W2: Energy transfer through low mode internal waves

Principal investigators: Prof. Monika Rhein (MARUM/University of Bremen), Prof. Jin-Song von Storch (Max Planck Institute for Meteorology)

Objectives

Processes and observational techniques associated with the generation, propagation, and dissipation of near inertial waves and internal tides. Internal tides are induced by barotropic tides over topographic features (depicted by the bathymetry of a seamount). Wind generates inertial oscillations in the surface mixed layer that generate near inertial waves below. Both high and low modes are excited by wind and tides. Low mode waves propagate long distances, while higher modes have stronger shear that results in local dissipation and mixing. The pattern of vertical displacement of an internal M2 tide as inferred from satellite altimetry is shown at the bottom (data provided by B. Dushaw). Measurements of internal wave energy fluxes will be carried out by moored instruments or by repeatedly lowering the instruments from a ship over the duration of one or two tidal cycles.

Internal gravity waves in the ocean are generated by tides, wind, and interaction of currents with rough seafloor topography. Models predict a global energy supply for the internal wave field of about 0.7–1.3 TW by the conversion of barotropic tides at mid-ocean ridges and abrupt topographic features. Winds acting on the oceanic mixed layer contribute 0.3–1.5 TW and mesoscale flow over rough topography adds an additional amount of 0.2 TW. Globally, 1–2 TW are needed to maintain the observed stratification of the deep ocean by diapycnal mixing that results from the breaking of internal waves. Ocean circulation models show significant impact of the spatial distribution of internal wave dissipation and mixing on the ocean state, e.g. thermal structure, stratification, and meridional overturning circulation. Observations indicate that the local ratio of generation and dissipation of internal waves is often below unity and thus the energy available for mixing must be redistributed by internal tides and near-inertial waves at low vertical wavenumber that can propagate thousands of kilometers from their source regions. Eddy-permitting global ocean circulation models are able to quantify the different sources of energy input and can also simulate the propagation of the lowest internal wave modes. However, the variation of the internal wave energy flux along its paths by wave-wave interaction or refraction by mesoscale features as well as its ultimate fate by dissipation remains to by parameterized.

This project aims to quantify the generation and propagation of internal waves in the global ocean, study the pathways of radiated low mode internal waves including processes operating along the pathways, identify regions of sources and sinks, estimate the contribution to local dissipation and identify the involved processes.

For these purposes we will use

dedicated global high resolution (1/10° or higher) model runs, with idealised forcing mechanisms
observations of internal wave energy fluxes along paths where satellite altimetry shows beams of converging low mode internal waves
and a combination of the model simulations with the available observations

to produce the best estimate of the global distributions of sources and sinks needed for an energetically consistent model of the diapycnal diffusivity induced by internal waves breaking.

Barotropic to baroclinic tidal energy conversion in W m^−2 (color scale is logarithmic) for the semidiurnal M2 tide from the high-resolution ocean circulation model STORMTIDE (Müller, 2013). Arrows denote energy flux (taken from Alford, 2003) for low mode internal tides from historical mooring records.

Invited Guests

No guests available.

Reports

Research Stay in San Diego by Zoi Kourkouraidou (Feb 24)

Last February I had my first research visit. After participating at the "Ocean Sciences Meeting 2024" in New Orleans, I crossed the continent and landed in beautiful San Diego, California. I visited the MOD Lab at SCRIPPS Institute of Oceanography, a team of oceanographers, engineers and PhD students who work on multi scale ocean dynamics.

Most specifically, I visited Dr. Amy Waterhouse who arranged for a rich and very fruitful schedule of meetings with both senior and early career researchers both from SCRIPPS and also from the University of San Diego (UCSD). I had the chance to learn about their work, was given a nice tour through their lab and also attended some of their seminars and one PhD defence. At the end of the week I was given the opportunity to present my own work in the CASPO seminar, where I got many interesting questions and inputs for my research.

The week went by very fast unfortunately, but I'm still very grateful for having the chance to network with so many researchers, learn about their science and visit this legendary institute! On top of these, I will certainly not easily forget the beautiful walks along the La Jolla beach, the stunning sunsets and the unique experience of going surfing during lunch break!

I am thankful to Amy for hosting me and taking care of my schedule and of course to the CRC181 for the funding.

Investigating internal wave energy fluxes

In my current work, I also look into the impact of mesoscale motion on the energy flux in this dataset.
Jonas Löb, PhD W2

My name is Jonas and I am a PhD Student in the subproject W2 “Low mode waves” in the working group Oceanography at the University Bremen. In this project I calculate low mode internal wave energy fluxes from mooring measurements and compare the results with measurements from satellite altimetry and a 1/10° ocean model (STORMTIDE2). Energy flux is an important quantity for these models because its divergence identifies sources and sinks.

Internal gravity waves occur all over the stratified ocean and can be grouped in different categories varying on their generation mechanism. I focus mainly on internal tides in the semidiurnal frequency M₂ generated by the barotropic tides over rough topography. Internal tides are a response of the astronomical gravitational forces of the ocean via oscillations in the sea surface elevation with horizontal tidal currents through the entire water column. These waves in the stratified ocean take the form of standing vertical oscillations of horizontal currents, called modes. The “zeroth” (barotropic) mode of horizontal velocity corresponds to horizontal ocean currents that are uniform from top to bottom. The first depth dependent (baroclinic) mode is characterized by flow in one direction at the top and in the opposite direct at the bottom. Higher modes have a more complicated vertical structure and their phase speed decreases with increasing mode number. The vertical structure of a mode can be calculated by the stratification, and velocity profiles can be fitted onto a linear combination of these modes. Low mode motions contain appreciable energy but quickly propagate away laterally. To study these low mode internal waves, we deployed a mooring inside a tidal beam in the eastern North Atlantic, south of the Azores, where a seamount chain stands out as a generation site for internal tides. In our study region the energy flux correlates reasonably well in direction, coherent – uncoherent portioning and mode ratio between mooring and model time series and satellite data. With regard to the total energy flux, the model and satellite observations underestimate the flux compared to the in situ data.

In my current work, I also look into the impact of mesoscale motion on the energy flux in this dataset. A surface eddy was crossing the mooring, and in the process dampening the energy flux in the first two modes by about one third, while a passing subsurface eddy dampened the energy mainly in the second mode. These observations support the idea that eddy interactions transfer energy from low modes into higher modes that can lead to increased dissipation. An open question is how much of the energy converted from lower to higher modes result in local dissipation, which is a crucial information in creating energy consistent ocean-climate models.

Publications

Brüggemann, N., Losch, M., Scholz, P., Pollmann, F., Danilov, S., Gutjahr, O., Jungclaus, J., Koldunov, N., Korn, P., Olbers, D., Eden, C. (2024). Parameterized Internal Wave Mixing in Three Ocean General Circulation Models. Journal of Advances in Modeling Earth Systems, 16, e2023MS003768. doi: https://doi.org/10.1029/2023MS003768
Lüschow, V. & von Storch, J-S. (2024). Sensitivity of internal-tide generation to stratification and its implication for deep overturning circulations. J. Phys. Ocean. 54, 319-330, doi: https://doi.org/10.1175/JPO-D-23-0058.1.
von Storch, J-S., Brüggemann, N., Korn, P. et al. (2023). Open-ocean tides simulated by ICON-O, version icon-2.6.6. Geosci. Model Dev. 16(17), 5179-5196, doi: https://doi.org/10.5194/gmd-16-5179-2023.
Chouksey, M., Eden, C., Masur, G. & Oliver, M. (2023). A comparison of methods to balance geophysical flows. J. Fluid Mech. 971, A2, doi: https://doi.org/10.1017/jfm.2023.602.
Olbers, D., Pollmann, F., Patel, A. & Eden, C. (2023). A model of energy and spectral shape for the internal gravity wave field in the deep-sea – The parametric IDEMIX model. J. Phys.Oceanogr. 53(5), doi: https://doi.org/10.1175/JPO-D-22-0147.1.
von Storch, J.-S. & Lüschow, V. (2023). Wind power input to ocean near-inertial waves diagnosed from a 5-km global coupled atmosphere-ocean general circulation model. J. Geophys. Res. - Oceans 128(2), e2022JC019111, doi: https://doi.org/10.1029/2022JC019111.
Chouksey, M., Griesel, A., Eden, C. & Steinfeldt, R. (2022). Transit Time Distributions and Ventilation Pathways Using CFCs and Lagrangian Backtracking in the South Atlantic of an Eddying Ocean Model. J. Phys. Oceanogr. 52(7), 1531–1548, doi: https://doi.org/10.1175/JPO-D-21-0070.1.
Chouksey, A., Griesel, A., Chouksey, M. & Eden, C. (2022). Changes in global ocean circulation due to isopycnal diffusion. J. Phys. Oceanogr. 52(9), 2219-2235, doi: https://doi.org/10.1175/JPO-D-21-0205.1.
Chouksey, M., Eden, C. & Olbers, D. (2022). Gravity Wave Generation in Balanced Sheared Flow Revisited. J. Phys. Oceanogr. 52, 1351–1362, doi: https://doi.org/10.1175/JPO-D-21-0115.1.
Eden, C., Olbers, D. & Eriksen, T. (2021). A closure for lee wave drag on the large-scale ocean circulation. J. Phys. Oceanogr. 51(12), doi: https://doi.org/10.1175/JPO-D-20-0230.1.
Löb, J., Köhler, J., Walter, M., Mertens, C., & Rhein, M. (2021). Time Series of Near-Inertial Gravity Wave Energy Fluxes: The Effect of a Strong Wind Event. J. Geophys. Res. - Oceans 126, e2021JC01747, doi: https://doi.org/10.1029/2021JC017472.
Löb, J., Köhler, J., Mertens, C., Walter, M., Li, Z., von Storch, J.‐S., et al. (2020). Observations of the low‐mode internal tide and its interaction with mesoscale flow south of the Azores. J. Geophys. Res. - Oceans 125, e2019JC015879, doi: https://doi.org/10.1029/2019JC015879.
Li, Z. & von Storch, J.-S. (2020). M2 internal-tide generation in STORMTIDE2. J. Geophys. Res. - Oceans 125, e2019JC01545, doi: https://doi.org/10.1029/2019JC015453.
Voelker, G. S., Olbers, D., Walter, M., Mertens, C., & Myers, P. G. (2020). Estimates of Wind Power and Radiative Near-Inertial Internal Wave Flux. The Hybrid Slab Model and Its Application to the North Atlantic. Ocean Dynam. 70, 1357–1376, doi: https://doi.org/10.1007/s10236-020-01388-y.
Köhler, J., Walter, M., Mertens, C., Stiehler, J., Li, Z., Zhao, Z., von Storch, J.-S., & Rhein, M. (2019). Energy flux observations in an internal tide beam in the eastern North Atlantic. J. Geophys. Res.-Oceans., Vol. 124 (8), 5747-5764, https://doi.org/10.1029/2019JC015156.
Voelker, G. S., P. G. Myers, M. Walter and B. R. Sutherland (2019). Generation of Oceanic Internal Gravity Waves by a Cyclonic Surface Stress Disturbance. Dynam. Atmos. Oceans, doi: https://doi.org/10.1016/j.dynatmoce.2019.03.005.
Mertens, C., Köhler, J., Walter, M., von Storch, J. S., & Rhein, M. (2019). Observations and Models of Low-Mode Internal Waves in the Ocean. In Energy Transfers in Atmosphere and Ocean (pp. 127-143). Springer, Cham., doi: https://doi.org/10.1007/978-3-030-05704-6_4.