A topological approach to understand a multiple-loop solar flare
We analyze the UV and X-ray data obtained by the SMM satellite for the flare starting at 02:36 UT on November 12, 1980 in AR 2779. From a detailed revision of the O v emission, we find that the observations are compatible with energy being released in a zone above the magnetic inversion line of the...
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| Autores principales: | Bagalá, L.G., Mandrini, C.H., Rovira, M.G., Démoulin, P., Hénoux, J.C. |
|---|---|
| Formato: | JOUR |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00380938_v161_n1_p103_Bagala |
| Aporte de: |
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