Articles | Volume 37, issue 3
https://doi.org/10.5194/angeo-37-405-2019
https://doi.org/10.5194/angeo-37-405-2019
Regular paper
 | 
11 Jun 2019
Regular paper |  | 11 Jun 2019

Evanescent acoustic-gravity modes in the isothermal atmosphere: systematization and applications to the Earth and solar atmospheres

Oleg K. Cheremnykh, Alla K. Fedorenko, Evgen I. Kryuchkov, and Yuriy A. Selivanov

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Cited articles

Antia, H. M.: Estimate of solar radius from f-mode, Astron. Astrophys., 330, 336–340, 1998. 
Athay, R. G.: The Solar Chromosphere and Corona: Quiet Sun, Reidel, Dordrecht, the Netherlands, 504 pp., 1976. 
Bannon, P. R.: On the anelastic approximation for a compressible atmosphere, J. Atmos. Sci., 53, 3618–3628, 1996. 
Beer, T.: Atmospheric Waves, John Wiley, New York, USA, 300 pp., 1974. 
Belashov, V. Yu.: Dynamics of nonlinear internal gravity waves at ionosphere F-region heights, Geomagn. Aeron+., 1990. 30, 637–641, 1990 (in English). 
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Short summary
The fundamental mode of oscillations of the solar atmosphere, f-mode, plays an important role in solar physics. At an early stage of observation, it was found that its frequency is related to the wavelength by a ratio characteristic of waves on the surface of deep water. Subsequent observations revealed its inaccuracy. We derived waves with a different frequency–wavelength ratio and compared them with other possible waves of this type in both the solar and terrestrial atmosphere.