Award Abstract # 2420209
Potential vorticity dynamics of the meridional overturning circulation

NSF Org: OCE
Division Of Ocean Sciences
Recipient: WOODS HOLE OCEANOGRAPHIC INSTITUTION
Initial Amendment Date: September 3, 2024
Latest Amendment Date: September 3, 2024
Award Number: 2420209
Award Instrument: Standard Grant
Program Manager: Sean Kennan
skennan@nsf.gov
 (703)292-7575
OCE
 Division Of Ocean Sciences
GEO
 Directorate for Geosciences
Start Date: September 1, 2024
End Date: August 31, 2027 (Estimated)
Total Intended Award Amount: $496,716.00
Total Awarded Amount to Date: $496,716.00
Funds Obligated to Date: FY 2024 = $496,716.00
History of Investigator:
  • Michael Spall (Principal Investigator)
    mspall@whoi.edu
Recipient Sponsored Research Office: Woods Hole Oceanographic Institution
266 WOODS HOLE RD
WOODS HOLE
MA  US  02543-1535
(508)289-3542
Sponsor Congressional District: 09
Primary Place of Performance: Woods Hole Oceanographic Institution
266 WOODS HOLE RD
WOODS HOLE
MA  US  02543-1535
Primary Place of Performance
Congressional District:
09
Unique Entity Identifier (UEI): GFKFBWG2TV98
Parent UEI:
NSF Program(s): PHYSICAL OCEANOGRAPHY
Primary Program Source: 01002425DB NSF RESEARCH & RELATED ACTIVIT
Program Reference Code(s):
Program Element Code(s): 161000
Award Agency Code: 4900
Fund Agency Code: 4900
Assistance Listing Number(s): 47.050

ABSTRACT

The meridional overturning circulation (MOC) is an important component of the general ocean circulation and the global climate system. The MOC is forced at high latitudes yet must navigate 1000s of kilometers of latitude to connect the source and sink regions. The dynamics that control the pathways, residence times, and meridional coherence of the MOC are not well understood. The primary intellectual merit of the proposed work is the development of a theoretical basis to better understand how water parcels of the MOC transit from low to high latitudes.

In this study the potential and relative vorticity budgets will be evaluated along the MOC pathways to identify the leading order physics and key regions of potential vorticity modification that occur as parcels transit from low to high latitudes. The relative vorticity analysis will reveal the regions and mechanisms that control the vertical transport, which is the MOC in depth space and is also important for the large-scale dynamics and exchanges between the interior and mixed layer. The approach will make use of a high resolution, idealized configuration of the mid-latitude wind- and buoyancy-forced circulation and the most recent ECCO state estimate. The idealized approach, for both the theoretical and numerical components, complements the global climate models more commonly used to study the MOC.

This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

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