Academic literature on the topic 'Earth tides'

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Journal articles on the topic "Earth tides"

1

Gemael, Camil. "Earth Tides in Brazil." Zentralblatt für Geologie und Paläontologie, Teil I 1985, no. 9-10 (1986): 1495–500. http://dx.doi.org/10.1127/zbl_geol_pal_1/1985/1986/1495.

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2

Kuo, John T. "Earth tides." Reviews of Geophysics 25, no. 5 (1987): 847. http://dx.doi.org/10.1029/rg025i005p00847.

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3

Levin, B. W., and E. V. Sasorova. "Seismotectonics and Earth tides." Russian Journal of Pacific Geology 6, no. 1 (2012): 70–77. http://dx.doi.org/10.1134/s1819714012010095.

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4

Agnew, Duncan C. "Time and tide: pendulum clocks and gravity tides." History of Geo- and Space Sciences 11, no. 2 (2020): 215–24. http://dx.doi.org/10.5194/hgss-11-215-2020.

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Abstract. Tidal fluctuations in gravity will affect the period of a pendulum and hence the timekeeping of any such clock that uses one. Since pendulum clocks were, until the 1940s, the best timekeepers available, there has been interest in seeing if tidal effects could be observed in the best performing examples of these clocks. The first such observation was in 1929, before gravity tides were measured with spring gravimeters; at the time of the second (1940–1943), such gravimeters were still being developed. Subsequent observations, having been made after pendulum clocks had ceased to be the
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5

Goring, Derek G., and Roy A. Walters. "Ocean‐tide loading and Earth tides around New Zealand." New Zealand Journal of Marine and Freshwater Research 36, no. 2 (2002): 299–309. http://dx.doi.org/10.1080/00288330.2002.9517087.

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6

Dehant, V., P. Defraigne, and J. M. Wahr. "Tides for a convective Earth." Journal of Geophysical Research: Solid Earth 104, B1 (1999): 1035–58. http://dx.doi.org/10.1029/1998jb900051.

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7

Auclair-Desrotour, P., J. Laskar, and S. Mathis. "Atmospheric tides in Earth-like planets." Astronomy & Astrophysics 603 (July 2017): A107. http://dx.doi.org/10.1051/0004-6361/201628252.

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Context. Atmospheric tides can strongly affect the rotational dynamics of planets. In the family of Earth-like planets, which includes Venus, this physical mechanism coupled with solid tides makes the angular velocity evolve over long timescales and determines the equilibrium configurations of their spin. Aims. Unlike the solid core, the atmosphere of a planet is subject to both tidal gravitational potential and insolation flux coming from the star. The complex response of the gas is intrinsically linked to its physical properties. This dependence has to be characterized and quantified for app
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8

Vieira, R. "Xth International Symposium on Earth Tides." Bulletin Géodésique 61, no. 2 (1987): 201–2. http://dx.doi.org/10.1007/bf02521269.

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9

Bai, Yanzhuo, Shengwen Chang, and Shangcheng Wu. "Relationship Between Earth-Moon Distance and Tides." Highlights in Science, Engineering and Technology 85 (March 13, 2024): 286–92. http://dx.doi.org/10.54097/xkxh4q35.

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For residents and fishermen in coastal cities, tidal phenomena are a dangerous existence, and for tidal power stations, tidal phenomena will bring clean energy to them. For the formation of tidal phenomena, the most closely related is the distance between the Earth and the Moon. Therefore, this paper collects the tides and Earth-Moon records in New York in 2022, and performs data visualization operations on the data, and uses STL (Seasonal Decomposition of Time Series), MSTL (Multiple Seasonal-Trend Decomposition using Loess) models to predict, so as to explore the concern between the Earth-Mo
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10

Navarro, Thomas, Timothy M. Merlis, Nicolas B. Cowan, and Natalya Gomez. "Atmospheric Gravitational Tides of Earth-like Planets Orbiting Low-mass Stars." Planetary Science Journal 3, no. 7 (2022): 162. http://dx.doi.org/10.3847/psj/ac76cd.

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Abstract Temperate terrestrial planets orbiting low-mass stars are subject to strong tidal forces. The effects of gravitational tides on the solid planet and that of atmospheric thermal tides have been studied, but the direct impact of gravitational tides on the atmosphere itself has so far been ignored. We first develop a simplified analytic theory of tides acting on the atmosphere of a planet. We then implement gravitational tides into a general circulation model of a static-ocean planet in a short-period orbit around a low-mass star—the results agree with our analytic theory. Because atmosp
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