Abstract
Global oscillation of the Sun with a period of 160 rain were first discovered in 1974 and since observed in Crimea during the last 6 years; they were confirmed, in 1976–1979, by Doppler measurements at Stanford (Scherrer et al., 1980) and quite recently by observations of Fossat and Grec at the south geographic pole. The average amplitude of the oscillation is about 0.5 m s-1. The phase shows remarkable stability at the period 160.010 min and good agreement between different sites on the Earth; therefore, this oscillation should now be recognized as definitely of solar origin. It is probably accompanied by synchronous fluctuations in the IR brightness and radio-emission of the Sun, and exhibits a dependence of the amplitude on the phase of solar rotation (with a peak of power at 27.2 days).
In agreement with results of the Birmingham group and the South Pole observation we also find evidence in favour of a discrete spectrum within the 5 min global oscillations of the Sun, with the average splitting of about 69.5 μHz in frequency.
Strict gas-dynamical equations being solved in the adiabatic approximation for a polytropic sphere n = 3 display the pattern of radial oscillations with wave packets separated by 120 m time-intervals filled with high frequency (and split by 117 μHz) oscillations implying a similarity with the observed pattern.
Similar content being viewed by others
References
Brookes, J. R., Isaak, G. R., and van der Raay, H. B.: 1976, Nature 259, 92.
Christensen-Dalsgaard, J. and Gough, D. O.: 1976, Nature 259, 89.
Claverie, A., Isaak, G. R., McLeod, C. P., van der Raay, H. B., and Roca Cortes, T.: 1979, Nature 282, 591.
Dittmer, P. H.: 1977, Thesis, Stanford Univ. IPR Report No. 686.
Eryushev, N. N., Kotov, V. A., Severny, A. B., and Tsvetkov, L. I.: 1979, Astron. Zh. Pis'ma (USSR) 5, 546.
Fossat, E. and Grec, G.: 1978, in Proc. 2nd European Meeting on Solar Physics, ‘Pleins Feux sur la Physique Solaire’, Toulouse, 1978, p. 151.
Fossat, E., Grec, G., Kotov, V. A., Severny, A. B., and Tsap, T. T.: 1980, Monthly Notices Roy. Astron. Soc. (submitted).
Fossat, E., Grec, G., and Pomerantz, M.: 1981, Solar Phys. 74, 59 (this volume).
Gough, D. O.: 1979, in Proc. Workshop on Nonradial and Nonlinear Stellar Pulsations, Tucson.
Grec, G. and Fossat, E.: 1979, Astron. Astrophys. 77, 351.
Kosovichev, A. G. and Popov, Ju. P.: 1979, J. Vichisl. Matem. Fisiki USSR 19, 1253.
Kosovichev, A. G. and Severny, A. B.: 1981, Astron. Zh. Piśma (USSR) 7, 304.
Kotov, V. A. and Koutchmy, S.: 1979, Uspechi Fiz. Nauk (USSR) 128, 730.
Kotov, V. A., Severny, A. B., and Tsap, T. T.: 1978, Monthly Notices Roy. Astron. Soc. 183, 61.
Koutchmy, S., Koutchmy, O., and Kotov, V. A.: 1980, Astron. Astrophys. 90, 372.
Scherrer, P. H., Wilcox, J. M., Severny, A. B., Kotov, V. A., and Tsap, T. T.: 1980, Astrophys. J. 237, L97.
Severny, A. B., Kotov, V. A., and Tsap, T. T.: 1976, Nature 259, 87.
Severny, A. B., Kotov, V. A., and Tsap, T. T.: 1980, Astron. Astrophys. 88, 317.
Author information
Authors and Affiliations
Additional information
Proceedings of the 14th ESLAB Symposium on Physics of Solar Variations, 16–19 September 1980, Scheveningen, The Netherlands.
Rights and permissions
About this article
Cite this article
Severny, A.B., Kotov, V.A. & Tsap, T.T. Present state of the study of 160-minutes solar oscillation. Sol Phys 74, 65–71 (1981). https://doi.org/10.1007/BF00151275
Issue Date:
DOI: https://doi.org/10.1007/BF00151275