Development of Source Surface Radius during Solar Cycles

Details Development of Source Surface Radius during Solar Cycles Development of Source Surface Radius during Solar Cycles

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008espm...122.111b&link_type=abstract

"12th European Solar Physics Meeting, Freiburg, Germany, held September, 8-12, 2008. Online at http://espm.kis.uni-freiburg.de/,

Physics

Scientific paper

The source surface radius presents one of the boundary condition in the modeling of solar coronal magnetic field. Its value affect the shape of the computed coronal magnetic structures. The pictures of solar corona obtained during total solar eclipses and processed by special numerical method, show very faint structures, extended to the several solar radii. Under the assumption that these structures represent a real magnetic situation in the corona, a value of the source surface radius can be estimated through the analysis of their shapes. We discuss some problems of calculation of its values and the evolution of source surface radius during solar activity cycle.

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