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We report direct evidence of a secondary flow excited by the Earth rotation in a water-filled spherical container spinning at constant rotation rate. This so-called {\it tilt-over flow} essentially consists in a rotation around an axis…

流体动力学 · 物理学 2013-10-15 J. Boisson , D. Cébron , F. Moisy , P. -P. Cortet

The influence of rotation and magnetic fields on the physical properties of isothermal gas clouds is discussed. The presence of rotation and/or magnetic fields results in an increase of the critical cloud mass with respect to gravitational…

天体物理学 · 物理学 2009-11-07 B. Vollmer , W. J. Duschl

Rotation contributes to internal mixing processes and observed variability in massive stars. A significant number of binary stars are not in strict synchronous rotation, including all eccentric systems. This leads to a tidally induced and…

太阳与恒星天体物理 · 物理学 2021-09-29 Gloria Koenigsberger , Edmundo Moreno , Norbert Langer

We study the dynamical instability in spherical gravitating systems with core using the Ricci curvature criterion. By means of numerical estimations of the Ricci curvature for static N-body systems, it is shown that the core can both,…

天体物理学 · 物理学 2010-11-11 T. Ghahramanyan

Earth-mass planets are expected to have atmospheres and experience thermal tides raised by the host star. These tides transfer energy to the planet that can counter the dissipation from bodily tides. Indeed, even a relatively thin…

地球与行星天体物理 · 物理学 2023-12-13 Ema F. S. Valente , Alexandre C. M. Correia

The competition between the torques induced by solid and thermal tides drives the rotational dynamics of Venus-like planets and super-Earths orbiting in the habitable zone of low-mass stars. The tidal responses of the atmosphere and…

地球与行星天体物理 · 物理学 2017-07-19 Pierre Auclair-Desrotour , Jacques Laskar , Stéphane Mathis , Alexandre Correia

Two main seismic features characterize the Earth's inner core: a North-South polar anisotropy and an East-West asymmetry of P-wave velocity and attenuation. Anisotropy is expected if shear deformation is induced by convective motions.…

地球物理 · 物理学 2015-06-04 Hugau Mizzon , Marc Monnereau

Bar structures can form internally due to the instability of their host galaxies or externally due to perturbations from other galaxies. We systematically quantify the growth timescales ($\tau_\mathrm{bar}$) of bars formed through these two…

星系天体物理 · 物理学 2025-07-01 Yirui Zheng , Juntai Shen , Xufen Wu , Bin-Hui Chen

The polar motion data is analyzed to obtain accurate position of the figure axis referred to the Earth-fixed frame. The variation of the figure axis should be the basic object to which the geophysical events are linked. By the method of…

地球与行星天体物理 · 物理学 2012-06-25 Yoshio Kubo

The motion of two planets around a Sun-like star under the combined effects of mutual interaction and tidal dissipation is investigated. The secular behaviour of the system is analyzed using two different approaches. First, we solve the…

地球与行星天体物理 · 物理学 2015-05-27 Adrián Rodríguez , Sylvio Ferraz-Mello , Tatiana A. Michtchenko , Cristian Beaugé , Octavio Miloni

Gravitational tidal interactions drive long-term rotational and orbital evolution in planetary systems, in multiple (particularly close binary) star systems and in planetary moon systems. Dissipation of tidal flows in Earth's oceans is…

地球与行星天体物理 · 物理学 2025-04-16 Adrian J. Barker

Inner core translation, with solidification on one hemisphere and melting on the other, provides a promising basis for understanding the hemispherical dichotomy of the inner core, as well as the anomalous stable layer observed at the base…

地球物理 · 物理学 2015-06-16 Renaud Deguen , Thierry Alboussière , Philippe Cardin

The Earth acts as a gigantic heat engine driven by decay of radiogenic isotopes and slow cooling, which gives rise to plate tectonics, volcanoes, and mountain building. Another key product is the geomagnetic field, generated in the liquid…

地球物理 · 物理学 2015-06-04 Monica Pozzo , Chris Davies , David Gubbins , Dario Alfè

Convective flow in Earth's iron-rich liquid core drives self-sustained dynamo action, generating Earth's magnetic field, which is strongest among all terrestrial planets of the solar system. Rock records show that this magnetic field has…

地球与行星天体物理 · 物理学 2025-08-04 Urmi Dutta , Chris J. Davies , Ashley P. Willis

In a multiplanet system, tides acting on the inner planet can significantly affect the orbital evolution of the entire system. While tides usually damp eccentricities, a novel mechanism identified by Correia et al. (2012) tends to raise…

地球与行星天体物理 · 物理学 2015-06-17 Richard Greenberg , Christa Van Laerhoven , Rory Barnes

The inertial (due to rotation) and gravitational fields of the Earth affect the motion of an elementary particle and its spin dynamics. This influence is not negligible and should be taken into account in high-energy physics experiments.…

广义相对论与量子宇宙学 · 物理学 2016-08-15 Yuri N. Obukhov , Alexander J. Silenko , Oleg V. Teryaev

It is usually believed that the geo-dynamo of the Earth or more generally of other planets, is created by the convective fluid motions inside their molten cores. An alternative to this thermal or compositional convection can however be…

流体动力学 · 物理学 2016-08-16 P. Le Gal , L. Lacaze , S. Le Dizès

Free core nutation (FCN) is the main factor that limits the accuracy of the modeling of the motion of Earth's rotational axis in the celestial coordinate system. Several FCN models have been proposed. A comparative analysis is made of the…

地球物理 · 物理学 2009-08-14 Zinovy Malkin

It has long been assumed the Earth's solid inner core started to grow when molten iron cooled to its melting point. However, the nucleation mechanism, which is a necessary step of crystallization, has not been well understood. Recent…

地球物理 · 物理学 2022-01-11 Yang Sun , Feng Zhang , Mikhail I. Mendelev , Renata M. Wentzcovitch , Kai-Ming Ho

Two-component convection driven by both compositional and thermal buoyancy within the fluid core of a rapidly rotating planet produces a predominantly axial dipole field. In a dynamo driven by strong compositional buoyancy that by itself…

流体动力学 · 物理学 2026-03-31 Debarshi Majumder , Binod Sreenivasan