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Analytical description of nonlinear acoustic waves in the solar chromosphere

Abstract
Vertical propagation of acoustic waves of finite amplitude in an isothermal, gravitationally stratified atmosphere is considered. Methods. Methods of nonlinear acoustics are used to derive a dispersive solution, which is valid in a long-wavelength limit, and a non-dispersive solution, which is valid in a short-wavelength limit. The influence of the gravitational field on wave-front breaking and shock formation is described. The generation of a second harmonic at twice the driving wave frequency, previously detected in numerical simulations, is demonstrated analytically. Results. Application of the results to three-minute chromospheric oscillations, driven by velocity perturbations at the base of the solar atmosphere, is discussed. Numerical estimates suggest that the second harmonic signal should be detectable in an upper chromosphere by an instrument such as the Fast Imaging Solar Spectrograph installed at the 1.6-m New Solar Telescope of the Big Bear Observatory.
Type
Journal Article
Type of thesis
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Citation
Litvinenko, Y. E., & Chae, J. (2017). Analytical description of nonlinear acoustic waves in the solar chromosphere. Astronomy and Astrophysics, 599. https://doi.org/10.1051/0004-6361/201629568
Date
2017
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Supervisors
Rights
This article has been published in the Astronomy and Astrophysics. © 2017 ESO.