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Surface gravity waves play a major role in the exchange of momentum, heat, energy, and gases between the ocean and the atmosphere. The interaction between currents and waves can lead to variations in the wave direction, frequency, and amplitude. In the present work, we use an ensemble of synthetic currents to force the wave model WAVEWATCH III and assess the relative impact of current divergence and vorticity in modifying several properties of the waves, including direction, period, directional spreading, and significant wave height Hs. We find that the spatial variability of Hs is highly sensitive to the nature of the underlying current and that refraction is the main mechanism leading to gradients of Hs. The results obtained using synthetic currents were used to interpret the response of surface waves to realistic currents by running an additional set of simulations using the llc4320 MITgcm output in the California Current region. Our findings suggest that wave parameters could be used to detect and characterize strong gradients in the velocity field, which is particularly relevant for the Surface Water and Ocean Topography (SWOT) satellite as well as several proposed satellite missions.

Author(s): Yu, Yao; Sandwell, David T; Gille, Sarah T; Boas, Ana Beatriz Villas | Abstract: SUMMARY The Ice, Cloud and land Elevation Satellite 2 (ICESat-2) laser altimetry mission, launched in September 2018, uses six parallel lidar tracks with very fine along-track resolution (15nm) to measure the topography of ice, land and ocean surfaces. Here we assess the ability of ICESat-2 ocean data to recover oceanographic signals ranging from surface gravity waves to the marine geoid. We focus on a region in the tropical Pacific and study photon height data in both the wavenumber and space domain. Results show that an ICESat-2 single track can recover the marine geoid at wavelengths g20nkm which is similar to the best radar altimeter data. The wavelength and propagation direction of surface gravity waves are sometimes well resolved by using a combination of the strong and weak beams, which are separated by 90nm. We find higher than expected power in the 3–20nkm wavelength band where geoid and ocean signals should be small. This artificial power is caused by the projection of 2-D surface waves with ∼300nm wavelengths into longer wavelengths (5–10nkm) because of the 1-D sampling along the narrow ICESat-2 profile. Thus ICESat-2 will not provide major improvements to the geoid recovery in most of the ocean.

Sea surface winds off the California coast are characterized by high wind events that occur in spring and summer. In June, a well-defined wind event region is formed off the five major capes, exten...

We gratefully acknowledge the research funding (grant number: OSR-2-16-RPP-3268.02 from KAUST (King Abdullah University of Science and Technology). We also appreciate the computational resources related to the supercomputer Shaheen II and the assistance provided by KAUST Supercomputer Laboratory. A.B.V.B. was funded by the SWOT program with NASA grants NNX16AH67G and 80NSSC20K1136. We wish to thank Fabrice Ardhuin for discussing the simulation results and the setup of the numerical simulations

Author(s): Clayson, Carol Anne; Centurioni, Luca; Cronin, Meghan F; Edson, James; Gille, Sarah; Muller-Karger, Frank; Parfitt, Rhys; Riihimaki, Laura D; Smith, Shawn R; Swart, Sebastiaan; Vandemark, Douglas; Boas, Ana Beatriz Villas; Zappa, Christopher J; Zhang, Dongxiao | Abstract: Abstract Air‐sea interactions are critical to large-scale weather and climate predictions because of the ocean's ability to absorb excess atmospheric heat and carbon and regulate exchanges of momentum, water vapor, and other greenhouse gases. These exchanges are controlled by molecular, turbulent, and wave-driven processes in the atmospheric and oceanic boundary layers. Improved understanding and representation of these processes in models are key for increasing Earth system prediction skill, particularly for subseasonal to decadal time scales. Our understanding and ability to model these processes within this coupled system is presently inadequate due in large part to a lack of data: contemporaneous long-term observations from the top of the marine atmospheric boundary layer (MABL) to the base of the oceanic mixing layer.We propose the concept of “Super Sites” to provide multi-year suites of measurements at specific locations to simultaneously characterize physical and biogeochemical processes within the coupled boundary layers at high spatial and temporal resolution. Measurements will be made from floating platforms, buoys, towers, and autonomous vehicles, utilizing both in-situ and remote sensors. The engineering challenges and level of coordination, integration, and interoperability required to develop these coupled ocean‐atmosphere Super Sites place them in an “Ocean Shot” class.

Surface waves are crucial for the dynamics of the upper ocean not only because they mediate exchanges of momentum, heat, energy, and gases between the ocean and the atmosphere, but also because they determine the sea state. The surface wave field in a given region is set by the combination of local and remote forcing. The present work characterizes the seasonal variability of the deep water surface wave field in the California Current region, as retrieved from over two decades of satellite altimetry data combined with wave buoys and wave model hindcast (WaveWatch III). In particular, the extent to which the local wind modulates the variability of the significant wave height, peak period, and peak direction is assessed. During spring/summer, regional-scale wind events of up to 10 m/s are the dominant forcing for waves off the California coast, leading to relatively short-period waves (8–10 s) that come predominantly from the north-northwest. The wave climatology throughout the California Current region shows average significant wave heights exceeding 2 m during most of the year, which may have implications for the planning and retrieval methods of the Surface Water and Ocean Topography (SWOT) satellite mission.

cited By 9; International audience; Ocean surface winds, currents, and waves play a crucial role in exchanges of momentum, energy, heat, freshwater, gases, and other tracers between the ocean, atmosphere, and ice. Despite surface waves being strongly coupled to the upper ocean circulation and the overlying atmosphere, efforts to improve ocean, atmospheric, and wave observations and models have evolved somewhat independently. From an observational point of view, community efforts to bridge this gap have led to proposals for satellite Doppler oceanography mission concepts, which could provide unprecedented measurements of absolute surface velocity and directional wave spectrum at global scales. This paper reviews the present state of observations of surface winds, currents, and waves, and it outlines observational gaps that limit our current understanding of coupled processes that happen at the air-sea-ice interface. A significant challenge for the coming decade of wind, current, and wave observations will come in combining and interpreting measurements from (a) wave-buoys and high-frequency radars in coastal regions, (b) surface drifters and wave-enabled drifters in the open-ocean, marginal ice zones, and wave-current interaction "hot-spots," and (c) simultaneous measurements of absolute surface currents, ocean surface wind vector, and directional wave spectrum from Doppler satellite sensors.

Rings are marine vortices with a scale of hundreds of kilometers that can last for months, whose associated transport and mixing play an important role in the ocean dynamics. Such features are traditionally treated as a geostrophic flow, but since the centrifugal acceleration is not negligible in the inner core, the cyclo-geostrophic balance is a better approximation for the rings. In the present work, we describe a novel objective technique to identify the ring center, which is used as the origin of a convenient framework to handle rings under the cyclo-geostrophic balance. Furthermore, we correct the velocity field by the translation to isolate the swirl movement, a procedure ignored by other methodologies. We show that the lack of such correction would lead to an error of 30km on the center definition of a ship surveyed North Brazil Current Ring with 160km of radius. Another distinct characteristic of our approach is the flexibility in the spatio-temporal structure of the data, because it allows for ungridded data, an important ability for in situ observations. That also enables the use of a hybrid dataset composed from different instruments. The error on the Monte Carlo experiments to identify the center of the propagating ring is less than 10km, and depends on the level of noise, sampling strategy, and strength of the ring, among other factors. This technique was fully implemented in PyRings, an open Python library with a collection of procedures to handle oceanic rings and mesoscale eddies in general. HighlightsIt is easier to handle the rings dynamics in a cylindrical coordinate system.The ring data is transformed to cylindrical coordinate using machine learning.A larger time span on the data is allowed due the translation speed correction.This formulation works with hybrid dataset composed from different instruments.This technique is available by the PyRings package, written in Python.

By collocating 10 years (1999-2009) of remotely sensed surface turbulent heat fluxes with satellite altimetry data, we investigate the impact of ocean mesoscale eddies on the latent and sensible heat fluxes in the South Atlantic ocean. Eddies were identified using the method proposed by Chaigneau et al. (2009), which is based on closed contours of sea level anomaly. Most of the identified eddies had a radius of ~70 km and amplitude of ~5 cm. On average, in the South Atlantic, eddies play a minor role on the ocean-atmosphere heat exchange. However, in strongly energetic regions such as the Brazil-Malvinas confluence or Agulhas Current retroflection regions, eddies can account up to 20-30% of the total variance of the surface turbulent heat fluxes with averaged anomalies of ±10-20 W/m2 for both heat flux components. Cyclonic (anticyclonic) eddies, associated with negative (positive) heat fluxes anomalies tend to cool (warm) the overlying atmosphere. A composite analysis of the turbulent heat fluxes anomalies within the eddies reveals a direct relationship between the eddy amplitude and the intensity of the latent and sensible fluxes anomalies, such that large-amplitude eddies have a stronger signature in the turbulent surface heat fluxes. Heat fluxes anomalies are also much stronger near the eddy centers and decay radially to reach minimum values outside the eddies. Uma combinação de 10 anos (1999-2009) de fluxos turbulentos de calor pela superfície, medidos a partir de satélites, e dados altimétricos de anomalia da altura da superfície do mar, foram o utilizados com objetivo de investigar o impacto de vórtices de meso-escala nos fluxos de calor sensível e latente na bacia do Atlântico Sul. Para a detecção dos vórtices foi aplicado o método proposto por Chaigneau et al. (2009), que baseia-se em contornos fechados de anomalia da altura da superfície do mar. A maior parte dos vórtices identificados possui raio de ~70 km e amplitude de ~5 cm. Em média, no Atlântico Sul, o impacto dos vórtices para as trocas de calor entre oceano e atmosfera é relativamente fraco. Entretanto, em regiões de alta variabilidade energética como na Confluência Brasil- Malvinas e na retroflecção da Corrente das Agulhas, vórtices de meso-escala podem contribuir com anomalias médias de até ±10-20 W/m2 nos fluxos turbulentos. Vórtices ciclônicos (anti-ciclônicos), associados com anomalias negativas (positivas) de fluxos de calor, tendem a esfriar (esquentar) a atmosfera adjacente. Mapas composite foram analisados para milhares de vórtices, mostrando um relação direta entre a magnitude das anomalias dos fluxos e a amplitude dos vórtices, de tal modo que vórtices de maior amplitude contribuem com maiores anomalias de calor latente e sensível. Além disso, os padrões espaciais dos composites médios revelam que as anomalias são significativamente maiores próximo ao centro dos vórtices e decaem radialmente até atingirem valores absolutos mínimos fora dos contornos dos vórtices.