Can we extrapolate a magnetic field when its topology is complex?
In order to understand various solar phenomena controlled by the magnetic field, such as X-ray bright points, flares and prominence eruptions, the structure of the coronal magnetic field must be known. This requires a precise extrapolation of the photospheric magnetic field. Presently, only potentia...
Guardado en:
| Autores principales: | Démoulin, P., Hénoux, J.C., Mandrini, C.H., Priest, E.R. |
|---|---|
| Formato: | JOUR |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00380938_v174_n1-2_p73_Demoulin |
| Aporte de: |
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