Abstract
Proper periods are calculated for oscillations of an isothermal gaseous layer with a homogeneous vertical magnetic field, limited by two rigid horizontal boundaries. The obtained results are in good agreement with the observed umbral oscillations in a sunspot.
Similar content being viewed by others
References
Gurman, J.B. and Leibacher, J.W.: 1984, Ap. J. 283, 959.
Leroy, B. and Schwartz, St.J.: 1982, Astr. Ap. 112, 84.
Lites, B.W. and Thomas, J.H.: 1985, Ap. J. 294, 682.
Scheuer, M.A. and Thomas, J.H.: 1981, Solar Phys. 71, 21.
Thomas, J.H. and Scheuer, M.A.: 1982, Solar Phys. 79, 19.
Thomas, J.H.: 1984, Astr. Ap. 135, 188.
Thomas, J.H.: 1985, Astr. Austr. J. Phys. 38, 811.
Uchida, Y. and Sakurai, T.: 1975, Publ. Astron. Soc. Japan 27, 259.
Zhugzhda, Yu.D.: 1979, Astron. Zhurn. 56, 74 (in Russian).
Zugzda, Y.D., Locans, V., and Staude, J.: 1983, Solar Phys. 82, 369.
Zugzda, Y.D., Staude, J., and Locans, V.: 1984, Solar Phys. 91, 219.
Zugzda, Y.D., Locans, V., and Staude, J.: 1985, Astr. Ap. 143, 201.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Zhukov, V.I., Efremov, V.I. & Nuraliev, B.T. The spectrum of umbral oscillations of the Scheuer-Thomas sunspot model. Sol Phys 109, 403–404 (1987). https://doi.org/10.1007/BF00160664
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00160664