Bibcode
Sanchez Almeida, J.; Collados, M.; del Toro Iniesta, J. C.; Solanki, S. K.
Referencia bibliográfica
Astronomy and Astrophysics (ISSN 0004-6361), vol. 196, no. 1-2, May 1988, p. 266-268.
Fecha de publicación:
5
1988
Número de citas
12
Número de citas referidas
12
Descripción
The "line ratio method" (Stenflo, 1973) has been extensively used in the
past to carry out measurements of the magnetic field strength in
spatially unresolved magnetic flux concentrations. The authors present
here a new variant of this technique, which is particularly simple as it
does not depend on any radiative transfer calculations and thus the
assumption of a model atmosphere is not required. General properties of
the transfer equation lead to a relationship between the circular
polarization generated by two lines which are identical except for their
Landé factors. This can be used to directly determine the field
strength from the measured line profiles. In order to test the method
the authors have applied it to experimental data. A comparison with the
traditional line ratio method is shown.