Rapid Spin Up and Spin Down of Flow Along Slopes
Henry G. Peterson, J\"orn Callies

TL;DR
This paper extends a one-dimensional model of stratified flow over slopes to include rapid spin up and spin down dynamics, capturing the physics of interior return flows driven by Ekman transport and Coriolis effects.
Contribution
The work introduces a constrained 1D model that incorporates interior return flow, enabling the simulation of rapid spin up and spin down phenomena along slopes, based on 2D dynamics.
Findings
The extended model accurately reproduces 2D mixing-generated spin up.
It provides a unified framework for Ekman arrest and spin down processes.
The model captures rapid adjustment of interior flows due to Coriolis acceleration.
Abstract
The near-bottom mixing that allows abyssal waters to upwell tilts isopycnals and spins up flow over the flanks of mid-ocean ridges. Meso- and large-scale currents along sloping topography are subjected to a delicate balance of Ekman arrest and spin down. These two seemingly disparate oceanographic phenomena share a common theory, which is based on a one-dimensional model of rotating, stratified flow over a sloping, insulated boundary. This commonly used model, however, lacks rapid adjustment of interior flows, limiting its ability to capture the full physics of spin up and spin down of along-slope flow. Motivated by two-dimensional dynamics, the present work extends the one-dimensional model by constraining the vertically integrated cross-slope transport and allowing for a barotropic cross-slope pressure gradient. This produces a closed secondary circulation by forcing Ekman transport…
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