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:
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2005
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0094243X_v784_n_p582_Vasquez http://hdl.handle.net/20.500.12110/paper_0094243X_v784_n_p582_Vasquez |
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