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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Published in | Solar physics Vol. 277; no. 1; pp. 131 - 151 |
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Main Author | |
Format | Journal Article |
Language | English |
Published |
Dordrecht
Springer Netherlands
01.05.2012
Springer Nature B.V |
Subjects | |
Online Access | Get full text |
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