In adiabatically stratified cluster gas the MTI saturates via large plumes destroyed by shear, producing turbulent kinetic energy that scales as χ ω_T.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
DNS identify four power-law regimes in Nusselt number versus aspect ratio in differentially heated cavities, with maximum heat flux at Re_u/Re_v ≈ 0.45 and optimal aspect ratio scaling as Γ_opt ∼ Ra^{-0.19}.
citing papers explorer
-
Magneto-Thermal Instability in Galaxy Clusters -- III. The Limit of Adiabatic Stratification
In adiabatically stratified cluster gas the MTI saturates via large plumes destroyed by shear, producing turbulent kinetic energy that scales as χ ω_T.
-
Geometry-controlled heat transport pathways and optimal heat transfer in differentially heated cavities
DNS identify four power-law regimes in Nusselt number versus aspect ratio in differentially heated cavities, with maximum heat flux at Re_u/Re_v ≈ 0.45 and optimal aspect ratio scaling as Γ_opt ∼ Ra^{-0.19}.