Готові списки джерел за темами / Atmospheric waves; Gravity waves; Thermosphere

Добірка наукової літератури з теми "Atmospheric waves; Gravity waves; Thermosphere"

Автор: Grafiati
Опубліковано: 10 грудня 2022
Оновлено: 28 січня 2023

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Статті в журналах з теми "Atmospheric waves; Gravity waves; Thermosphere"

1

Nishida, Kiwamu, Naoki Kobayashi, and Yoshio Fukao. "Background Lamb waves in the Earth's atmosphere." Geophysical Journal International 196, no. 1 (November 5, 2013): 312–16. http://dx.doi.org/10.1093/gji/ggt413.

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Abstract Lamb waves of the Earth's atmosphere in the millihertz band have been considered as transient phenomena excited only by large events. Here, we show the first evidence of background Lamb waves in the Earth's atmosphere from 0.2 to 10 mHz, based on the array analysis of microbarometer data from the USArray in 2012. The observations suggest that the probable excitation source is atmospheric turbulence in the troposphere. Theoretically, their energy in the troposphere tunnels into the thermosphere at a resonant frequency via thermospheric gravity wave, where the observed amplitudes indeed take a local minimum. The energy leak through the frequency window could partly contribute to thermospheric wave activity.
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2

Jesch, David, Alexander S. Medvedev, Francesco Castellini, Erdal Yiğit, and Paul Hartogh. "Density Fluctuations in the Lower Thermosphere of Mars Retrieved From the ExoMars Trace Gas Orbiter (TGO) Aerobraking." Atmosphere 10, no. 10 (October 15, 2019): 620. http://dx.doi.org/10.3390/atmos10100620.

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The upper atmosphere of Mars is constantly perturbed by small-scale gravity waves propagating from below. As gravity waves strongly affect the large-scale dynamics and thermal state, constraining their statistical characteristics is of great importance for modeling the atmospheric circulation. We present a new data set of density perturbation amplitudes derived from accelerometer measurements during aerobraking of the European Space Agency’s Trace Gas Orbiter. The obtained data set presents features found by three previous orbiters: the lower thermosphere polar warming in the winter hemisphere, and the lack of links between gravity wave activity and topography. In addition, the orbits allowed for demonstrating a very weak diurnal variability in wave activity at high latitudes of the southern winter hemisphere for the first time. The estimated vertical damping rates of gravity waves agree well with theoretical predictions. No clear anticorrelation between perturbation amplitudes and the background temperature has been found. This indicates differences in dissipation mechanisms of gravity waves in the lower and upper thermosphere.
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3

Ford, E. A. K., A. L. Aruliah, E. M. Griffin, and I. McWhirter. "High time resolution measurements of the thermosphere from Fabry-Perot Interferometer measurements of atomic oxygen." Annales Geophysicae 25, no. 6 (June 29, 2007): 1269–78. http://dx.doi.org/10.5194/angeo-25-1269-2007.

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Abstract. Recent advances in the performance of CCD detectors have enabled a high time resolution study of the high latitude upper thermosphere with Fabry-Perot Interferometers (FPIs) to be performed. 10-s integration times were used during a campaign in April 2004 on an FPI located in northern Sweden in the auroral oval. The FPI is used to study the thermosphere by measuring the oxygen red line emission at 630.0 nm, which emits at an altitude of approximately 240 km. Previous time resolutions have been 4 min at best, due to the cycle of look directions normally observed. By using 10 s rather than 40 s integration times, and by limiting the number of full cycles in a night, high resolution measurements down to 15 s were achievable. This has allowed the maximum variability of the thermospheric winds and temperatures, and 630.0 nm emission intensities, at approximately 240 km, to be determined as a few minutes. This is a significantly greater variability than the often assumed value of 1 h or more. A Lomb-Scargle analysis of this data has shown evidence of gravity wave activity with waves with short periods. Gravity waves are an important feature of mesosphere-lower thermosphere (MLT) dynamics, observed using many techniques and providing an important mechanism for energy transfer between atmospheric regions. At high latitudes gravity waves may be generated in-situ by localised auroral activity. Short period waves were detected in all four clear nights when this experiment was performed, in 630.0 nm intensities and thermospheric winds and temperatures. Waves with many periodicities were observed, from periods of several hours, down to 14 min. These waves were seen in all parameters over several nights, implying that this variability is a typical property of the thermosphere.
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4

Becker, Erich. "Mean-Flow Effects of Thermal Tides in the Mesosphere and Lower Thermosphere." Journal of the Atmospheric Sciences 74, no. 6 (June 1, 2017): 2043–63. http://dx.doi.org/10.1175/jas-d-16-0194.1.

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Abstract This study addresses the heat budget of the mesosphere and lower thermosphere with regard to the energy deposition of upward-propagating waves. To this end, the energetics of gravity waves are recapitulated using an anelastic version of the primitive equations. This leads to an expression for the energy deposition of waves that is usually resolved in general circulation models. The energy deposition is shown to be mainly due to the frictional heating and, additionally, due to the negative buoyancy production of wave kinetic energy. The frictional heating includes contributions from horizontal and vertical momentum diffusion, as well as from ion drag. This formalism is applied to analyze results from a mechanistic middle-atmosphere general circulation model that includes energetically consistent parameterizations of diffusion, gravity waves, and ion drag. This paper estimates 1) the wave driving and energy deposition of thermal tides, 2) the model response to the excitation of thermal tides, and 3) the model response to the combined energy deposition by parameterized gravity waves and resolved waves. It is found that thermal tides give rise to a significant energy deposition in the lower thermosphere. The temperature response to thermal tides is positive. It maximizes at polar latitudes in the lower thermosphere as a result of poleward circulation branches that are driven by the predominantly westward Eliassen–Palm flux divergence of the tides. In addition, thermal tides give rise to a downward shift and reduction of the gravity wave drag in the upper mesosphere. Including the energy deposition in the model causes a substantial warming in the upper mesosphere and lower thermosphere.
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5

Broutman, Dave, Stephen D. Eckermann, and Douglas P. Drob. "The Partial Reflection of Tsunami-Generated Gravity Waves." Journal of the Atmospheric Sciences 71, no. 9 (August 28, 2014): 3416–26. http://dx.doi.org/10.1175/jas-d-13-0309.1.

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Abstract A vertical eigenfunction equation is solved to examine the partial reflection and partial transmission of tsunami-generated gravity waves propagating through a height-dependent background atmosphere from the ocean surface into the lower thermosphere. There are multiple turning points for each vertical eigenfunction (at least eight in one example), yet the wave transmission into the thermosphere is significant. Examples are given for gravity wave propagation through an idealized wind jet centered near the mesopause and through a realistic vertical profile of wind and temperature relevant to the tsunami generated by the Sumatra earthquake on 26 December 2004.
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6

Robinson, T. R. "Acoustic gravity wave growth and damping in convecting plasma." Annales Geophysicae 12, no. 2/3 (January 31, 1994): 210–19. http://dx.doi.org/10.1007/s00585-994-0210-5.

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Abstract. The propagation of acoustic gravity waves through steadily convecting plasma in the thermosphere has been analysed theoretically. The growth and damping rates of internal gravity waves due to the feedback effects of wave-modulated Joule heating and Laplace forcing have been calculated. It is found that large convection flow velocities lead to the growth of large-scale internal gravity waves, whilst small- and medium-scale waves are heavily damped, under similar conditions. It has also been shown that wave growth is favoured for waves travelling against the plasma flow direction. The effects of critical coupling when wave phase speeds match the plasma flow speed have also been investigated. The results of these calculations are discussed in the context of the atmospheric energy budget and thermosphere-ionosphere coupling.
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7

Li, Qinzeng, Jiyao Xu, Hanli Liu, Xiao Liu, and Wei Yuan. "How do gravity waves triggered by a typhoon propagate from the troposphere to the upper atmosphere?" Atmospheric Chemistry and Physics 22, no. 18 (September 19, 2022): 12077–91. http://dx.doi.org/10.5194/acp-22-12077-2022.

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Abstract. Gravity waves (GWs) strongly affect atmospheric dynamics and photochemistry and the coupling between the troposphere, stratosphere, mesosphere, and thermosphere. In addition, GWs generated by strong disturbances in the troposphere (e.g. thunderstorms and typhoons) can affect the atmosphere of Earth from the troposphere to the thermosphere. However, the fundamental process of GW propagation from the troposphere to the thermosphere is poorly understood because it is challenging to constrain this process using observations. Moreover, GWs tend to dissipate rapidly in the thermosphere because the molecular diffusion increases exponentially with height. In this study, a double-layer airglow network was used to capture concentric GWs (CGWs) over China that were excited by Typhoon Chaba (2016). We used ERA5 reanalysis data and Multi-functional Transport Satellite-1R observations to quantitatively describe the propagation processes of typhoon-generated CGWs from the troposphere, through the stratosphere and mesosphere, to the thermosphere. We found that the CGWs in the mesopause region were generated directly by the typhoon in the troposphere. However, the backward-ray-tracing analysis suggested that CGWs in the thermosphere originated from the secondary waves generated by the dissipation of the CGW and/or nonlinear processes in the mesopause region.
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8

Yasui, Ryosuke, Kaoru Sato, and Yasunobu Miyoshi. "The Momentum Budget in the Stratosphere, Mesosphere, and Lower Thermosphere. Part II: The In Situ Generation of Gravity Waves." Journal of the Atmospheric Sciences 75, no. 10 (October 2018): 3635–51. http://dx.doi.org/10.1175/jas-d-17-0337.1.

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The contributions of gravity waves to the momentum budget in the mesosphere and lower thermosphere (MLT) is examined using simulation data from the Ground-to-Topside Model of Atmosphere and Ionosphere for Aeronomy (GAIA) whole-atmosphere model. Regardless of the relatively coarse model resolution, gravity waves appear in the MLT region. The resolved gravity waves largely contribute to the MLT momentum budget. A pair of positive and negative Eliassen–Palm flux divergences of the resolved gravity waves are observed in the summer MLT region, suggesting that the resolved gravity waves are likely in situ generated in the MLT region. In the summer MLT region, the mean zonal winds have a strong vertical shear that is likely formed by parameterized gravity wave forcing. The Richardson number sometimes becomes less than a quarter in the strong-shear region, suggesting that the resolved gravity waves are generated by shear instability. In addition, shear instability occurs in the low (middle) latitudes of the summer (winter) MLT region and is associated with diurnal (semidiurnal) migrating tides. Resolved gravity waves are also radiated from these regions. In Part I of this paper, it was shown that Rossby waves in the MLT region are also radiated by the barotropic and/or baroclinic instability formed by parameterized gravity wave forcing. These results strongly suggest that the forcing by gravity waves originating from the lower atmosphere causes the barotropic/baroclinic and shear instabilities in the mesosphere that, respectively, generate Rossby and gravity waves and suggest that the in situ generation and dissipation of these waves play important roles in the momentum budget of the MLT region.
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9

Paulino, Igo, Joyrles F. Moraes, Gleuson L. Maranhão, Cristiano M. Wrasse, Ricardo Arlen Buriti, Amauri F. Medeiros, Ana Roberta Paulino, et al. "Intrinsic parameters of periodic waves observed in the OI6300 airglow layer over the Brazilian equatorial region." Annales Geophysicae 36, no. 1 (February 28, 2018): 265–73. http://dx.doi.org/10.5194/angeo-36-265-2018.

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Abstract. Periodic waves were observed in the OI6300 airglow images over São João do Cariri (36.5∘ W, 7.4∘ S) from 2012 to 2014 with simultaneous observations of the thermospheric wind using two Fabry–Pérot interferometers (FPIs). The FPIs measurements were carried out at São João do Cariri and Cajazeiras (38.5∘ W, 6.9∘ S). The observed spectral characteristics of these waves (period and wavelength) as well the propagation direction were estimated using two-dimensional Fourier analysis in the airglow images. The horizontal thermospheric wind was calculated from the Doppler shift of the OI6300 data extracted from interference fringes registered by the FPIs. Combining these two techniques, the intrinsic parameters of the periodic waves were estimated and analyzed. The spectral parameters of the periodic waves were quite similar to the previous observations at São João do Cariri. The intrinsic periods for most of the waves were shorter than the observed periods, as a consequence, the intrinsic phase speeds were faster compared to the observed phase speeds. As a consequence, these waves can easily propagate into the thermosphere–ionosphere since the fast gravity waves can skip turning and critical levels. The strength and direction of the wind vector in the thermosphere must be the main cause for the observed anisotropy in the propagation direction of the periodic waves, even if the sources of these waves are assumed to be isotropic. Keywords. Meteorology and atmospheric dynamics (waves and tides)
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10

Vargas, Fabio, Jorge L. Chau, Harikrishnan Charuvil Asokan, and Michael Gerding. "Mesospheric gravity wave activity estimated via airglow imagery, multistatic meteor radar, and SABER data taken during the SIMONe–2018 campaign." Atmospheric Chemistry and Physics 21, no. 17 (September 13, 2021): 13631–54. http://dx.doi.org/10.5194/acp-21-13631-2021.

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Abstract. We describe in this study the analysis of small and large horizontal-scale gravity waves from datasets composed of images from multiple mesospheric airglow emissions as well as multistatic specular meteor radar (MSMR) winds collected in early November 2018, during the SIMONe–2018 (Spread-spectrum Interferometric Multi-static meteor radar Observing Network) campaign. These ground-based measurements are supported by temperature and neutral density profiles from TIMED/SABER (Thermosphere, Ionosphere, Mesosphere Energetics and Dynamics/Sounding of the Atmosphere using Broadband Emission Radiometry) satellite in orbits near Kühlungsborn, northern Germany (54.1∘ N, 11.8∘ E). The scientific goals here include the characterization of gravity waves and their interaction with the mean flow in the mesosphere and lower thermosphere and their relationship to dynamical conditions in the lower and upper atmosphere. We have obtained intrinsic parameters of small- and large-scale gravity waves and characterized their impact in the mesosphere via momentum flux (FM) and momentum flux divergence (FD) estimations. We have verified that a small percentage of the detected wave events is responsible for most of FM measured during the campaign from oscillations seen in the airglow brightness and MSMR winds taken over 45 h during four nights of clear-sky observations. From the analysis of small-scale gravity waves (λh < 725 km) seen in airglow images, we have found FM ranging from 0.04–24.74 m2 s−2 (1.62 ± 2.70 m2 s−2 on average). However, small-scale waves with FM > 3 m2 s−2 (11 % of the events) transport 50 % of the total measured FM. Likewise, wave events of FM > 10 m2 s−2 (2 % of the events) transport 20 % of the total. The examination of large-scale waves (λh > 725 km) seen simultaneously in airglow keograms and MSMR winds revealed amplitudes > 35 %, which translates into FM = 21.2–29.6 m2 s−2. In terms of gravity-wave–mean-flow interactions, these large FM waves could cause decelerations of FD = 22–41 m s−1 d−1 (small-scale waves) and FD = 38–43 m s−1 d−1 (large-scale waves) if breaking or dissipating within short distances in the mesosphere and lower thermosphere region.
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Дисертації з теми "Atmospheric waves; Gravity waves; Thermosphere"

1

De, Deuge Maria. "Optical observations of gravity waves in the high-latitude thermosphere /." Title page, abstract and contents only, 1990. http://web4.library.adelaide.edu.au/theses/09SM/09smd485.pdf.

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2

Negale, Michael. "Investigating the Climatology of Mesospheric and Thermospheric Gravity Waves at High Northern Latitudes." DigitalCommons@USU, 2018. https://digitalcommons.usu.edu/etd/6937.

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An important property of the Earth's atmosphere is its ability to support wave motions, and indeed, waves exist throughout the Earth's atmosphere at all times and all locations. What is the importance of these waves? Imagine standing on the beach as water waves come crashing into you. In this case, the waves transport energy and momentum to you, knocking you off balance. Similarly, waves in the atmosphere crash, known as breaking, but what do they crash into? They crash into the atmosphere knocking the atmosphere off balance in terms of the winds and temperatures. Although the Earth's atmosphere is full of waves, they cannot be observed directly; however, their effects on the atmosphere can be observed. Waves can be detected in the winds and temperatures, as mentioned above, but also in pressure and density. In this dissertation, three different studies of waves, known as gravity waves, were performed at three different locations. For these studies, we investigate the size of the waves and in which direction they move. Using specialized cameras, gravity waves were observed in the middle atmosphere (50-70 miles up) over Alaska (for three winter times) and Norway (for one winter time). A third study investigated gravity waves at a much higher altitude (70 miles on up) using radar data from Alaska (for three years). These studies have provided important new information on these waves and how they move through the atmosphere. This in turn helps to understand in which direction these waves are crashing into the atmosphere and therefore, which direction the energy and momentum are going. Studies such as these help to better forecast weather and climate.
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3

Beldon, Charlotte. "VHF radar studies of mesosphere and thermosphere." Thesis, University of Bath, 2008. https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.512294.

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4

Halliday, Oliver John. "Atmospheric convection and gravity waves." Thesis, University of Leeds, 2018. http://etheses.whiterose.ac.uk/22414/.

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5

Eckermann, Stephen D. "Atmospheric gravity waves : obsevations and theory /." Title page, table of contents and abstract only, 1990. http://web4.library.adelaide.edu.au/theses/09PH/09phe1862.pdf.

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Thesis (Ph. D.)--University of Adelaide, Dept. of Physics and Mathematical Physics, 1990.
Copies of author's previously published articles inserted. Includes bibliographical references (leaves 261-288).
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6

Gibson-Wilde, Dorothy E. "Atmospheric gravity waves in constituent distributions /." Title page, abstract and contents only, 1996. http://web4.library.adelaide.edu.au/theses/09PH/09phg4516.pdf.

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7

Yan, Xiuping. "Satellite observations of atmospheric gravity waves." Thesis, University of Leicester, 2010. http://hdl.handle.net/2381/7979.

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A new methodology of gravity wave observations has been developed for the HIgh Resolution Dynamics Limb Sounder (HIRDLS). Individual vertical profiles of gravity-wave temperature perturbations that were determined by subtraction of a dynamic 31 day background field and a 1000 km along-track temperature filter were Fourier transformed to estimate the gravity-wave temperature amplitudes and vertical wavelengths (~2 – 16 km) in the stratosphere. Gravity wave activity is highly variable with season and can be highly orographically dependent, especially in the winter extratropics. Investigations of episodes of enhanced gravity waves over the southern Andes, the Cascade Range and the Rockies in the winter months of 2006 indicate that orographic gravity waves propagate downwind from the mountains. By way of contrast, observations of gravity waves around the Himalayas show a strong relationship with the cyclones in that region. HIRDLS observations over the southern Andes during July-September 2006 were compared to the orographic gravity-wave parameterization scheme in the UK Met Office Unified Model®. The results indicate that the observed waves are likely to be orographically excited. The observed wave activity extends large distances (a few thousand kilometres) downwind of the mountains and over the ocean. This downstream wave activity is not represented by the parameterization scheme similar to many schemes, which assume that the waves propagate vertically above the mountains only. Gravity waves over the tropics and tropical South America were compared with the AVHRR Outgoing Longwave Radiation (OLR), TRMM convective rainfall and ECMWF winds for convective sources. The comparisons show that the peak gravity wave temperature amplitudes correspond closely to the OLR ≤ 200 W/m ², in good agreement with the mesoscale cyclones and are above the updrifts, which indicate deep convective generation of the gravity waves. These waves show vertical propagation with higher-frequency and ~ 7.5 km vertical wavelengths in the lower stratosphere.
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8

Watkins, Christopher Lloyd. "Atmospheric gravity waves on giant planets." Thesis, Queen Mary, University of London, 2012. http://qmro.qmul.ac.uk/xmlui/handle/123456789/8683.

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Internal gravity waves are a common feature of stratified fluids. They facilitate transport of momentum and energy – thus influencing the evolution of the fluid. There is a large body of research addressing the behaviour of gravity waves in the terrestrial atmosphere. This thesis builds and extends the research to giant planets – in particular to close-in extrasolar giant planets and the solar system giant planet, Jupiter. Because the atmospheres of close-in giant planets are expected to be strongly stratified, knowledge of the behaviour of gravity waves in such atmospheres is especially important. Close-in giant planets are thought to have their rotations and orbital period 1:1 synchronised, i.e., they are “tidally locked”. Such planets do not exist in the Solar System. However, many are known from observations of extrasolar systems. Their synchronisation means that they have a permanent day-side and night-side leading to interesting atmospheric dynamics. Modelling these circulations with global circulation models (GCMs) and comparing these models with observations is an active research area. However, many GCMs filter some or all gravity waves removing their effects. This thesis addresses this by explicitly looking at the effects gravity waves can have on the circulation. It is shown that gravity waves provide a mechanism for accelerating, decelerating, and heating the flow. Further, horizontally propagating gravity waves are shown to provide a possible means for coupling the day- and night-sides of tidally locked planets. As well as affecting the dynamics of the atmosphere, gravity wave behaviour is affected by the dynamics of the atmosphere. Therefore, gravity waves can be used to explore atmospheric properties. In this thesis gravity waves observed in Jupiter’s atmosphere, by the Galileo probe, are used to identify features of Jupiter’s atmosphere such as the altitude of the turbopause and the vertical profile of zonal winds at the probe entry site.
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9

Powell, Jonathan. "Stochastic modelling of atmospheric gravity waves." Thesis, University of Edinburgh, 2004. http://hdl.handle.net/1842/15652.

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Internal gravity waves have an important effect on the large-scale circulation of the middle atmosphere, which is conditioned by the deposition of momentum due to their breaking. The propagation of gravity waves is influenced by the properties of the background wind. This thesis examines this influence: it uses stochastic techniques to study gravity wave propagation through a randomly fluctuating background wind. It begins by describing general features of the atmosphere and gravity wave propagation. The basic equations of fluid flow within the atmosphere are derived. These lead via the WKB approximation to a dispersion relation and to ray equations for gravity wave propagation. Propagation equations, such as the ray equations and dispersion relation, are derived in a general context. The notion of a Wigner matrix is introduced, and this is used to derive transport equations for a general Hamiltonian system that may contain random components. These results generalise earlier works by Ryzhik and Guo and Wang. Atmospheric gravity waves are described as an application and the equations derived via the WKB approximation are recovered. The major factor influencing the distribution of gravity waves is the spread of their wavenumber as they propagate through a wind. This is described by the Doppler spreading model. A one-dimensional system with a randomly fluctuating background wind, dependent on altitude only, is considered. The model revisits that of Souprayen by using an Ornstein-Uhlenbeck process to describe the wind. Simple equations for the energy spectrum induced by gravity waves are derived. Analytic forms of the energy spectrum are given and features of the spectrum such as the m-3 spectral tail (where m is the vertical wavenumber), central wavenumber and scaling with the Brunt-Väisälä frequently are found to be consistent with observations. An equation for the force on the background, induced by gravity wave breaking is also derived.
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10

Jacobi, Christoph, Friederike Liilienthal, T. Schmidt, and la Torre A. de. "Modeling the Southern Hemisphere winter circulation using realistic zonal mean gravity wave information in the lower atmosphere." Universität Leipzig, 2016. https://ul.qucosa.de/id/qucosa%3A16703.

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A mechanistic global circulation model is used to simulate the mesospheric and lower thermospheric circulation during austral winter. The model includes a gravity wave (GW) parameterization that is initiated by prescribed GW parameters in the troposphere. In standard configuration, these waves are described by a simple distribution with large amplitudes in the winter hemisphere and small ones in summer. Here we replace this distribution by a more realistic one, which is based on observations of potential GW energy using GPS radio occultations, but which is normalized to the same global mean amplitude. The model experiment shows that this new gravity wave distribution leads to weaker zonal winds in the mesosphere, a downward shift of the meridional poleward mesospheric wind jet, enhanced downwelling in the mid-to-high-latitude winter mesosphere and warming of the polar stratopause.
Ein globales mechanistisches Zirkulationsmodell wird verwendet um die Dynamik der Mesosphäre und unteren Thermosphäre im Südwinter zu simulieren. Das Modell beinhaltet eine Schwerewellenparametrisierung die durch eine vorgeschriebene Schwerewellenverteilung in der oberen Troposphäre angetrieben wird. In der Standardkonfiguration besteht diese aus einer einfachen zonal gemittelten Verteilung mit größeren Amplituden im Winter als im Sommer. Wir ersetzen diese Verteilung durch eine realistischere, die auf der beobachteten globalen Verteilung der potentiellen Energie von Schwerewellen basiert und auf die gleiche global gemittelte Amplitude normiert wird. Das Modellexperiment zeigt, dass die neue Schwerewellenverteilung zu schwächeren zonalen Winden in der Mesosphäre, einer Verschiebung des meridionalen Jets nach unten, verstärkten Abwinden in der Mesosphäre mittlerer und höherer Breiten im Winter, und einer Erwärmung der polaren Winterstratopause führt.
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Книги з теми "Atmospheric waves; Gravity waves; Thermosphere"

1

Smith, R. E. The Marshall Engineering Thermosphere (MET) model. [Marshall Space Flight Center, Ala.]: National Aeronautics and Space Administration, Marshall Space Flight Center, 1998.

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2

An introduction to atmospheric gravity waves. 2nd ed. Waltham, MA: Elsevier, 2012.

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3

Dewan, Edmond M. Direct experimental evidence for an atmospheric gravity wave cascade. Hanscom Air Force Base, MA: Air Force Research Laboratory, Space Vehicles Directorate, Air Force Materiel Command, 1999.

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4

Evers, Läslo Gerardus. The inaudible symphony: On the detection and source identification of atmospheric infrasound. Delft: Delf Univerity of Technology, 2008.

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5

Evers, Läslo Gerardus. The inaudible symphony: On the detection and source identification of atmospheric infrasound. Delft: Delf Univerity of Technology, 2008.

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6

John, Stanford. Rossby-gravity waves in tropical total ozone data. [Washington, DC: National Aeronautics and Space Administration, 1993.

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7

John, Stanford. Rossby-gravity waves in tropical total ozone data. [Washington, DC: National Aeronautics and Space Administration, 1993.

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8

Fakhrutdinova, A. N. Volnovai︠a︡ struktura t︠s︡irkuli︠a︡t︠s︡ii nizhneĭ i sredneĭ atmosfery Zemli. Kazanʹ: Kazanskiĭ gos. universitet, 2006.

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9

Kelder, H. On waves in the upper atmosphere. De Bilt: Koninklijk Nederlands Meteorologisch Instituut, 1986.

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10

Fairall, C. W. A model of gravity-wave-induced variability and turbulence in the stratified free atmosphere. Boulder, Colo: U.S. Dept. of Commerce, National Oceanic and Atmospheric Administration, Environmental Research Laboratories, Wave Propagation Laboratory, 1990.

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Частини книг з теми "Atmospheric waves; Gravity waves; Thermosphere"

1

Oyama, S., and B. J. Watkins. "Generation of Atmospheric Gravity Waves in the Polar Thermosphere in Response to Auroral Activity." In Dynamic Coupling Between Earth’s Atmospheric and Plasma Environments, 463–73. New York, NY: Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4614-5677-3_16.

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2

Gardner, L. C., and R. W. Schunk. "Traveling Atmospheric Disturbance and Gravity Wave Coupling in the Thermosphere." In Modeling the Ionosphere-Thermosphere System, 101–6. Chichester, UK: John Wiley & Sons, Ltd, 2014. http://dx.doi.org/10.1002/9781118704417.ch9.

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3

Mikumo, Takeshi, and Shingo Watada. "Acoustic-Gravity Waves from Earthquake Sources." In Infrasound Monitoring for Atmospheric Studies, 263–79. Dordrecht: Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9508-5_9.

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4

Mayr, H. G., I. Harris, and W. D. Pesnell. "Properties of Thermospheric Gravity Waves on Earth, Venus and Mars." In Venus and Mars: Atmospheres, Ionospheres, and Solar Wind Interactions, 91–111. Washington, D. C.: American Geophysical Union, 2013. http://dx.doi.org/10.1029/gm066p0091.

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5

Achatz, Ulrich. "Gravity Waves and Their Impact on the Atmospheric Flow." In Atmospheric Dynamics, 407–505. Berlin, Heidelberg: Springer Berlin Heidelberg, 2022. http://dx.doi.org/10.1007/978-3-662-63941-2_10.

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6

Fritts, David C., and Thomas S. Lund. "Gravity Wave Influences in the Thermosphere and Ionosphere: Observations and Recent Modeling." In Aeronomy of the Earth's Atmosphere and Ionosphere, 109–30. Dordrecht: Springer Netherlands, 2011. http://dx.doi.org/10.1007/978-94-007-0326-1_8.

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7

Remmler, Sebastian, Stefan Hickel, Mark D. Fruman, and Ulrich Achatz. "Direct Numerical Simulation of Breaking Atmospheric Gravity Waves." In High Performance Computing in Science and Engineering ‘14, 593–607. Cham: Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-10810-0_39.

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8

ReVelle, D. O. "Acoustic-Gravity Waves from Impulsive Sources in the Atmosphere." In Infrasound Monitoring for Atmospheric Studies, 305–59. Dordrecht: Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9508-5_11.

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9

Fritts, David C. "Gravity Wave-Tidal Interactions in the Middle Atmosphere: Observations and Theory." In The Upper Mesosphere and Lower Thermosphere: A Review of Experiment and Theory, 121–31. Washington, D. C.: American Geophysical Union, 2013. http://dx.doi.org/10.1029/gm087p0121.

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10

Hara, Tetsu, Jeffrey E. Hare, James B. Edson, and James M. Wilczak. "Effect of Surface Gravity Waves on Near-Surface Atmospheric Turbulence." In Atmospheric and Oceanographic Sciences Library, 127–52. Dordrecht: Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-015-9291-8_5.

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Тези доповідей конференцій з теми "Atmospheric waves; Gravity waves; Thermosphere"

1

Wurtele, M. G., A. Datta, and D. M. Landau. "CAT - Generating Breakdown of Atmospheric Gravity Waves." In World Aviation Congress & Exposition. 400 Commonwealth Drive, Warrendale, PA, United States: SAE International, 1997. http://dx.doi.org/10.4271/975578.

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2

Kaufmann, Martin, and Rui Song. "Atmospheric gravity waves observation from a lunar base." In IGARSS 2016 - 2016 IEEE International Geoscience and Remote Sensing Symposium. IEEE, 2016. http://dx.doi.org/10.1109/igarss.2016.7729962.

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3

Li, Xiaofeng. "SAR imaging of oceanic and atmospheric gravity waves." In 2017 Progress in Electromagnetics Research Symposium - Fall (PIERS - FALL). IEEE, 2017. http://dx.doi.org/10.1109/piers-fall.2017.8293485.

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4

Cherniakov, Sergei M., Valentin C. Roldugin, and Alexey V. Roldugin. "Airglow intensity variations affected by acoustic-gravity waves at high latitudes." In XXII International Symposium Atmospheric and Ocean Optics. Atmospheric Physics, edited by Gennadii G. Matvienko and Oleg A. Romanovskii. SPIE, 2016. http://dx.doi.org/10.1117/12.2242778.

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5

Nikolashkin, Semen V., Anastasiia M. Ammosova, and Igor I. Koltovskoi. "Properties of internal gravity waves observed on noctilucent clouds on high latitudes." In XXV International Symposium, Atmospheric and Ocean Optics, Atmospheric Physics, edited by Gennadii G. Matvienko and Oleg A. Romanovskii. SPIE, 2019. http://dx.doi.org/10.1117/12.2540836.

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6

Mayor, Shane D. "Observations of microscale internal gravity waves over an orchard canopy." In Propagation Through and Characterization of Atmospheric and Oceanic Phenomena. Washington, D.C.: OSA, 2017. http://dx.doi.org/10.1364/pcaop.2017.pw1d.3.

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7

Gavrilov, Nikolai M., Sergey P. Kshevetskii, and Rada O. Manuilova. "Effects of nonlinear interactions of spectral components of acoustic-gravity waves in the atmosphere." In 26th International Symposium on Atmospheric and Ocean Optics, Atmospheric Physics, edited by Gennadii G. Matvienko and Oleg A. Romanovskii. SPIE, 2020. http://dx.doi.org/10.1117/12.2574794.

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8

Huang, Weigen, Xilin Gan, Jingsong Yang, Bin Fu, and Peng Chen. "SAR observations of atmospheric gravity waves over the East China Sea." In SPIE Europe Remote Sensing, edited by Lorenzo Bruzzone, Claudia Notarnicola, and Francesco Posa. SPIE, 2009. http://dx.doi.org/10.1117/12.829876.

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9

Jumper, George, Edmund Murphy, Anthony Ratkowski, and Jean Vernin. "Multi-Sensor Campaign to Correlate Atmospheric Optical Turbulence to Gravity Waves." In 42nd AIAA Aerospace Sciences Meeting and Exhibit. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2004. http://dx.doi.org/10.2514/6.2004-1077.

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10

Smalikho, I. N., V. A. Banakh, and A. V. Falits. "Doppler lidar observation of the gravity waves near Lake Baikal in the summer of 2015." In XXII International Symposium Atmospheric and Ocean Optics. Atmospheric Physics, edited by Gennadii G. Matvienko and Oleg A. Romanovskii. SPIE, 2016. http://dx.doi.org/10.1117/12.2248617.

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Звіти організацій з теми "Atmospheric waves; Gravity waves; Thermosphere"

1

Fritts, David C. Nonlinear Spectral Evolution of Atmospheric Gravity Waves. Fort Belvoir, VA: Defense Technical Information Center, November 2000. http://dx.doi.org/10.21236/ada387509.

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2

Hara, Tetsu. Interaction Between Surface Gravity Waves and Near Surface Atmospheric Turbulence. Fort Belvoir, VA: Defense Technical Information Center, September 1997. http://dx.doi.org/10.21236/ada634931.

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3

Hara, Tetsu. Statistical Characteristics of Small Scale Wind-waves and Their Modulation by Longer Gravity Waves and Atmospheric Forcing. Fort Belvoir, VA: Defense Technical Information Center, September 1997. http://dx.doi.org/10.21236/ada627814.

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4

Chunchuzov, I., P. W. Vachon, and X. Li. Analysis and Modelling of Atmospheric Gravity Waves Observed in RADARSAT SAR Images. Natural Resources Canada/ESS/Scientific and Technical Publishing Services, 2000. http://dx.doi.org/10.4095/219569.

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