An explanation for the Stokes V asymmetry in solar faculae

Sanchez Almeida, J.; Collados, M.; del Toro Iniesta, J. C.
Referencia bibliográfica

Astronomy and Astrophysics (ISSN 0004-6361), vol. 201, no. 2, Aug. 1988, p. L37-L40.

Fecha de publicación:
8
1988
Número de autores
3
Número de autores del IAC
3
Número de citas
32
Número de citas referidas
31
Descripción
The asymmetry in the Stokes V profile observed in solar faculae can be explained by assuming that the magnetic field increases with height while downflow speed decreases. The MHD compatibility of such solution is briefly discussed together with an observational test for that possibility.