We estimate the wind speeds in Titan's thermosphere by considering the various terms of the wind equation, without actually solving it, with a view to anticipating what might be observed by the Cassini spacecraft in 2004. The winds, which are driven by horizontal pressure gradients produced by solar heating, are controlled in the Earth's thermosphere by ion-drag and coriolis force, but in Titan...

The most consistently useful simple model for the study of odd deformed nuclei, the particle-rotor model (strong coupling limit of the core-particle coupling model) has nevertheless been beset by a long-standing problem: It is necessary in many cases to introduce an ad hoc parameter that reduces the size of the Coriolis interaction coupling the collective and single-particle motions. Of the num...

The nonlinear theory of acoustic-gravity waves (AGWs) in the atmosphere is revisited with effects Coriolis force. Previous literature [Phys. Scr. \textbf{90} (2015) 055001] advanced. Starting from a set fluid equations modified by force, general linear dispersion relation derived which manifests coupling high-frequency and low-frequency internal gravity (IGWs). frequency IGWs enhanced Earth's a...

The Garrett and Munk spectrum describes the turbulence of ocean interior due to internal gravity waves. We use unique large scale Coriolis facility force by waves reproduce main features wave in a stratified fluid laboratory. A transition from weakly nonlinear strongly was indeed observed when increasing buoyancy Reynolds number.

In this paper, we study the number of traveling wave families near a shear flow under influence Coriolis force, where speeds lie outside range u. Under $$\beta $$ -plane approximation, if u has critical point at which attains its minimal (resp. maximal) value, then unique transitional value exists in positive negative) half-line such that changes suddenly from finite to infinite when passes thr...

We derive fully nonlinear, weakly dispersive model equations for propagation of surface gravity waves in a shallow, homogeneous ocean of variable depth on the surface of a rotating sphere. A numerical model is developed for the weakly nonlinear version of the model based on a combined finite-volume and finitedifference method with a fourth-order MUSCL-TVD scheme in space and a third-order SSP R...