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3D Coronal Structures and Magnetic Field During the Total Solar Eclipse of 29 March 2006
- 1.0333718 - ASÚ 2010 RIV NL eng J - Journal Article
Ambrož, Pavel - Druckmüller, M. - Galal, A.A. - Hamid, R.H.
3D Coronal Structures and Magnetic Field During the Total Solar Eclipse of 29 March 2006.
Solar Physics. Roč. 258, č. 2 (2009), s. 243-265. ISSN 0038-0938. E-ISSN 1573-093X
R&D Projects: GA AV ČR IAA300030506; GA AV ČR IAA300030808
Institutional research plan: CEZ:AV0Z10030501
Keywords : Sun * eclipse observations * corona
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
Impact factor: 3.628, year: 2009
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.
Permanent Link: http://hdl.handle.net/11104/0178643
Number of the records: 1