Abstract
The model calculations of 5-min solar oscillations are performed with consideration for the presence of ‘canopy’ magnetic field in the solar chromosphere. It is shown that the occurrence of Alfvén resonances for 5-min oscillations in the solar chromosphere leads on the one hand to some change of the 5-min oscillation frequencies (up to a few µHz), and on the other hand to the heating of the chromosphere. The acoustic energy flux incoming to the chromosphere is of order 1 × 10 5 erg cm-2 s-1.
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References
Ando, H. and Osaki, I.: 1977, Publ. Astron. Soc. Japan 29, 221.
Giovanelli, R. G.: 1980, Solar Phys. 68, 49.
Heyvaerts, J. and Priest, E. R.: 1984, Astron. Astrophys. 137, 63.
Ionson, J. A.: 1984, Astrophys. J. 276, 375.
Kappraff, J. M. and Tataronis, J. A.: 1977, J. Plasma Phys. 18, 209.
Kuperus, M., Ionson, J. A., and Spicer, D. S.: 1982, Ann. Rev. Astron. Astrophys. 19, 7.
Libbrecht, K. J.: 1988, Astrophys. J. 334, 510.
Mein, P., Mein, N., and Schmieder, B.: 1980, in F. Moriyama and J. C. Hénoux (eds.), Proc. Japan- France Seminar on Solar Physics, p. 70.
Rae, I. C. and Roberts, B.: 1982, Monthly Notices Roy. Astron. Soc. 1201, 1171.
Spruit, H. C.: 1981, in Jordan (ed.), The Sun as the Star, p. 385.
Tataronis, J. A.: 1975, J. Plasma Phys. 13, 87.
Toomre, J.: 1986, in Gough (ed.), Seismology of the Sun and the Distant Stars, p. 1.
Zhughda, Y. D.: 1972, Solar Phys. 25, 329.
Zhukov, V. I.: 1989, Astron. Astrophys. 222, 293.
Zhukov, V. I.: 1990, Astophys. Space Sci. 174, 173.
Zhukov, V. I.: 1992, Solar Phys. 139, 201.
Zhukov, V. I.: 1996, Astron. Astrophys., in press.
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Zhukov, V.I. THE RESONANT ABSORPTION OF 5-MIN OSCILLATIONS IN THE SOLAR ATMOSPHERE. Solar Physics 173, 15–24 (1997). https://doi.org/10.1023/A:1004958120915
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DOI: https://doi.org/10.1023/A:1004958120915