Publication 107 · Ocean and geophysical convection
Toward understanding polar heat transport enhancement in subglacial oceans on icy moons
R. Hartmann, R.J.A.M. Stevens, D. Lohse, R. Verzicco, Geophys. Res. Lett. 51 (3) e2023GL105401 (2024).
Main finding
The local polar enhancement and low-latitude reduction are strong within the sampled no-slip Ra=10^6 DNS. The global response is a reduction, not an enhancement. The boundary-layer and rapid-rotation scalings are consistency interpretations, and icy-moon relevance remains qualitative and quantitatively unvalidated.
Why this matters
Why rotation can redistribute heat toward poles without increasing the global total.
Research context
The spherical-shell calculation extends rotating-convection ideas from cylindrical cells to latitude-dependent geometry. Alignment of buoyancy and rotation permits Taylor-column and Ekman-pumping enhancement near the poles, whereas their near-orthogonal orientation suppresses radial transport at low latitude; salinity and planetary parameter values remain outside the simulated regime.
Read the article View in the complete publication list Related research