Maximum principles for the primitive equations of the atmosphere
From MaRDI portal
Publication:1864103
DOI10.3934/dcds.2001.7.343zbMath1030.86004OpenAlexW1988567082MaRDI QIDQ1864103
Publication date: 16 March 2003
Published in: Discrete and Continuous Dynamical Systems (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.3934/dcds.2001.7.343
Lua error in Module:PublicationMSCList at line 37: attempt to index local 'msc_result' (a nil value).
Related Items (13)
Optimal distributed control of the three-dimensional planetary geostrophic equations ⋮ Some boundedness of solutions for the primitive equations of the atmosphere and the ocean ⋮ Global attractors for the three-dimensional viscous primitive equations of large-scale atmosphere in log-pressure coordinate ⋮ Random attractors for the three dimensional stochastical planetary geostrophic equations of large-scale ocean circulation ⋮ The equations of the atmosphere with humidity and saturation: uniqueness and physical bounds ⋮ The existence of a pullback attractor for the three dimensional non-autonomous planetary geostrophic viscous equations of large-scale Ocean circulation ⋮ Pullback attractors for three dimensional non-autonomous planetary geostrophic viscous equations of large-scale ocean circulation ⋮ Global attractor of the three-dimensional primitive equations of large-scale Ocean and atmosphere dynamics ⋮ Phase transition models in atmospheric dynamics ⋮ Random attractor for the three-dimensional planetary geostrophic equations of large-scale ocean circulation with small multiplicative noise ⋮ On a model of target detection in molecular communication networks ⋮ Pullback attractor for nonautonomous primitive equations of large-scale ocean and atmosphere dynamics ⋮ Approximation of stationary statistical properties of the three-dimensional primitive equations of large-scale ocean and atmosphere dynamics
This page was built for publication: Maximum principles for the primitive equations of the atmosphere
