Готові списки джерел за темами / Gravity waves

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Добірка наукової літератури з теми "Gravity waves"

Автор: Grafiati
Опубліковано: 4 червня 2021
Оновлено: 9 червня 2025

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Статті в журналах з теми "Gravity waves"

1

Naciri, Mamoun, and Chiang C. Mei. "Evolution of short gravity waves on long gravity waves." Physics of Fluids A: Fluid Dynamics 5, no. 8 (August 1993): 1869–78. http://dx.doi.org/10.1063/1.858812.

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2

Dias, Frédéric, and Christian Kharif. "NONLINEAR GRAVITY AND CAPILLARY-GRAVITY WAVES." Annual Review of Fluid Mechanics 31, no. 1 (January 1999): 301–46. http://dx.doi.org/10.1146/annurev.fluid.31.1.301.

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3

Akers, Benjamin F., David M. Ambrose, and J. Douglas Wright. "Gravity perturbed Crapper waves." Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences 470, no. 2161 (January 8, 2014): 20130526. http://dx.doi.org/10.1098/rspa.2013.0526.

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Crapper waves are a family of exact periodic travelling wave solutions of the free-surface irrotational incompressible Euler equations; these are pure capillary waves, meaning that surface tension is accounted for, but gravity is neglected. For certain parameter values, Crapper waves are known to have multi-valued height. Using the implicit function theorem, we prove that any of the Crapper waves can be perturbed by the effect of gravity, yielding the existence of gravity–capillary waves nearby to the Crapper waves. This result implies the existence of travelling gravity–capillary waves with multi-valued height. The solutions we prove to exist include waves with both positive and negative values of the gravity coefficient. We also compute these gravity perturbed Crapper waves by means of a quasi-Newton iterative scheme (again, using both positive and negative values of the gravity coefficient). A phase diagram is generated, which depicts the existence of single-valued and multi-valued travelling waves in the gravity–amplitude plane. A new largest water wave is computed, which is composed of a string of bubbles at the interface.
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4

Gnevyshev, Vladimir, and Sergei Badulin. "Wave Patterns of Gravity–Capillary Waves from Moving Localized Sources." Fluids 5, no. 4 (November 24, 2020): 219. http://dx.doi.org/10.3390/fluids5040219.

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We study wave patterns of gravity–capillary waves from moving localized sources within the classic setup of the problem of ship wakes. The focus is on the co-existence of two wave systems with opposite signatures of group velocity relative to the localized source. It leads to the problem of choice of signs for phase functions of the gravity (“slow”) and capillary (“fast”) branches of the dispersion relation: the question generally ignored when constructing phase patterns of the solutions. We detail characteristic angles of the wake patterns: (i) angle of demarcation of gravity and capillary waves—“the phase Mach” cone, (ii) angle of the minimal group velocity of gravity–capillary waves—“the group Mach” cone, (iii, iv) angles of cusps of isophases that appear after a threshold current speed. The outer cusp cone is naturally associated with the classic cone of Kelvin for pure gravity waves. The inner one results from the effect of capillarity and tends to the “group Mach” pattern at high speeds of current. Amplitudes of the wave patterns are estimated within the recently proposed approach of reference functions for the problem of propagation of packets of linear dispersive waves. The effect of shape is discussed for elliptic reference sources.
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5

Naeser, Harald. "The Capillary Waves’ Contribution to Wind-Wave Generation." Fluids 7, no. 2 (February 10, 2022): 73. http://dx.doi.org/10.3390/fluids7020073.

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Published theories and observations have shown that dissipation of gravity waves implies frequency downshifting of wave energy. Hence, for wind-waves, the wind energy input to the highest frequencies is of special interest. Here it is shown that this input is vital, because the direct wind energy input obtained by the air-pressure’s work on most gravity waves is slightly less than what the waves need to grow. Further, the wind’s input of the angular momentum that waves need to grow is found to be absent at most gravity wave frequencies. The capillary waves that appear at the surface of the sea when the wind is blowing solve these problems. To demonstrate this, an extension of linear wave theory is established to study possibilities and limitations for transfer of energy and angular momentum from the wind to waves through these frequencies. The theory describes regular, gravity–capillary waves with constant amplitude under laminar conditions. It includes surface tensions, viscosity, gravity and a wind-generated shear current, and shows that these waves—contrary to most gravity waves—receive more energy from the wind than they dissipate and angular momentum they cannot keep. Hence, the problem of the missing input of energy and angular momentum from wind to gravity waves is solved by transfers through the capillary waves. This implies that capillary waves are vital to obtain growing gravity waves.
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6

Wang, Xiujuan, Lingkun Ran, Yanbin Qi, Zhongbao Jiang, Tian Yun, and Baofeng Jiao. "Analysis of Gravity Wave Characteristics during a Hailstone Event in the Cold Vortex of Northeast China." Atmosphere 14, no. 2 (February 20, 2023): 412. http://dx.doi.org/10.3390/atmos14020412.

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Based on high-resolution pressure data collected by a microbarograph and Fourier transform (FFT) data processing, a detailed analysis of the frequency spectra characteristics of gravity waves during a hailstone event in the cold vortex of Northeast China (NECV) on 9 September 2021 is presented. The results show that the deep NECV served as the large-scale circulation background for the hailstone event. The development of hailstones was closely related to gravity waves. In different hail stages, the frequency spectra characteristics of gravity waves were obviously different. One and a half hours before hailfall, there were gravity wave precursors with periods of 50–180 min and corresponding amplitudes ranging from 30 to 60 Pa. During hailfall, the center amplitudes of the gravity waves were approximately 50 Pa and 60 Pa, with the corresponding period ranges expanding to 60–70 min and 160–240 min. Simultaneously, hailstones initiated shorter periods (26–34 min) of gravity waves, with the amplitudes increasing to approximately 12–18 Pa. The relationship between hailstones and gravity waves was positive. After hailfall, gravity waves weakened and dissipated rapidly. As shown by the reconstructed gravity waves, key periods of gravity wave precursors ranged from 50–180 min, which preceded hailstones by several hours. When convection developed, there was thunderstorm high pressure and an outflow boundary. The airflow converged and diverged downstream, resulting in the formation of gravity waves and finally triggering hailfall. Gravity wave predecessors are significant for hail warnings and artificial hail suppression.
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7

Kenyon, Kern E. "Frictionless Surface Gravity Waves." Natural Science 12, no. 04 (2020): 199–201. http://dx.doi.org/10.4236/ns.2020.124017.

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8

SUN, TIEN-YU, and KAI-HUI CHEN. "ON INTERNAL GRAVITY WAVES." Tamkang Journal of Mathematics 29, no. 4 (December 1, 1998): 249–69. http://dx.doi.org/10.5556/j.tkjm.29.1998.4254.

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 We are concerned with the steady wave motions in a 2-fluid system with constant densities. This is a free boundary problem in which the lighter fluid is bounded above by a free surface and is separated from the heavier one down below by an interface. By using a contractive mapping principle type argument. a constructive proof to the existence of some of these exact periodic internal gravity waves is proveded. 
 
 
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9

Vikulin, A. V., A. A. Dolgaya, and S. A. Vikulina. "Geodynamic waves and gravity." Geodynamics & Tectonophysics 5, no. 1 (2014): 291–303. http://dx.doi.org/10.5800/gt-2014-5-1-0128.

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Longuet-Higgins, M. S. "Bifurcation in gravity waves." Journal of Fluid Mechanics 151, no. -1 (February 1985): 457. http://dx.doi.org/10.1017/s0022112085001057.

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Дисертації з теми "Gravity waves"

1

Popat, Nilesh R. "Steep capillary waves on gravity waves." Thesis, University of Bristol, 1989. http://hdl.handle.net/1983/78695ee9-b923-4374-b70c-6589b4215241.

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The frequent presence of ripples on the free surface of water. on both thin film flows and ponds or lakes motivates this theoretical investigation into the propagation of ripples on gravity waves. These ripples are treated as "slowly-varying" waves in a reference frame where the gravity wave flow is steady. The methods used are those of the averaged Lagrangian (Whitham 1965,1967,1974) and the averaged equations of motion (Phillips 1966) which are shown to be equivalent. The capillary wave modulation is taken to be steady in the reference frame which brings the gravity wave, or gravity driven flow, to rest. Firstly the motion over ponds or lakes is considered. Linear capillary-gravity waves are examined in order to set the scene. Crapper's (1957) exact finite-amplitude waves are examined next to show the actual behaviour of the flow field. The underlying gravity driven flow is that of pure gravity waves over an' "infinite" depth liquid. These gravity waves are modelled with "numerically exact" solutions for periodic plane-waves. The initial studies are inviscid and show that steep gravity waves either "absorb" or "sweep-up" a range of capillary waves or, alternatively, cause them to break in the vicinity of gravity wave crests. Improvements on the theory are made by including viscous dissipation of wave energy. This leads to a number of solutions approaching "stopping velocities" or the "stopped waves solution". In addition to these effects "higher-order dispersion" is introduced for weakly nonlinear waves near linear caustics. This clarifies aspects of the dissipation results and shows that wave reflection sometimes occurs. Secondly, waves on thin film flows are considered. Linear capillary-gravity waves are again examined in order to set the scene. Kinnersley's (1957) exact finite-amplitude waves are examined next to show the actual behaviour of the flow field. The underlying gravity driven flow is given by shallow water gravity waves. No modelling of these is necessary simply because they are included within Whitham's or Phillips' equations ab initio. This study is inviscid and shows the unexpected presence of critical velocities at which pairs of solution branches originate. iii
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2

Leaman, Nye Abigail. "Scattering of internal gravity waves." Thesis, University of Cambridge, 2011. https://www.repository.cam.ac.uk/handle/1810/238679.

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Internal gravity waves play a fundamental role in the dynamics of stably stratified regions of the atmosphere and ocean. In addition to the radiation of momentum and energy remote from generation sites, internal waves drive vertical transport of heat and mass through the ocean by wave breaking and the mixing subsequently produced. Identifying regions where internal gravity waves contribute to ocean mixing and quantifying this mixing are therefore important for accurate climate and weather predictions. Field studies report significantly enhanced measurements of turbulence near 'rough' ocean topography compared with those recorded in the ocean interior or near more gradually varying topography (e.g. Toole et al. 1997, J. Geophys. Res. 102). Such observations suggest that interaction of waves with rough topography may act to skew wave energy spectra to high wavenumbers and hence promote wave breaking and fluid mixing. This thesis examines the high wavenumber scatter and spatial partitioning of wave energy at 'rough' topography containing features that are of similar scales to those characterising incident waves. The research presented here includes laboratory experiments using synthetic schlieren and PIV to visualise two-dimensional wavefields produced by small amplitude oscillations of cylinders within linear salt-water stratifications. Interactions of wavefields with planar slopes and smoothly varying sinusoidal topography are compared with those with square-wave, sawtooth and pseudo knife-edge profiles, which have discontinuous slopes. Far-field structures of scattered wavefields are compared with linear analytical models. Scatter to high wavenumbers is found to be controlled predominantly by the relative slopes and characterising length scales of the incident wavefield and topography, as well as the shape and aspect ratio of the topographic profile. Wave energy becomes highly focused and the spectra skewed to higher wavenumbers by 'critical' regions, where the topographic slope is comparable with the slope of the incident wave energy vector, and at sharp corners, where topographic slope is not defined. Contrary to linear geometric ray tracing predictions (Longuet-Higgins 1969, J. Fluid Mech. 37), a significant back-scattered field can be achieved in near-critical conditions as well as a forward scattered wavefield in supercritical conditions, where the slope of the boundary is steeper than that of the incident wave. Results suggest that interaction with rough benthic topography could efficiently convert wave energy to higher wavenumbers and promote fluid mixing in such ocean regions.
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3

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

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Doherty, Mary Jane. "Focal lengths and gravity waves." Thesis, Massachusetts Institute of Technology, 1985. http://hdl.handle.net/1721.1/73280.

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Thesis (M.S.V.S.)--Massachusetts Institute of Technology, Dept. of Architecture, 1985.<br>MICROFICHE COPY AVAILABLE IN ARCHIVES AND ROTCH.<br>Transferred to 1/2 in VHS videotape from 8 mm film.<br>Includes bibliographical references (leaves 56-57).<br>Film is composed of tiny photographs which, when projected, sometimes look very much like people and things in the real world. Film, too, cannot be separated from its tools. Aesthetic criticism was, and still is, weighted towards consideration of the life-like tiny photographs. This thesis traces the evolution of film technology in order to establish the point where non- fiction ideology (aesthetics) lost pace with technical innovation - a derailment, so to speak, with nefarious implications for the present-day filmmaker. The emphasis is on lenses - the provocative "camera eye" - and sound recording equipment - which proved to be the rate-limiter of technical advance. This thesis considers two filmmaking solutions to the present malaise; the Standard TV Documentary, and the single-person shooting methodology of former MIT filmmakers, Jeff Kreines and Joel DeMott - both of which, in turn , will be compared to my own response - in the form of a movie, Gravity, which is about the members of an MIT experimental astrophysics laboratory trying to discover gravity waves. A videotape copy of the movie. is included with the thesis paper.<br>by Mary Jane Doherty.<br>M.S.V.S.
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Mantke, Wolfgang. "Spin and gravity." Thesis, Georgia Institute of Technology, 1989. http://hdl.handle.net/1853/27605.

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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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Meza, Valle Claudio Alejandro. "Early detection of extreme waves by acoustic gravity-waves." Tesis, Universidad de Chile, 2019. http://repositorio.uchile.cl/handle/2250/171084.

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Tesis para optar al grado de Magíster en Ciencias de la Ingeniería, Mención Matemáticas Aplicadas<br>Extreme waves generated in the ocean are of high importance because various maritime structures in the world, including ships, are confronted to this type of wave events, both in deep waters and in coastal areas. Some extreme waves correspond to wave phenomena generated in an atypical way in the ocean, also called monster waves, freak waves, rogue waves, extreme waves, solitons etc., since their generation differs from the common waves generated by wind. Assuming a slightly compressible ocean, the generation and analysis of acoustic-gravity waves (AGW or acoustic waves) in the ocean have been the subject of study for some time, because from them it is possible to obtain some information from the gravity wave, in this case a extreme wave that have generated them, and also to know other kind of phenomena induced by these AGW, as is the case of the bottom pressure. In the present work, a mathematical model has been developed which represents the generation and propagation of an extreme wave represented by a pressure change in the surface of the ocean considering compressible fluid, from which the generation and propagation of acoustic waves is induced. Since sound travels at a speed of 1500 m/s in the ocean, these waves arrive first at any observation point, allowing early detection of the extreme wave from the pressure in the oceanic bottom due to propagation of the acoustic wave. The theoretical development and two-dimensional numerical simulations are presented in the document. The implementation of this methodology and its results is relevant in the field of civil and maritime engineering in Chile since its high potential in coastal zones, due to the fact that for some years, the frequency of extreme wave events has been seen increased, and having an alternative detection system for extreme wave events can become a relevant factor in coastal management and natural disasters services. It is important to mention that this type of work has not been developed previously in Chile.<br>proyectos Centros de Excelencia Basal Conicyt PIA AFB 170001 CMM & UMI-CNRS 2807 y Fondecyt Regular 1171854
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8

Horne, Iribarne Ernesto. "Transport properties of internal gravity waves." Thesis, Lyon, École normale supérieure, 2015. http://www.theses.fr/2015ENSL1027/document.

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Les ondes internes sont produites par suite de l’équilibre dynamique entre les forces de flottabilité et la gravité quand une particule de fluide est déplacée verticalement dans un milieu stratifié stable. Les systèmes géophysiques tels que océan et l’atmosphère sont naturellement stratifiés et donc favorables à la propagation des ondes internes. En outre, ces deux environnements stockent une grande quantité de particules tant dans leur intérieur que sur les bords. Par conséquent, les ondes internes et les particules vont inévitablement interagir dans ces systèmes. Au cours de ce travail, des expériences exploratoires sont réalisées pour étudier le transport par érosion des particules, généré par les ondes internes. Afin de déterminer un seuil de transport, les propriétés particulières des réflexions d’ondes internes («réflexion critique ») sont utilisées pour augmenter l’intensité du champ d’ondes à la surface de réflexion. Une méthode a été développée en collaboration avec une équipe de traitement du signal pour améliorer la détermination des composantes de l’onde impliquées dans une réflexion quasi critique. Cela nous a permis de comparer nos résultats expérimentaux avec une théorie de la réflexion critique, montrant un bon accord et permettant d’extrapoler ces résultats à des expériences au-delà de la nôtre et à des conditions océaniques. Nous avons aussi étudié l’interaction des ondes internes avec une colonne de particules en sédimentation. Deux effets principaux ont été observés : la colonne oscille autour d’une position d’équilibre, et elle est déplacée dans son ensemble. La direction du déplacement de la colonne est expliquée par le calcul de l’effet de la dérive Lagrangienne produite pour des ondes. Cet effet pourrait également expliquer la dépendance en fréquence du déplacement<br>Internal waves are produced as a consequence of the dynamic balance between buoyancy and gravity forces when a particle of fluid is vertically displaced in a stably stratified environment. Geophysical systems such as ocean and atmosphere are naturally stratified and therefore suitable for internal waves propagation. Furthermore, these two environments stock a vast amount of particles at their boundaries and in their bulk. Therefore, internal waves and particles will inexorably interact in these systems. In this work, exploratory experiments are performed to study wave generated erosive transport of particles. In order to determine a transport threshold, the peculiar properties of internal waves (“critical reflection”) are employed to increase the intensity of the wave field at the boundaries. A method was developed in collaboration with a signal processing team to improve the determination of the wave components involved in near-critical reflection. This method enabled us to compare our experimental results with a theory of critical reflection, showing good agreement and allowing to extrapolate these results to experiments beyond ours and to oceanic conditions. In addition, we study the interaction of internal waves with a column of particles in sedimentation. Two main effects are observed: the column oscillates around an equilibrium position, and it is displaced as a whole. The direction of the displacement of the column is explained by computing the effect of the Lagrangian drift of the waves. This effect could also explain the frequency dependence of the displacement
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9

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.<br>Copies of author's previously published articles inserted. Includes bibliographical references (leaves 261-288).
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10

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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Книги з теми "Gravity waves"

1

Dastidar, Pranab R. Magneto-gravity. Mumbai: P.R. Dastidar, 2006.

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2

A, Datta, Sharman R. D, and Dryden Flight Research Facility, eds. Lee waves: Benign and malignant. Edwards, Calif: National Aeronautics and Space Administration, Dryden Flight Research Facility, 1993.

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3

Agnon, Yehuda. Nonlinear diffraction of ocean gravity waves. Woods Hole, Mass: Woods Hole Oceanographic Institution, 1986.

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4

Williams, JohnM. Tables of progressive gravity waves. Boston (Mass.): Pitman Advanced Publishing Program, 1985.

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5

Vanden-Broeck, J. M. Gravity-capillary free-surface flows. New York: Cambridge University Press, 2010.

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6

N, Hunt J., ed. Gravity waves in water of finite depth. Southampton: Computational Mechanics Publications, 1997.

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Vanden-Broeck, J. M. Gravity-capillary free-surface flows. New York: Cambridge University Press, 2010.

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8

Keeley, J. R. SAR sensitivities to surface gravity waves. Ottawa: Department of Fisheries and Oceans, 1992.

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9

K, Dutt P., and Langley Research Center, eds. Acoustic gravity waves: A computational approach. Hampton, Va: National Aeronautics and Space Administration, Langley Research Center, 1987.

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10

Rabinovich, A. B. Dlinnye gravitat͡s︡ionnye volny v okeane: Zakhvat, resonans, izluchenie. Sankt-Peterburg: Gidrometeoizdat, 1993.

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Частини книг з теми "Gravity waves"

1

Olbers, Dirk, Jürgen Willebrand, and Carsten Eden. "Gravity Waves." In Ocean Dynamics, 179–210. Berlin, Heidelberg: Springer Berlin Heidelberg, 2012. http://dx.doi.org/10.1007/978-3-642-23450-7_7.

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Hooke, William H. "Gravity Waves." In Mesoscale Meteorology and Forecasting, 272–88. Boston, MA: American Meteorological Society, 1986. http://dx.doi.org/10.1007/978-1-935704-20-1_12.

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Manasseh, Richard. "Internal gravity waves." In Fluid Waves, 119–32. Boca Raton: CRC Press, 2021. http://dx.doi.org/10.1201/9780429295263-5.

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Părău, Emilian I., and Jean-Marc Vanden-Broeck. "Gravity-Capillary and Flexural-Gravity Solitary Waves." In Nonlinear Water Waves, 183–99. Cham: Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-030-33536-6_11.

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Hogan, Peter A., and Dirk Puetzfeld. "‘Spherical’ Gravity Waves." In SpringerBriefs in Physics, 23–29. Cham: Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-031-16826-0_4.

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Pedlosky, Joseph. "Internal Gravity Waves." In Waves in the Ocean and Atmosphere, 59–66. Berlin, Heidelberg: Springer Berlin Heidelberg, 2003. http://dx.doi.org/10.1007/978-3-662-05131-3_7.

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Pierini, Stefano. "Internal Gravity Waves." In UNITEXT for Physics, 147–64. Cham: Springer Nature Switzerland, 2025. https://doi.org/10.1007/978-3-031-77991-6_11.

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Sakellariadou, Mairi. "Gravitational Waves." In Modified Gravity and Cosmology, 375–83. Cham: Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-83715-0_25.

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9

Maeder, André. "Transport by Gravity Waves." In Physics, Formation and Evolution of Rotating Stars, 449–72. Berlin, Heidelberg: Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-76949-1_17.

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Miles, Alan J., and B. Roberts. "Magnetoacoustic-Gravity Surface Waves." In Mechanisms of Chromospheric and Coronal Heating, 508–10. Berlin, Heidelberg: Springer Berlin Heidelberg, 1991. http://dx.doi.org/10.1007/978-3-642-87455-0_84.

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Тези доповідей конференцій з теми "Gravity waves"

1

AYON-BEATO, ELOY, GASTON GIRIBET, and MOKHTAR HASSAINE. "CRITICAL GRAVITY WAVES." In Proceedings of the MG13 Meeting on General Relativity. WORLD SCIENTIFIC, 2015. http://dx.doi.org/10.1142/9789814623995_0085.

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2

Mochimaru, Yoshihiro. "Gravity-capillary, solitary waves." In RENEWABLE ENERGY SOURCES AND TECHNOLOGIES. AIP Publishing, 2019. http://dx.doi.org/10.1063/1.5127488.

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3

Russo, Pedro, Pedro Oliveira, Catarina Sá-Dantas, Filipe Correia, and Vasco Almeida. "Faraday Waves Zero Gravity Experiment." In 56th International Astronautical Congress of the International Astronautical Federation, the International Academy of Astronautics, and the International Institute of Space Law. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2005. http://dx.doi.org/10.2514/6.iac-05-a2.p.04.

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4

Shafi, Qaisar. "Will Planck Observe Gravity Waves?" In The European Physical Society Conference on High Energy Physics. Trieste, Italy: Sissa Medialab, 2014. http://dx.doi.org/10.22323/1.180.0483.

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5

Lehn, Waldemar H., Wayne K. Silvester, and David M. Fraser. "Mirages with Atmospheric Gravity Waves." In Light and Color in the Open Air. Washington, D.C.: Optica Publishing Group, 1993. http://dx.doi.org/10.1364/lcoa.1993.thb.3.

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6

Onorato, Miguel. "Numerical Simulation Of Surface Gravity Waves." In 28th Conference on Modelling and Simulation. ECMS, 2014. http://dx.doi.org/10.7148/2014-0007.

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Trofimov, Evgenii A. "EXPERIMENTAL STUDY OF INTERNAL GRAVITY WAVES." In Science Present and Future: Research Landscape in the 21st century. Иркутск: Федеральное государственное бюджетное учреждение науки "Иркутский научный центр Сибирского отделения Российской академии наук", 2022. http://dx.doi.org/10.54696/isc_49741454.

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8

Lin, Chunshan, and Misao Sasaki. "Resonant Amplification of Primordial Gravitational Waves." In Second LeCosPA International Symposium: Everything about Gravity. WORLD SCIENTIFIC, 2017. http://dx.doi.org/10.1142/9789813203952_0035.

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Whiteway, J. A., and A. I. Carswell. "Rayleigh Lidar Measurements at Toronto." In Optical Remote Sensing of the Atmosphere. Washington, D.C.: Optica Publishing Group, 1991. http://dx.doi.org/10.1364/orsa.1991.owe8.

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Анотація:
Since June 1991, Rayleigh lidar measurements at York University are being carried out on a continuous basis (every clear night). The goal is to understand the properties of gravity waves and their effects on thermal structure in the mesosphere and upper stratosphere. This involves detailed study of: propagation of individual waves, interactions amongst gravity waves, gravity wave spectra, general wave characteristics as a function of altitude, the relationship between gravity waves and disturbances in thermal structure, and a developing climatology.
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Kim, Eun-jin. "Angular momentum transport by internal gravity waves." In Waves in dusty, solar and space plasmas. AIP, 2000. http://dx.doi.org/10.1063/1.1324948.

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Звіти організацій з теми "Gravity waves"

1

Guza, R. T. Surface Gravity Waves And Ambient Microseismic Noise. Fort Belvoir, VA: Defense Technical Information Center, September 1992. http://dx.doi.org/10.21236/ada256498.

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2

Muller, Peter. ARI: Internal Gravity Waves at Abrupt Topography. Fort Belvoir, VA: Defense Technical Information Center, January 1991. http://dx.doi.org/10.21236/ada266383.

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3

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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4

Ko, Dong S. A Multiscale Nested Modeling Framework to Simulate the Interaction of Surface Gravity Waves with Nonlinear Internal Gravity Waves. Fort Belvoir, VA: Defense Technical Information Center, September 2015. http://dx.doi.org/10.21236/ad1013704.

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5

Muller, Peter. Scattering of Internal Gravity Waves at Finite Topography. Fort Belvoir, VA: Defense Technical Information Center, September 1997. http://dx.doi.org/10.21236/ada628215.

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6

Bottone, Steven. Acoustic-Gravity Waves From Low-Altitude Localized Disturbances. Fort Belvoir, VA: Defense Technical Information Center, May 1993. http://dx.doi.org/10.21236/ada264804.

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7

Muller, Peter. Scattering of Internal Gravity Waves at Finite Topography. Fort Belvoir, VA: Defense Technical Information Center, September 2001. http://dx.doi.org/10.21236/ada624678.

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8

Sullivan, Peter P., James C. McWilliams, and Chin-Hoh Moeng. Surface Gravity Waves and Coupled Marine Boundary Layers. Fort Belvoir, VA: Defense Technical Information Center, September 2001. http://dx.doi.org/10.21236/ada625363.

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9

Silverstein, Eva, and Alexander Westphal. Monodromy in the CMB: Gravity Waves and String Inflation. Office of Scientific and Technical Information (OSTI), March 2008. http://dx.doi.org/10.2172/926191.

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Dunkerton, Timothy J. Gravity Waves in the Atmosphere: Instability, Saturation, and Transport. Fort Belvoir, VA: Defense Technical Information Center, November 1995. http://dx.doi.org/10.21236/ada303638.

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