Validation of two MHD models of the solar corona with rotational tomography
We demonstrate a validation of two 3D MHD models of the corona by comparing density values from solar rotational tomography (SRT) to densities and morphological properties of the two MHD solutions for CR 2029 (2005 April 21-May 18). The two MHD models are given by the Stanford and Michigan models, a...
Guardado en:
| Publicado: |
2008
|
|---|---|
| Materias: | |
| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v682_n2_p1328_Vasquez http://hdl.handle.net/20.500.12110/paper_0004637X_v682_n2_p1328_Vasquez |
| Aporte de: |
Ejemplares similares
-
Validation of two MHD models of the solar corona with rotational tomography
por: Vasquez, A.M., et al. -
The solar minimum corona from differential emission measure tomography
Publicado: (2010) -
The solar minimum corona from differential emission measure tomography
por: Vásquez, A.M., et al. -
The effect of proton temperature anisotropy on the solar minimum corona and wind
Publicado: (2003) -
The effect of proton temperature anisotropy on the solar minimum corona and wind
por: Vásquez, A.M., et al.