Global Ocean Cascades and a Direct Gyrescale-Mesoscale energy pathway induced by the atmosphere.
ORAL
Abstract
Our understanding of the ocean's spatial scales and their coupling has been derived mostly from Fourier analysis in small "representative" regions, typically a few hundred kilometers in size, that cannot capture the vast dynamic range at planetary scales. Using coarse-graining on a 1/12-degree reanalysis dataset, we probe a range of spatial scales spanning more than three orders of magnitude, including mesoscales and planetary scales, and quantify both the kinetic energy (KE) spectral density and the across-scale KE transfer. Since coarse-graining preserves the temporal signal, we are able to observe in the oceanic mesoscale, a steady propagation of energy to larger scales across the seasonal cycle, indicative of a scale-local energy cascade. This 'spectral advection' signal presents a characteristic lag time of ~27 days per octave, and is present in both the KE spectra and the KE transfer. Combined with a phase-lag between the KE spectra and KE transfer signals, this suggests that energy transferred across scale $\ell$ is primarily deposited at scales $\approx4\times\ell$. We also find that the highly energetic mesoscales have a direct transfer with gyrescales (> 1000km), which is induced by the atmospheric circulation cells (Hadley, Ferrel, Polar). This gyrescale-mesoscale exchange is new and absent from standard theories of gyre circulation.
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Publication: B. Storer, M. Buzzicotti, H. Khatri,, S. Griffies, H. Aluie, Science Advances, 9, eadi7420 (2023) https://doi.org/10.1126/sciadv.adi7420
Presenters
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Hussein Aluie
University of Rochester
Authors
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Benjamin A Storer
Department of Mechanical Engineering, University of Rochester
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Michele Buzzicotti
University of Rome Tor Vergata and INFN
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Hemant Khatri
University of Liverpool
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Stephen Griffies
Princeton/GFDL
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Hussein Aluie
University of Rochester