation Selected magnetic field lines were derived for different parameters of the extrapolation numerical model. The coincidence of the observed coronal white light fine structures and the computed field lines positron provides a 3-D causal relationship between coronal structures and the coronal magnetic field. Processed images of the solar white light corona with excelent spatial resolution were taken by authors during the total solar elipse observations on March 29, 2006 in Egypt. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2010
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