Magnetic Energy Storage and Current Density Distributions for Different Force-Free Models

In the last decades, force-free-field modelling has been used extensively to describe the coronal magnetic field and to better understand the physics of solar eruptions at different scales. Especially the evolution of active regions has been studied by successive equilibria in which each computed ma...

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Bibliographic Details
Published inSolar physics Vol. 277; no. 1; pp. 131 - 151
Main Author Regnier, S
Format Journal Article
LanguageEnglish
Published Dordrecht Springer Netherlands 01.05.2012
Springer Nature B.V
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