Horizontal shear instabilities in low-Froude high-Re stratified flows produce vertical shear through two distinct pathways, each leading to small-scale KH instabilities at large buoyancy Reynolds number but with different peak mixing efficiencies.
year = 1997, month = jan, volume =
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
years
2026 3verdicts
UNVERDICTED 3representative citing papers
A lithium chemical evolution model for the GSE galaxy matches survey data showing Spite-like and eRGB plateaus at low metallicity with a hint of reduced nova contributions.
New spectroscopic measurements of RGB stars in nine open clusters confirm mass-dependent extra-mixing processes and indicate that initial 17O and 18O abundances may vary.
citing papers explorer
-
Two pathways to diapycnal mixing in strongly stratified flows with no initial vertical shear
Horizontal shear instabilities in low-Froude high-Re stratified flows produce vertical shear through two distinct pathways, each leading to small-scale KH instabilities at large buoyancy Reynolds number but with different peak mixing efficiencies.
-
Gaia-Sausage-Enceladus: Lithium evolution from early red-giant-branch and main-sequence stars
A lithium chemical evolution model for the GSE galaxy matches survey data showing Spite-like and eRGB plateaus at low metallicity with a hint of reduced nova contributions.
-
Spectroscopic analysis of RGB stars in nine open clusters
New spectroscopic measurements of RGB stars in nine open clusters confirm mass-dependent extra-mixing processes and indicate that initial 17O and 18O abundances may vary.