Modeling Static Magnetic Field Structures in Solar Corona

Details Modeling Static Magnetic Field Structures in Solar Corona Modeling Static Magnetic Field Structures in Solar Corona

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005seraj.171....1c&link_type=abstract

Serbian Astronomical Journal, Vol. 171, p. 1-10.

Astronomy and Astrophysics

Astronomy

Sun: Magnetic Fields, Sun: Corona

Scientific paper

We give an overview of procedures to recover and simulate typical coronal static magnetic field topologies from given boundary data on the photosphere. Relatively simple analytical treatments allow for solutions representing magnetic structures that are invariant in one coordinate, and satisfying prescribed boundary conditions. Starting from elementary active regions in a form of localized sources/sinks of magnetic field lines on the photospheric level, we set up various composed boundary conditions which yield complex magnetic structures in the corona above.

Affiliated with

Also associated with

No associations

Rating

Modeling Static Magnetic Field Structures in Solar Corona 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 Modeling Static Magnetic Field Structures in Solar Corona, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modeling Static Magnetic Field Structures in Solar Corona will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1460274