
NSF Org: |
OCE Division Of Ocean Sciences |
Recipient: |
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Initial Amendment Date: | July 12, 2017 |
Latest Amendment Date: | August 7, 2017 |
Award Number: | 1736595 |
Award Instrument: | Standard Grant |
Program Manager: |
Baris Uz
bmuz@nsf.gov (703)292-4557 OCE Division Of Ocean Sciences GEO Directorate for Geosciences |
Start Date: | October 1, 2017 |
End Date: | September 30, 2021 (Estimated) |
Total Intended Award Amount: | $258,254.00 |
Total Awarded Amount to Date: | $258,254.00 |
Funds Obligated to Date: |
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History of Investigator: |
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Recipient Sponsored Research Office: |
8622 DISCOVERY WAY # 116 LA JOLLA CA US 92093-1500 (858)534-1293 |
Sponsor Congressional District: |
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Primary Place of Performance: |
La Jolla CA US 92093-0210 |
Primary Place of
Performance Congressional District: |
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Unique Entity Identifier (UEI): |
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Parent UEI: |
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NSF Program(s): | PHYSICAL OCEANOGRAPHY |
Primary Program Source: |
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Program Reference Code(s): |
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Program Element Code(s): |
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Award Agency Code: | 4900 |
Fund Agency Code: | 4900 |
Assistance Listing Number(s): | 47.050 |
ABSTRACT
Ocean flows at relatively large scales, typically more than tens of miles, are mostly confined to horizontal plane due to the rotation of the Earth. At the smaller submesoscale, this constraint is much reduced, allowing more vigorous vertical motion, which plays a crucial role in mediating upper ocean heat content and air-sea exchange. Improving the representation of these processes in numerical models is therefore important for accurate forecasts of a wide range of directly societally relevant phenomena, from ENSO to tropical monsoons to the rate of Arctic sea ice melt. Due to their intrinsic short lateral scales (order of km) and fast time scales (order of inertial period or faster), submesoscale flows have been difficult to observe directly in the ocean. Numerical and analytical studies, on the other hand, have made substantial progress in describing the dynamics of idealized submesoscale flows. Criteria have been developed for the onset of different submesoscale instabilities. Parametrizations have been made to account for these instabilities in global ocean models where they are not resolved. Yet little of the knowledge gained from these studies has been confirmed by or compared with observations, which makes it difficult to move forward with confidence. This project will address this gap by combining development and application of a comprehensive linear stability model with analysis of several substantial oceanographic datasets already in hand. This project largely written by and will fund an early career scientist.
The model, developed by the early career scientist, is novel in that it is forced by observed profiles of density and velocity, unlike many idealized mean states that have been used in the past. Preliminary work demonstrates its capacity to reproduce a vast range of types of submesoscale instabilities, from mixed layer baroclinic instability to symmetric instability to Langmuir circulation, and everything in between. Unlike linear stability models before, it can smoothly transition from one instability class to another; i.e. it produces a broad spectrum of instabilities from a single mean flow state input. The model will be forced by and then compared with amassed datasets from several recent oceanographic expeditions. Two of the data-sets have shown strong evidence of submesoscale activity, both with anecdotal examples and systematic statistics. Model skill will be developed and tested using profiles from several of these examples. In turn, it is anticipated that the model results will help illuminate the nature of the dynamical instabilities present in the observations; because the model is initialized with real gradient profiles and allows a fully complex superposition of a wide range of instabilities, it is uniquely suited for detangling complex observations in a broadband ocean. Comparison of model predictions with available observations that span multiple ocean basins and multiple seasons will help develop understanding of broad patterns of submesoscale variability, the sorts of patterns that can be used to validate new global parametrization development.
PUBLICATIONS PRODUCED AS A RESULT OF THIS RESEARCH
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PROJECT OUTCOMES REPORT
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This Project Outcomes Report for the General Public is displayed verbatim as submitted by the Principal Investigator (PI) for this award. Any opinions, findings, and conclusions or recommendations expressed in this Report are those of the PI and do not necessarily reflect the views of the National Science Foundation; NSF has not approved or endorsed its content.
This award primarily supported the postdoctoral work of Dr. Sean Haney (shown below) Tragically, Dr. Haney passed away during the final reporting period. Here I?ll provide a brief summary of his work, which I am hopeful will have a significant impact on the field.
Historically, there have been several different sub-communities within physical oceanography. One subset has studied processes which have fast time scales and are often nonlinear. Those processes include internal gravity waves (like surface waves but propagating on density layers within the ocean), and turbulent mixing. Those processes often have smaller spatial scales and are not able to be directly represented in climate models but need to be parameterized in some way. And the on the other hand there is a community studying the large-scale circulation of the ocean, including big currents like the Gulf Stream and associated meanders and large-scale eddies (storms of the ocean). These motions are largely two-dimensional, in that they move different water masses horizontally in the ocean, but not vertically. Over the last decade or so there has been increasing interest in the edges of large-scale circulation patterns, fronts between different water masses, and their instabilities. Small and highly nonlinear instabilities on the edges of big features like the Gulf Stream break the normal balance, allowing vertical exchange of heat, nutrients and dissolved greenhouse gasses between the surface ocean and the deeper interior below.
Dr. Haney?s work has revolved around the intersection between these types of motions. He was particularly interested in the fact that at some point the space and time-scales of instabilities on the edge of larger currents are the same as the space and time-scales of internal gravity waves. The ocean does not know that we think of them as separate phenomena, and so it is somewhat inevitable that they will interact. He explored the nature and theoretical underpinnings of that interaction. He also found a remarkable example of that type of interaction in ocean data. He observed a situation where a shoaling internal wave actually transformed itself into a gravity current, driven by a density anomaly. The observation is both a remarkable confirmation of some of the theory, and fascinating to look at. Sean was a proponent of open access science, and his work is viewable to the public here (https://doi.org/10.1175/JPO-D-21-0062.1). Sean was a gifted scientist and a joy to work with; he will be missed.
Last Modified: 02/01/2022
Modified by: Jennifer A Mackinnon
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