Please use this identifier to cite or link to this item:
Modeling deep equatorial circulation
|uhm_phd_9325058_r.pdf||Version for non-UH users. Copying/Printing is not permitted||4.25 MB||Adobe PDF||View/Open|
|uhm_phd_9325058_uh.pdf||Version for UH users||4.19 MB||Adobe PDF||View/Open|
|Title:||Modeling deep equatorial circulation|
|Abstract:||Observations show that there are significant zonal currents near the equator below the thermocline, the so called equatorial deep jets. The dynamics of these currents are unknown. In this study, the origin of the equatorial deep jets is explored through a series of numerical experiments. High resolution thermohaline spin up experiments were undertaken to investigate the thermohaline hypothesis of equatorial deep jets. It is found that the deep circulation strongly depends on the deep stratification. If this is unrealistically weak, an alternating jet structure and strong deep upwelling near the equator can be generated. This strong upwelling can result in an extra meridional overturning cell near the equator in the meridional mass transport streamfunction. The lack of stratification in the deep ocean is a generic deficiency of large scale circulation models which employ insulating bottom boundary conditions. The deep stratification can be improved greatly by using a Newtonian bottom boundary condition for temperature. The resulting streamfunction is more realistic and the deep equatorial overturning cell and alternating jets disappeared. It is the bottom boundary condition rather than the size of the vertical diffusion coefficient that is more important in determining the deep stratification and deep equatorial flow. Even though we cannot completely rule out the thermohaline forcing hypothesis of the equatorial deep jets (because thermohaline spinup experiments with very low explicit diffusion have not been carried out to investigate the dynamics of thermohaline circulation in a low diffusive regime), it is improbable that the deep jets are purely thermohaline in origin. High resolution, low diffusion wind-forced equatorial models were next run to investigate whether subthermocline mean equatorial currents can be generated via instabilities of the surface currents and wave-wave interactions. It is found that if eddy diffusion coefficients for momentum and heat are low enough, there are significant subthermocline time-mean currents. These currents are connected to low latitude western and eastern boundary subsurface currents. The eddy processes (Reynolds stress divergence) are found to be as important as the parameterized sub-grid processes (explicit diffusion).|
|Description:||Thesis (Ph. D.)--University of Hawaii at Manoa, 1993.|
Includes bibliographical references (leaves 152-157).
xix, 157 leaves, bound ill. 29 cm
|Rights:||All UHM dissertations and theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission from the copyright owner.|
|Appears in Collections:||Ph.D. - Oceanography|
Please contact firstname.lastname@example.org if you need this content in an alternative format.
Items in ScholarSpace are protected by copyright, with all rights reserved, unless otherwise indicated.