Pages that link to "Item:Q468619"
From MaRDI portal
The following pages link to The existence of a pullback attractor for the three dimensional non-autonomous planetary geostrophic viscous equations of large-scale Ocean circulation (Q468619):
Displaying 11 items.
- Pullback attractors for three dimensional non-autonomous planetary geostrophic viscous equations of large-scale ocean circulation (Q478251) (← links)
- Non-autonomous planetary 3D geostrophic equations with oscillating external force and its global attractor (Q533029) (← links)
- Pullback \(\mathbb{V}\)-attractor of a three dimensional globally modified two-phase flow model (Q1661054) (← links)
- Optimal distributed control of the three-dimensional planetary geostrophic equations (Q2120307) (← links)
- Approximation of stationary statistical properties of the three dimensional autonomous planetary geostrophic equations of large-scale ocean circulation (Q2188137) (← links)
- Pullback attractors for the multi-layer quasi-geostrophic equations of the Ocean (Q2510883) (← links)
- Regularity ``in large'' for the \(3D\) Salmon's planetary geostrophic model of ocean dynamics (Q2687509) (← links)
- Random attractor for the three-dimensional planetary geostrophic equations of large-scale ocean circulation with small multiplicative noise (Q2804513) (← links)
- Random attractors for the three dimensional stochastical planetary geostrophic equations of large-scale ocean circulation (Q4584669) (← links)
- Global well‐posedness and finite‐dimensional global attractor for a 3‐D planetary geostrophic viscous model (Q4790321) (← links)
- Necessary and sufficient criteria for existence, regularity, and asymptotic stability of enhanced pullback attractors with applications to 3D primitive equations (Q6057504) (← links)