Extended deep equatorial layering as a possible imprint of inertial instability

12Citations
Citations of this article
12Readers
Mendeley users who have this article in their library.

This article is free to access.

Abstract

The deep equatorial track of the world ocean is subject to intense zonal flow fields that still remain to be better understood. Inertial instability has been invoked to explain some of its features. Here we present possible in situ imprints of such a mechanism in the equatorial Atlantic Ocean below the thermocline. We analyse the observed pattern of homogeneous density layers of 50-100 m vertical scale, which are characterized by a large meridional coherency up to 2° of latitude, a concentration in the vicinity of the equator and foremost a vertical localization within regions of well-mixed angular momentum (westward jets). These distinctive properties suggest inertial instability to be a plausible mechanism for this extended layering. Numerical simulations forced by a time-oscillating shear reproduce the observed density layering characteristics. The prescription of deep jets in the background flow controls the vertical localization of the layering inside westward jets. Copyright 2004 by the American Geophysical Union.

Cite

CITATION STYLE

APA

d’Orgeville, M., Hua, B. L., Schopp, R., & Bunge, L. (2004). Extended deep equatorial layering as a possible imprint of inertial instability. Geophysical Research Letters, 31(22), 1–5. https://doi.org/10.1029/2004GL020845

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free