Modeling static magnetic field structures in solar corona

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 pr...

Full description

Bibliographic Details
Main Author: Čadež V.M.
Format: Article
Language:English
Published: Astronomical Observatory, Department of Astronomy, Belgrade 2005-01-01
Series:Serbian Astronomical Journal
Subjects:
Online Access:http://www.doiserbia.nb.rs/img/doi/1450-698X/2005/1450-698X0571001C.pdf