A new technique for comparing solar dynamo models and observations
We present a new technique suitable for a detailed comparison between solar dynamo models and observations. The method is based on the technique of dynamo spectroscopy proposed by Hoyng & Schutgens (1995) and bi-orthogonal decomposition of solar data. This decomposition provides a representation...
Guardado en:
Autores principales: | Mininni, P.D., Gómez, D.O. |
---|---|
Formato: | Artículo publishedVersion |
Lenguaje: | Inglés |
Publicado: |
2004
|
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00046361_v426_n3_p1065_Mininni |
Aporte de: |
Ejemplares similares
-
A new technique for comparing solar dynamo models and observations
por: Mininni, P.D., et al. -
A new technique for comparing solar dynamo models and observations
por: Mininni, P.D., et al.
Publicado: (2004) -
A new technique for comparing solar dynamo models and observations
por: Mininni, Pablo Daniel, et al.
Publicado: (2004) -
Quasi-separatrix layers in solar flares: II. Observed magnetic configurations
por: Démoulin, P., et al. -
Quasi-separatrix layers in solar flares: II. Observed magnetic configurations
Publicado: (1997)