References

• Agnelli G., Cacciani A., Fofi M., 1975, Solar Phys. 44, 509
• Babcock H.D., Babcock H.W., 1952, PASP 64, 282
• Beckers J.M., 1968, Solar Phys. 3, 258
• Bendlin C., Volkmer R., Kneer F., 1992, A&A 257, 817 NASA ADS
• Bonaccini D., 1988, Infrared Imaging Filter With Lithium Niobate Double Channel Fabry Perot Interferometer, NOAO Preprint, No. 179
• Cacciani A., Fofi M., 1978, Solar Phys. 59, 179
• Cacciani A., 1981, Space Sci. Rev. 29, 403
• Cacciani A., Paverani E., Smith E., Zirin H., 1991, in Solar Polarimetry, November L. (ed.). Progress Toward an Advanced Imaging Vector Magnetograph, U.S.A., p. 133
• Elmore D.F., Lites B.W., Tomcryk S., et al., 1992, in Polarization Analysis and Measurement, SPIE, 1746, 22
• Guoxiang A., Fear R.J., Peiwen J., 1990, Acta Astrophys. Sin. 10, 2, 180-187
• Hagyard M.J., Cumings N.R., West E.A., Smith J.E., 1982, Solar Phys. 80, 33 NASA ADS
• Keller C.U., Aebersold F., Egger U., et al., 1992, LEST Technical Report No. 53
• Kobanov N.I., 1983, Colar Phys. 82, 237
• Kobanov N.I.,1983, Solar Phys. 145, 11 NASA ADS
• Lebedev N.N., Grigoryev V.M., Klochek N.V., Kobanov N.I., 1972, A Method of Measuring the Magnetic Field Strength, Author's Certificate USSR No. 335562. Bull. Izobr., No. 13
• Mein P., 1991, A&A 248, 669 NASA ADS
• Mickey D.L., Canfield R.C., La Bonte B.J., et al., 1996, Solar Phys. (submitted)
• Povel H.P., Aebersold H., Stenflo J.O., 1990, Appl. Opt. 29, 1186
• Povel H.P., Keller C.U., Yadigaroglu I.A., 1994, Appl. Opt. 33, 19, 4254
• Rakuljic G.A., Leyva V., 1993, Opt. Lett. 18, 6, 459-461
• Ramsey H.E., 1971, Solar Phys. 21, 54
• Rhodes E.J.Jr., Cacciani A., Tomczyk S., et al., 1984, Adv. Space Res. 4, 103-112
• Rust D.M., 1984, Some Design Considerations for a solar magnetograph, Preprint APL/IHU 84-27
• Rust D.M., 1985, Austr. J. Phys. 38, 781
• Rust D.M., 1986, Instrum. Astron. SPIE 627, 39
• Sakurai T., Ichimoto K., Hiel E., Miyazaki H., 1991, Solar Terrestr. Environ. Res. Jap. 15, 11
• West E.A., 1985, NASA Conf. Publ. 2374, 160