3D Coronal Structures and Magnetic Field during a Total Solar Eclipse 29. March 2006. |
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Pavel Ambroz Submitted: 2009-07-07 02:40
The good quality of the observing sequence of about 60
photographs of the white-light corona taken during the total solar
eclipse observations on 29 March 2006, in Al Sallum, Egypt,
enable us to use a new method of image processing for enhancement
of the fine structure of coronal phenomena. We present selected
magnetic field lines derived for different parameters of the
extrapolation model. The coincidence of the observed coronal white
light fine structures and the computed field-line positions
provides a 3D causal relationship between coronal structures and
the coronal magnetic field.
Authors: P. Ambroz, M. Druckmuller, A.A. Galal, R.H. Hamid
Projects: SoHO-EIT
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Publication Status: Solar Physics, (accepted)
Last Modified: 2009-07-08 06:44
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