Calculation and Visualization of Magnetic Field in the Solar Corona during Total Solar Eclipses in 2006 and 2008

Details Calculation and Visualization of Magnetic Field in the Solar Corona during Total Solar Eclipses in 2006 and 2008 Calculation and Visualization of Magnetic Field in the Solar Corona during Total Solar Eclipses in 2006 and 2008

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ysc..conf...65s&link_type=abstract

YSC'16 Proceedings of Contributed Papers (eds. Choliy V. Ya., Ivashchenko G.), pp. 65-69

Physics

Scientific paper

Magnetic fields in the solar corona during total solar eclipses on March 29, 2006 and August 1, 2008 were calculated in the Potential Field Source Surface (PFSS) model. Observed photospheric magnetic field data from Wilcox Solar Observatory (WSO) were used. Coronal field line maps were constructed in potential classical line-of-sight and radial approximations. It was concluded that the observed structures of the solar corona during these eclipses are in good agreement with configuration of lines of magnetic force calculated using radial approximation without any polar field corrections.

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