Source Surface Radius and its Development During Solar Cycle

Details Source Surface Radius and its Development During Solar Cycle Source Surface Radius and its Development During Solar Cycle

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..370..255b&link_type=abstract

Solar and Stellar Physics Through Eclipses ASP Conference Series, Vol. 370, proceedings of the conference held 27-29 March, 2006

Physics

Scientific paper

The source surface radius, at which the coronal magnetic field is considered to be radial, plays an important role in the current solar coronal magnetic field modeling. Its value affects shapes of computed magnetic structures. Total solar eclipse pictures of corona, processed by a special numerical method, show very faint structures, extended from chromosphere to 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 present values of the source surface radius for 8 eclipses and the evolution of source surface radius during a solar activity cycle.

Affiliated with

Also associated with

No associations

Rating

Source Surface Radius and its Development During Solar Cycle does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Source Surface Radius and its Development During Solar Cycle, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Source Surface Radius and its Development During Solar Cycle will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-765554