Mathematical Modeling of Equatorial Atmospheric Waves Similar to Those Travelling along a Hexagon-shaped Path at the North Pole of Saturn
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Publication:4607563
DOI10.1051/mmnp/201712315zbMath1445.85002OpenAlexW2620063386MaRDI QIDQ4607563
Publication date: 14 March 2018
Published in: Mathematical Modelling of Natural Phenomena (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1051/mmnp/201712315
Free boundary problems for PDEs (35R35) Planetary atmospheres (85A20) Waves for incompressible viscous fluids (76D33) Other free boundary flows; Hele-Shaw flows (76D27)
Related Items (1)
Cites Work
- Symmetries and Conservation Laws of a Spectral Nonlinear Model for Atmospheric Baroclinic Jets
- A Spectral Method for the Vorticity Equation on the Surface
- Effects of rotation on stability of viscous stationary flows on a spherical surface
- Nonlinear viscous fluid patterns in a thin rotating spherical domain and applications
- Some results on the Navier-Stokes equations in thin 3D domains
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