Bibcode
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 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.