The long-term evolution of AR 7978: Testing coronal heating models
We derive the dependence of the mean coronal heating rate on the magnetic flux density. Our results are based on a previous study of the plasma parameters and the magnetic flux density (B̄) in the active region NOAA 7978 from its birth to its decay, throughout five solar rotations using the Solar an...
Guardado en:
| Publicado: |
2003
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v586_n1I_p592_Demoulin http://hdl.handle.net/20.500.12110/paper_0004637X_v586_n1I_p592_Demoulin |
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