LES of a real campus finds shielding controls individual building drag, quantified by upstream fetch ratio L_s/H_s and relative height ratio H_s/H.
(1962), Finite amplitude free convection as an initial value problem - I
4 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 4representative citing papers
Dynamo-generated magnetic fields confine the tachocline against radiative spreading in global simulations, with stronger stable stratification producing longer cycles, deeper penetration via skin effect, and better confinement plus interior spin-down transmission.
Sparse hierarchies of K coupled gyrostats (M=2K+1 modes, no linear feedback) possess exactly (M+1)/2 quadratic invariants recoverable as Casimirs of a constructible non-canonical Poisson structure.
3D anelastic simulations find that both convective zone Busse columns and weather-layer PV homogenization produce Jupiter-like jets, with the weather layer causing deviations in thermal wind balance and long-term high-latitude jet migration.
citing papers explorer
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Building drag and shielding in a realistic urban environment
LES of a real campus finds shielding controls individual building drag, quantified by upstream fetch ratio L_s/H_s and relative height ratio H_s/H.
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A Dynamo Confinement Scenario for the Solar Tachocline and its Implications for Spin-down in the Radiative Spreading Regime
Dynamo-generated magnetic fields confine the tachocline against radiative spreading in global simulations, with stronger stable stratification producing longer cycles, deeper penetration via skin effect, and better confinement plus interior spin-down transmission.
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Quadratic invariants and Hamiltonian structure in coupled gyrostat low-order model hierarchies
Sparse hierarchies of K coupled gyrostats (M=2K+1 modes, no linear feedback) possess exactly (M+1)/2 quadratic invariants recoverable as Casimirs of a constructible non-canonical Poisson structure.
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Superrotation and Jet Migration in Simulations of Jupiter's Convective Zone and Weather Layer
3D anelastic simulations find that both convective zone Busse columns and weather-layer PV homogenization produce Jupiter-like jets, with the weather layer causing deviations in thermal wind balance and long-term high-latitude jet migration.