3D Coronal Structures and Magnetic Field During the Total Solar Eclipse of 29 March 2006

Details 3D Coronal Structures and Magnetic Field During the Total Solar Eclipse of 29 March 2006 3D Coronal Structures and Magnetic Field During the Total Solar Eclipse of 29 March 2006

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009soph..258..243a&link_type=abstract

Solar Physics, Volume 258, Issue 2, pp.243-265

Physics

4

Eclipse Observations, Corona, Structures, Magnetic Fields, Corona

Scientific paper

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.

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