Inversion Techniques Applied to Sunspot Spectropolarimetric Data

Bibcode
1997ASPC..118..197W
Westendorp Plaza, C.; del Toro Iniesta, J. C.; Ruiz Cobo, B.; Martinez Pillet, V.; Lites, B. W.; Skumanich, A.
Referencia bibliográfica

1st Advances in Solar Physics Euroconference. Advances in Physics of Sunspots, ASP Conf. Ser. Vol. 118., Eds.: B. Schmieder, J.C. del Toro Iniesta, & M. Vazquez, p. 197.

Fecha de publicación:
0
1997
Número de autores
6
Número de autores del IAC
0
Número de citas
7
Número de citas referidas
6
Descripción
Two inversion techniques are compared: the Unno-Rachkov-sky fitting method (UR) and the Stokes Inversion based on Response functions (SIR). Results with synthetic profiles in sunspot model atmospheres and real data show that whilst UR is well suited for recovering a constant vec B, SIR enables us to know the run with depth of vec B and the line of sight velocity together with the temperature stratification.
Tipo
Sin árbitro
Manchas solares
Campos magnéticos

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