Abstract
Time series of the nonsplit Fei 7090 Å line have been observed in several sunspots with a 100 x 100 diode array corresponding to 48 arc sec times 1.39 Å. The spatial behaviour of Doppler motions along one fixed slit position has been studied as a function of time. Former results are confirmed, that the power in the five minute range decreases from the photosphere to the umbra, where, however, values still well above the noise level are measured. Regarding the penumbra, the power tends to exhibit a maximum at locations where the line-of-sight component of a radial horizontal field should be maximal. This indicates that the direction of the oscillatory velocities might be influenced by the magnetic field or the Evershed flow. No significant power is found in the 3 min range. An exception might be seen in a small patch at the limb of the umbra of one spot.
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Abdelatif, T. E. and Thomas, J. H.: 1987, Astrophys. J. 320, 884.
Abdelatif, T. E., Lites, B. W., and Thomas, J. H.: 1986, Astrophys. J. 311, 1015.
Balthasar, H., Fangmeier, E., Küveler, G., and Wiehr, E.: 1986, in J. Christensen-Dalsgaard and S. Frandsen (eds.), ‘Advances in Helio- and Asteroseismology’, IAU Symp. 123 (in press).
Balthasar, H. and Wiehr, E.: 1984, Solar Phys. 94, 99.
Beckers, J. M. and Schultz, R. B.: 1972, Solar Phys. 27, 61.
Bhatnagar, A., Livingston, W. C., and Harvey, J. W.: 1972, Solar Phys. 27, 80.
Canfield, R. C.: 1976, Solar Phys. 50, 239.
Groth, E. J.: 1975, Astrophys. J. Suppl. 29, 285.
Gurman, J. B.: 1987, Solar Phys. 108, 61.
Hasan, S. S. and Sobouti, Y.: 1987, Monthly Notices Roy. Astron. Soc. 228, 427.
Koch, A., Küveler, G., and Schröter, E. H.: 1979, Solar Phys. 64, 13.
Küveler, G. and Wiehr, E.: 1985, Astron. Astrophys. 142, 205.
Küveler, G. and Wöhl, H.: 1983, Astron. Astrophys. 122, 69.
Lites, B. W.: 1986a, Astrophys. J. 301, 922.
Lites, B. W.: 1986b, Astrophys. J. 301, 1005.
Lites, B. W. and Thomas, J. H.: Astrophys. J. 294, 682.
Livingston, W. C. and Mahaffay, C.: 1981, in L. E. Cram and J. H. Thomas (eds.), The Physics of Sunspots, Sacramento Peak Conference, p. 112.
Pallé, P. L., Perez, J. C., Régulo, C., Roca Cortes, T., Isaak, G. R., McLeod, C. P., and van der Raay, H. B.: 1986, Astron. Astrophys. 169, 313.
Rice, B. J. and Gaizauskas, V.: 1973, Solar Phys. 32, 421.
Schröter, E. H. and Soltau, D.: 1976, Astron. Astrophys. 49, 463.
Soltau, D. and Wiehr, E.: 1984, Astron. Astrophys. 123, 263.
Soltau, D., Schröter, E. H., and Wöhl, H.: 1976, Astron. Astrophys. 50, 367.
Staude, J., Žugžda, Y. D., and Locans, V.: 1985, Solar Phys. 95, 37.
Staude, J., Žugžda, Y. D., and Locans, V.: 1987, 10th IAU European Regional Astronomical Meeting, Prague (in press).
Thomas, J. H., Lites, B. W., Gurman, J. B., and Ladd, E. F.: 1987, Astrophys. J. 312, 457.
von Uexküll, M., Kneer, F., and Mattig, W.: 1983, Astron. Astrophys. 123, 263.
Wiehr, E.: 1986, in E. H. Schröter, M. Vázquez, and A. Whyller (eds.), Proceedings of the Inaugural Workshop for the D-E-S Telescope Installations on the Canary Islands (in press).
Wiehr, E. and Stellmacher, G.: 1984, in R. Müller (ed.), High Resolution in Solar Physics, Toulouse, p. 254.
Wiehr, E., Wittmann, A., and Wöhl, H.: 1980, Solar Phys. 68, 207.
Žugžda, Y. D., Staude, J., and Locans, V.: 1984, Solar Phys. 91, 219.
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Balthasar, H., Küveler, G. & Wiehr, E. A comparison of the oscillations in sunspot umbrae, penumbrae, and the surrounding photosphere. Sol Phys 112, 37–48 (1987). https://doi.org/10.1007/BF00148485
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DOI: https://doi.org/10.1007/BF00148485