Energy input flux in the global quiet-sun corona
We present first results of a novel technique that provides, for the first time, constraints on the energy input flux at the coronal base (r ∼ 1.025 R o) of the quiet Sun at a global scale. By combining differential emission measure tomography of EUV images, with global models of the coronal magneti...
Guardado en:
| Autores principales: | Mac Cormack, C., Vásquez, A.M., López Fuentes, M., Nuevo, F.A., Landi, E., Frazin, R.A. |
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| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v843_n1_p_MacCormack |
| Aporte de: |
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