Solar coronal heating: AC versus DC
The heating of the plasma confined in active regions of the solar corona is caused by the dissipation of magnetic stresses induced by the photospheric motions of the loop footpoints. The aim of the present paper is to analyze whether solar coronal heating is dominated by slow (DC) or rapid (AC) phot...
Guardado en:
| Autores principales: | Milano, L.J., Gómez, D.O., Martens, P.C. |
|---|---|
| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v490_n1PARTI_p442_Milano |
| Aporte de: |
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