2014
DOI: 10.1121/1.4902426
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Dissipation of acoustic-gravity waves: An asymptotic approach

Abstract: Acoustic-gravity waves in the middle and upper atmosphere and long-range propagation of infrasound are strongly affected by air viscosity and thermal conductivity. To characterize the wave dissipation, it is typical to consider idealized environments, which admit plane-wave solutions. Here, an asymptotic approach is developed that relies instead on the assumption that spatial variations of environmental parameters are gradual. It is found that realistic assumptions about the atmosphere lead to rather different… Show more

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Cited by 20 publications
(23 citation statements)
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References 17 publications
(30 reference statements)
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“…Acoustic‐gravity waves (AGWs) in the atmosphere have the dispersion relation [ Godin , , ] m2=ωd2cs2γ2g24cs4k2[]1()γ1g2ωd2cs2, where c s and u are the sound speed and wind velocity, γ ≈ 1.4 is the ratio of specific heats in air at constant pressure and constant volume, ( k x , k y , m ) and ω are the AGW wave vector and frequency, k = ( k x , k y , 0) is the horizontal wave vector, and ω d = ω − k · u is the intrinsic frequency. Here we disregard the effect of dissipative processes on the AGW dispersion relation.…”
Section: Properties Of Atmospheric Wavesmentioning
confidence: 99%
“…Acoustic‐gravity waves (AGWs) in the atmosphere have the dispersion relation [ Godin , , ] m2=ωd2cs2γ2g24cs4k2[]1()γ1g2ωd2cs2, where c s and u are the sound speed and wind velocity, γ ≈ 1.4 is the ratio of specific heats in air at constant pressure and constant volume, ( k x , k y , m ) and ω are the AGW wave vector and frequency, k = ( k x , k y , 0) is the horizontal wave vector, and ω d = ω − k · u is the intrinsic frequency. Here we disregard the effect of dissipative processes on the AGW dispersion relation.…”
Section: Properties Of Atmospheric Wavesmentioning
confidence: 99%
“…, c 0 is the sound speed, H is the scale height, g is the gravitational acceleration, ω 0 = ω À k Á u = ω À k x u x À k y u y , and u x and u y are the zonal and meridional components of the background neutral wind [Godin, 2015]. In practice, thermospheric AGWs can have a considerable imaginary component of k z , both because there are large spatial regions where they may exist as evanescent waves and because of the viscous attenuation [Godin, 2014]. If a wave is in the shadow zone (this happens when the expression under radical sign in equation (10) is negative), it is still observable, but equation (9) is not valid: vertical gradient of the phase determines a different physical quantity.…”
Section: 1002/2016ja022495mentioning
confidence: 99%
“…AGWs of oceanic origin, and especially the AGWs radiated by IGWs in deep water, are characterized by considerably higher horizontal phase speeds, which can exceed the maximum wind speeds. This leads to larger horizontal spatial scales and, correspondingly, to weaker viscous absorption (Godin 2014). Fast AGWs do not have critical levels and escape the critical level filtering (Hines 1960;Gossard and Hooke 1975).…”
Section: Observationsmentioning
confidence: 99%