scholarly journals Flow at the interface of two rotating fluids

2019 ◽  
Vol 1382 ◽  
pp. 012026
Author(s):  
I V Naumov ◽  
B R Sharifullin ◽  
V N Shtern
Keyword(s):  
1995 ◽  
Vol 74 (4) ◽  
pp. 530-533 ◽  
Author(s):  
Juan Millán-Rodríguez ◽  
Michael Bestehorn ◽  
Carlos Pérez-García ◽  
Rudolf Friedrich ◽  
Marc Neufeld
Keyword(s):  

1970 ◽  
Vol 42 (4) ◽  
pp. 803-822 ◽  
Author(s):  
S. Leibovich

The Korteweg–de Vries equation is shown to govern formation of solitary and cnoidal waves in rotating fluids confined in tubes. It is proved that the method must fail when the tube wall is moved to infinity, and the failure is corrected by singular perturbation procedures. The Korteweg–de Vries equation must then give way to an integro-differential equation. Also, critical stationary flows in tubes are considered with regard to Benjamin's vortex breakdown theories.


Author(s):  
Emmanuel Dormy ◽  
Radostin Simitev ◽  
Friedrich Busse ◽  
Andrew Soward
Keyword(s):  

2010 ◽  
Vol 90 (1) ◽  
pp. 135-144
Author(s):  
Milivoj Gavrilov ◽  
Lazar Lazic ◽  
Jasmina Djordjevic

Out of all atmospheric processes on the planets of the Solar System, special attention will be devoted here to leading circulation of planetary or global scales, known as Rossby waves. These waves occur in all rotating fluids that have relative movement to the rotation system. Rossby waves exert dominant influence on so-called global weather. Based on the knowledge of some properties of Rossby waves are made approximate analysis of weather conditions on the planets of the Solar System. Also, these considerations can serve as an introduction to weather forecasting on the planet. .


2018 ◽  
Vol 3 (2) ◽  
pp. 627-648 ◽  
Author(s):  
A. Durán

AbstractIn this paper a rotating two-fluid model for the propagation of internal waves is introduced. The model can be derived from a rotating-fluid problem by including gravity effects or from a nonrotating one by adding rotational forces in the dispersion balance. The physical regime of validation is discussed and mathematical properties of the new system, concerning well-posedness, conservation laws and existence of solitary-wave solutions, are analyzed.


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