Results 41 to 50 of about 349,003 (221)
Tidal dissipation in Europa: A correction [PDF]
The possibility that tidal dissipation in a thin ice crust was sufficient to preserve liquid water on Jupiter's satellite Europa was suggested by Cassen et al. [1979]. However, their calculation of the tidal heating rate for that situation is in error.
P. Cassen, S. J. Peale, R. T. Reynolds
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Dispersion processes in weakly dissipative tidal channels
We report the results of an extensive experimental campaign dedicated to the analysis of turbulent dispersion owing to the circulations in tidal environments, characterized by a tidal inlet and a channel with lateral tidal flats. We focus on weakly-convergent and weakly-dissipative estuaries or tidal embankments, where the internal waters communicate ...
De Leo, Annalisa +2 more
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Unravelling tidal dissipation in gaseous giant planets [PDF]
International audienceContext. Tidal dissipation in planetary interiors is one of the key physical mechanisms that drive the evolution of star-planet and planet-moon systems.
M. Guenel +5 more
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Tidal Dissipation in Rotating Giant Planets
[Abridged] Tides may play an important role in determining the observed distributions of mass, orbital period, and eccentricity of the extrasolar planets. In addition, tidal interactions between giant planets in the solar system and their moons are thought to be responsible for the orbital migration of the satellites, leading to their capture into ...
Ogilvie, G. I., Lin, D. N. C.
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Tidal Dissipation in WASP-12 [PDF]
Abstract WASP-12 is a hot Jupiter system with an orbital period of P = 1.1 days, making it one of the shortest-period giant planets known. Recent transit timing observations by Maciejewski et al. and Patra et al. found a decreasing period with = 3.2 Myr.
Nevin N. Weinberg +3 more
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Tidal deformation and dissipation of rotating black holes [PDF]
6+1 pages, 1 figure; updated to match published ...
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Tidal Dissipation in Stars and Giant Planets [PDF]
Astrophysical fluid bodies that orbit close to one another induce tidal distortions and flows that are subject to dissipative processes. The spin and orbital motions undergo a coupled evolution over astronomical timescales, which is relevant for many types of binary star, short-period extrasolar planetary systems, and the satellites of the giant ...
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Energy dissipation in a tidal estuary [PDF]
The extent and mechanism of energy dissipation has been studied in Coos Bay, a coastal plain estuary. Coos Bay is located on the central Oregon coast, 184 nautical miles south of Astoria, Oregon, and 35 nautical miles north of Cape Blanco.
Blanton, Jackson Orin
core +4 more sources
Tidal Dissipation in Rotating Solar‐Type Stars [PDF]
We calculate the excitation and dissipation of low-frequency tidal oscillations in uniformly rotating solar-type stars. For tidal frequencies smaller than twice the spin frequency, inertial waves are excited in the convective envelope and are dissipated by turbulent viscosity. Enhanced dissipation occurs over the entire frequency range rather than in a
Ogilvie, G. I., Lin, D. N. C.
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Synchronization‐Dissipation in the Cardiorespiratory System
By modeling central nervous coupling and viscoelastic interactions in the cardiorespiratory system we show that synchronization produces a 10% gain in cardiac efficiency in humans. It is surmised that respiratory sinus arrhythmia improves cardiac pumping efficiency by reducing dynamic stress and power dissipation in the pulmonary vasculature.
Joshua R. Border +3 more
wiley +1 more source

