Pith. sign in

REVIEW

Compressible turbulent convection in highly stratified adiabatic background

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2305.16479 v3 pith:6ET27V3E submitted 2023-05-25 physics.flu-dyn astro-ph.SR

Compressible turbulent convection in highly stratified adiabatic background

classification physics.flu-dyn astro-ph.SR
keywords convectioncompressiblehighlyturbulentadiabaticasymmetrydensityheat
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

Buoyancy-driven turbulent convection leads to a fully compressible flow with a strong top-down asymmetry of first- and second-order statistics when the adiabatic equilibrium profiles of temperature, density and pressure decay very strongly across the convection layer. The growth of this asymmetry and the formation of an increasingly thicker stabilized sublayer with a negative mean convective heat flux at the top of the convection zone is reported here by a series highly resolved three-dimensional direct numerical simulations beyond the Oberbeck-Boussinesq and anelastic limits for dimensionless dissipation numbers $0.1 \le D\le 0.8$ at fixed Rayleigh number $Ra=10^6$ and superadiabaticity. The highly stratified compressible convection regime appears for $D > D_{\rm crit}\approx 0.65$, when density fluctuations collapse to those of pressure; it is characterized by an up to nearly 50\% reduced global turbulent heat transfer and a sparse network of focused thin thermal plumes falling through the top sublayer deep into the bulk.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.