Determining the Solar Source of a Magnetic Cloud Using a Velocity Difference Technique
For large eruptions on the Sun, it is often a problem that the core dimming region cannot be observed due to the bright emission from the flare itself. However, spectroscopic data can provide the missing information through the measurement of Doppler velocities. In this paper we analyse the well-stu...
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| Autores principales: | Harra, L.K., Mandrini, C.H., Dasso, S., Gulisano, A.M., Steed, K., Imada, S. |
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| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00380938_v268_n1_p213_Harra |
| Aporte de: |
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