On the Frequency of Internal Gravity Waves in the Atmosphere: Comparing Theory with Observations

This paper is devoted to the dynamics of the propagation of non-planetary scale internal gravity waves (IGWs) in the stratified atmosphere. We consider the system of equations describing internal gravity waves in three approximations: (1) the incompressible fluid approximation, (2) the anelastic gas...

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Main Authors: Robert G. Zakinyan, Alaa H. Kamil, Vladislav A. Svetlichny, Arthur R. Zakinyan
Format: Article
Language:English
Published: MDPI AG 2025-01-01
Series:Atmosphere
Subjects:
Online Access:https://www.mdpi.com/2073-4433/16/1/73
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author Robert G. Zakinyan
Alaa H. Kamil
Vladislav A. Svetlichny
Arthur R. Zakinyan
author_facet Robert G. Zakinyan
Alaa H. Kamil
Vladislav A. Svetlichny
Arthur R. Zakinyan
author_sort Robert G. Zakinyan
collection DOAJ
description This paper is devoted to the dynamics of the propagation of non-planetary scale internal gravity waves (IGWs) in the stratified atmosphere. We consider the system of equations describing internal gravity waves in three approximations: (1) the incompressible fluid approximation, (2) the anelastic gas (compressible fluid) approximation, and (3) a new approximation called the non-Boussinesq gas approximation. For each approximation, a different dispersion relation is given, from which it follows that the oscillation frequency of internal gravity waves depends on the direction of propagation, the horizontal and vertical components of the wave vector, the vertical gradient of the background temperature, and the background wind shear. In each of the three cases, the maximum frequency of internal gravity waves is different. Moreover, in the anelastic gas approximation, the maximum frequency is equal to the Brunt–Väisälä buoyancy frequency, and in the incompressible fluid approximation, it is larger than the Brunt–Väisälä frequency by a factor of <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><msqrt><mn>7</mn></msqrt><mo>≅</mo><mn>2.6</mn></mrow></semantics></math></inline-formula>. In the model proposed in this paper, the value of the maximum frequency of internal gravity waves occupies an intermediate position between the above limits. The question arises: which of the above fluid representations adequately describe the dynamics of internal gravity waves? This paper compares the above theories with observational data and experiments.
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spelling doaj-art-4b46066d623b4cdfa168a0a2cd2b56a12025-01-24T13:21:55ZengMDPI AGAtmosphere2073-44332025-01-011617310.3390/atmos16010073On the Frequency of Internal Gravity Waves in the Atmosphere: Comparing Theory with ObservationsRobert G. Zakinyan0Alaa H. Kamil1Vladislav A. Svetlichny2Arthur R. Zakinyan3Department of Theoretical and Mathematical Physics, North-Caucasus Federal University, 355017 Stavropol, RussiaDepartment of Physics, University of Misan, Amarah 62001, IraqDepartment of Theoretical and Mathematical Physics, North-Caucasus Federal University, 355017 Stavropol, RussiaDepartment of Theoretical and Mathematical Physics, North-Caucasus Federal University, 355017 Stavropol, RussiaThis paper is devoted to the dynamics of the propagation of non-planetary scale internal gravity waves (IGWs) in the stratified atmosphere. We consider the system of equations describing internal gravity waves in three approximations: (1) the incompressible fluid approximation, (2) the anelastic gas (compressible fluid) approximation, and (3) a new approximation called the non-Boussinesq gas approximation. For each approximation, a different dispersion relation is given, from which it follows that the oscillation frequency of internal gravity waves depends on the direction of propagation, the horizontal and vertical components of the wave vector, the vertical gradient of the background temperature, and the background wind shear. In each of the three cases, the maximum frequency of internal gravity waves is different. Moreover, in the anelastic gas approximation, the maximum frequency is equal to the Brunt–Väisälä buoyancy frequency, and in the incompressible fluid approximation, it is larger than the Brunt–Väisälä frequency by a factor of <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><msqrt><mn>7</mn></msqrt><mo>≅</mo><mn>2.6</mn></mrow></semantics></math></inline-formula>. In the model proposed in this paper, the value of the maximum frequency of internal gravity waves occupies an intermediate position between the above limits. The question arises: which of the above fluid representations adequately describe the dynamics of internal gravity waves? This paper compares the above theories with observational data and experiments.https://www.mdpi.com/2073-4433/16/1/73internal gravity wavesdispersion relationBrunt–Väisälä frequencyTaylor–Goldstein equationphase velocitygravity wave breaking
spellingShingle Robert G. Zakinyan
Alaa H. Kamil
Vladislav A. Svetlichny
Arthur R. Zakinyan
On the Frequency of Internal Gravity Waves in the Atmosphere: Comparing Theory with Observations
Atmosphere
internal gravity waves
dispersion relation
Brunt–Väisälä frequency
Taylor–Goldstein equation
phase velocity
gravity wave breaking
title On the Frequency of Internal Gravity Waves in the Atmosphere: Comparing Theory with Observations
title_full On the Frequency of Internal Gravity Waves in the Atmosphere: Comparing Theory with Observations
title_fullStr On the Frequency of Internal Gravity Waves in the Atmosphere: Comparing Theory with Observations
title_full_unstemmed On the Frequency of Internal Gravity Waves in the Atmosphere: Comparing Theory with Observations
title_short On the Frequency of Internal Gravity Waves in the Atmosphere: Comparing Theory with Observations
title_sort on the frequency of internal gravity waves in the atmosphere comparing theory with observations
topic internal gravity waves
dispersion relation
Brunt–Väisälä frequency
Taylor–Goldstein equation
phase velocity
gravity wave breaking
url https://www.mdpi.com/2073-4433/16/1/73
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