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Relevant bibliographies by topics / Tidal dipole

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Journal articles
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Academic literature on the topic 'Tidal dipole'

Author: Grafiati

Published: 4 June 2021

Last updated: 19 February 2022

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Journal articles on the topic "Tidal dipole"

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Wells, Mathew G., and Gert-Jan F. van Heijst. "A model of tidal flushing of an estuary by dipole formation." Dynamics of Atmospheres and Oceans 37, no. 3 (2003): 223–44. http://dx.doi.org/10.1016/j.dynatmoce.2003.08.002.

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Rainey, R. C. T. "Key features of wave energy." Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 370, no. 1959 (2012): 425–38. http://dx.doi.org/10.1098/rsta.2011.0251.

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For a weak point source or dipole, or a small body operating as either, we show that the power from a wave energy converter (WEC) is the product of the particle velocity in the waves, and the wave force (suitably defined). There is a thus a strong analogy with a wind or tidal turbine, where the power is the product of the fluid velocity through the turbine, and the force on it. As a first approximation, the cost of a structure is controlled by the force it has to carry, which governs its strength, and the distance it has to be carried, which governs its size. Thus, WECs are at a disadvantage c

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TOMOZAWA, YUKIO. "THE CMB DIPOLE AND CIRCULAR GALAXY DISTRIBUTION." Modern Physics Letters A 22, no. 21 (2007): 1553–67. http://dx.doi.org/10.1142/s0217732307023936.

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The validity of Hubble's law defies the determination of the center of the big bang expansion, even if it exists. Every point in the expanding universe looks like the center from which the rest of the universe flies away. In this paper, we show that the distri- bution of apparently circular galaxies is not uniform in the sky and that there exists a special direction in the universe in our neighborhood. The data is consistent with the assumption that the tidal force due to the mass distribution around the universe center causes the deformation of galactic shapes depending on its orientation and

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Yahil, A. "Contributions to the Local Gravitational Field from beyond the Local Supercluster." Symposium - International Astronomical Union 117 (1987): 435–43. http://dx.doi.org/10.1017/s0074180900150673.

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IRAS 60μ sources are used to map the local (≲200h−1 Mpc, Ho =100h km s−1 Mpc−1) gravitational field, and to determine its dipole component, on the assumption that the infrared radiation traces the matter. The dipole moment is found to point in the direction of the anisotropy of the microwave background radiation. Comparison of the two anisotropies, using linear perturbation theory, yields an estimate of the cosmological density parameter, Ω =0.85±0.16, with nonlinear effects increasing Ωo by ∼15%. The quadrupolar tidal field within the Local Supercluster, due presumably to the same density inh

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Costa, L. Filipe O., and Carlos A. R. Herdeiro. "The gravitational force on a gyroscope and the electromagnetic force on a magnetic dipole as analogous tidal effects." Journal of Physics: Conference Series 229 (May 1, 2010): 012031. http://dx.doi.org/10.1088/1742-6596/229/1/012031.

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Grue, John. "Nonlinear interfacial wave formation in three dimensions." Journal of Fluid Mechanics 767 (February 23, 2015): 735–62. http://dx.doi.org/10.1017/jfm.2015.42.

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AbstractA three-dimensional two-layer, fully dispersive and strongly nonlinear interfacial wave model, including the interaction with a time-varying bottom topography, is developed. The method is based on a set of integral equations. The source and dipole terms are developed in series expansions in the vertical excursions of the interface and bottom topography, obtaining explicit inversion by Fourier transform. Calculations of strongly nonlinear interfacial waves with excursions comparable to the thinner layer depth show that the quadratic approximation of the method contains the essential dyn

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Cartwright, Paula J., Peter R. C. S. Fearns, Paul Branson, et al. "Identifying Metocean Drivers of Turbidity Using 18 Years of MODIS Satellite Data: Implications for Marine Ecosystems under Climate Change." Remote Sensing 13, no. 18 (2021): 3616. http://dx.doi.org/10.3390/rs13183616.

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Turbidity impacts the growth and productivity of marine benthic habitats due to light limitation. Daily/monthly synoptic and tidal influences often drive turbidity fluctuations, however, our understanding of what drives turbidity across seasonal/interannual timescales is often limited, thus impeding our ability to forecast climate change impacts to ecologically significant habitats. Here, we analysed long term (18-year) MODIS-aqua data to derive turbidity and the associated meteorological and oceanographic (metocean) processes in an arid tropical embayment (Exmouth Gulf in Western Australia) w

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Pearson, K. J., G. A. Wynn, and A. R. King. "Simulations of Angular Momentum Evolution in Wind-Fed CV Precursors." International Astronomical Union Colloquium 158 (1996): 443–44. http://dx.doi.org/10.1017/s025292110003935x.

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It is thought that the secondary stars in cataclysmic variables (CVs) may undergo a period of mass loss in the form of a wind during the evolution of the system (Mullan et al. 1992). This wind is thought to magnetically brake the secondary star with a time-scale ~ 108 yr (e.g. van Paradijs 1986). When the secondary’s spin has been brought close to synchronism with the orbit it is possible for tidal torques to lock the secondary in synchronous rotation.We have modelled this process by adapting a method that has proved successful in explaining the properties of the intermediate polars (Wynn &amp

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Morris, Mark. "8.1. Magnetic phenomena in galactic nuclei." Symposium - International Astronomical Union 184 (1998): 331–40. http://dx.doi.org/10.1017/s0074180900085144.

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The magnetic environment of the Galactic nucleus contrasts sharply with that of the Galactic disk. The inner few hundred parsecs of our Galaxy appear to be dominated by a strong (~milligauss) and uniform dipole field which dominates the pressure within the central intercloud medium. An attractive hypothesis for the origin of the central vertical field is that it results from the concentration of protogalactic field by radial inflow of gas throughout the Galaxy's lifetime. The predominant orientation of the magnetic field within dense molecular clouds is parallel to the galactic plane, which ca

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Sasaki, Hideharu, Shinichiro Kida, Ryo Furue, et al. "A global eddying hindcast ocean simulation with OFES2." Geoscientific Model Development 13, no. 7 (2020): 3319–36. http://dx.doi.org/10.5194/gmd-13-3319-2020.

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Abstract. A quasi-global eddying ocean hindcast simulation using a new version of our model, called OFES2 (Ocean General Circulation Model for the Earth Simulator version 2), was conducted to overcome several issues with unrealistic properties in its previous version, OFES. This paper describes the model and the simulated oceanic fields in OFES2 compared with OFES and also observed data. OFES2 includes a sea-ice model and a tidal mixing scheme, is forced by a newly created surface atmospheric dataset called JRA55-do, and simulated the oceanic fields from 1958 to 2016. We found several improvem

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Dissertations / Theses on the topic "Tidal dipole"

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Nicolau, del Roure Francisco. "Laboratory studies of eddy structures and exchange processes through tidal inlets." [College Station, Tex. : Texas A&M University, 2007. http://hdl.handle.net/1969.1/ETD-TAMU-1949.

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Whilden, Kerri Ann. "Laboratory Analysis of Vortex Dynamics For Shallow Tidal Inlets." 2009. http://hdl.handle.net/1969.1/ETD-TAMU-2009-08-7178.

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Estuaries depend on the transport of nutrients and sediments from the open sea to help maintain a prosperous environment. One of the major transport mechanisms is the propagation of large two dimensional vortical structures. At the mouth of an inlet, tidal flow forces the formation of two dimensional vortical structures whose lateral extent is much greater than the water depth. After the starting jet vortex dipole detaches from the inlet, secondary vortices shed due to separation from the inlet boundary and eventually reach the starting-jet dipole. An idealized inlet con figuration was utiliz

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Book chapters on the topic "Tidal dipole"

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van Heijst, G., and M. Wells. "Dipole formation by tidal flow in a channel." In Shallow Flows. Taylor & Francis, 2004. http://dx.doi.org/10.1201/9780203027325.ch7.

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Conference papers on the topic "Tidal dipole"

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Chowdhury, Piyali, and Manasa Ranjan Behera. "Impact of Climate Modes on Shoreline Evolution: Southwest Coast of India." In ASME 2017 36th International Conference on Ocean, Offshore and Arctic Engineering. American Society of Mechanical Engineers, 2017. http://dx.doi.org/10.1115/omae2017-61354.

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Coastal geomorphology is a complex phenomenon which is governed by nearshore wave and tidal climate. Change in climate indices (like sea surface temperature, sea level, intensified cyclone activity, among others) and climate modes (like El Nino Southern Oscillation (ENSO), Southern Annular Mode (SAM), Indian Ocean Dipole (IOD)) affect the wave climate and modify many coastal processes thereby altering the geomorphology of shorelines. In countries like India where tropical and sub-tropical cyclones are common, the coastal geomorphology is under constant threat. Coasts are also vulnerable to ant

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Goldschmidt, Margalit Z., Michael L. Jonson, and Joseph F. Horn. "Acoustic Control of a Maneuverable Marine Hydrokinetic Cycloturbine." In ASME 2019 International Mechanical Engineering Congress and Exposition. American Society of Mechanical Engineers, 2019. http://dx.doi.org/10.1115/imece2019-11381.

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Abstract Marine Hydrokinetic (MHK) cycloturbines exploit tidal currents to generate sustainable electric power. Because of the harsh marine environment, MHK cycloturbines require frequent maintenance and repair, which for current systems necessitates the use of a ship, making the process difficult and costly. A novel MHK cycloturbine system has been designed that uses pitching foils for maneuver, potentially circumventing the costs and difficulties associated with deployment and repairs. The vehicle fatigue is decreased and the vehicle’s acoustic signature underwater is reduced by design of a

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