Solar corona magnetic structure and stagnated wind outflow
Solar observations made with the Ultraviolet Coronagraph Spectrometer (UVCS) aboard the Solar and Heliosphere Observatory (SoHO) spacecraft, have revealed that coronal protons and heavier ions have anisotropic temperature distributions. In a recent work we developed semi-empirical models for the sol...
Guardado en:
| Autor principal: | Vásquez, A.M. |
|---|---|
| Formato: | CONF |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0094243X_v784_n_p582_Vasquez |
| Aporte de: |
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