The role of the geothermal heat flux in driving the abyssal ocean circulation. Issue 12 (25th June 2013)

• Record Type: Journal Article
• Authors: Mashayek, A.; Ferrari, R.; Vettoretti, G.; Peltier, W. R.
• Is Part Of: Geophysical research letters. Volume 40:Issue 12(2013:Jun.)
• Page Start: 3144
• Page End: 3149
• Publication Date: 2013-06-25
• Subjects: Geophysics -- Periodicals; Planets -- Periodicals; Lunar geology -- Periodicals; 550
• DOI: 10.1002/grl.50640
• Languages: English
• ISSNs: 0094-8276

Abstract

<abstract abstract-type="main" id="grl50640-abs-0001"> <title> <x xml:space="preserve">Abstract</x> </title> <p id="grl50640-para-0001">[1] The results presented in this paper demonstrate that the geothermal heat flux (GHF) from the solid Earth into the ocean plays a non‐negligible role in determining both abyssal stratification and circulation strength. Based upon an ocean data set, we show that the map of upward heat flux at the ocean floor is consistent (within a factor of 2) with the ocean floor age‐dependent map of GHF. The observed buoyancy flux above the ocean floor is consistent with previous suggestions that the GHF acts to erode the abyssal stratification and thereby enhances the strength of the abyssal circulation. Idealized numerical simulations are performed using a zonally averaged single‐basin model which enables us to address the GHF impact as a function of the depth dependence of diapycnal diffusivity. We show that ignoring this vertical variation leads to an under‐prediction of the influence of the GHF on the abyssal circulation. Independent of the diffusivity profile, introduction of the GHF in the model leads to steepening of the Southern Ocean isopycnals and to strengthening of the eddy‐induced circulation and the Antarctic bottom water cell. The enhanced circulation ventilates the GHF derived heating to shallow depths, primarily in the Southern Ocean.</p> </abstract>