Abstract
A magneto-optical filter was built to establish its utility for measuring solar oscillations. A theoretical model is described and the asymptotic behaviour of the Faraday effect in the filter is deduced. Experimental work confirms to first order the asymptotic model.
Similar content being viewed by others
References
Agnelli, G., Cacciani, A., and Fofi, M.: 1975, Solar Phys. 44, 509.
Cimino, M., Cacciani, A., and Fofi, M.: 1970, Solar Phys. 11, 319.
Fossat, E., Gelly, B., and Grec, G.: 1986, in D. O. Gough (ed.), Seismology of the Sun and the Distant Stars, NATO Series, J.Vol. 169, p. 405.
Litvak, M.: 1985, in Selection of a Wavelength Analyzer for a Solar Oscillations Imaging Experiment, Section 6, JPL D-2018.
Rachkowsky, D. N.: 1962, Izv. Krymsk. Astrofiz. Obs. 27, 148.
Rhodes, E. J. Jr., Cacciani, A., Tomczyk, S., and Ulrich, R. K.: 1986a, in D. O. Gough (ed.), Seismology of the Sun and the Distant Stars, NATO Series, Vol. 169, p. 309.
Rhodes, E. J., Jr., Cacciani, A., and Tomczyk, S.: 1986b, in D. O. Gough (ed.), Seismology of the Sun and the Distant Star, NATO Series, Vol. 169, p. 359.
Yeh, P.: 1982, Applied Opt. 21, 2069.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Appourchaux, T. The Faraday effect in a magneto-optical filter. Sol Phys 109, 393–397 (1987). https://doi.org/10.1007/BF00160662
Received:
Revised:
Issue Date:
DOI: https://doi.org/10.1007/BF00160662