3.1. Statistical Description of Mesoscale Eddies
Figure 1 presents a global characterization of mesoscale eddy activity. The figure shows the detection from each atlas accumulated on a
gridded map, with areas of eddy generation and disappearance clearly delineated. The latter were identified as the initial and final detection point of each eddy trajectory that was monitored for a minimum of 4 weeks. The highest concentrations of eddy activity are defined by a high density of eddy generations and disappearances, with a total exceeding
eddies per degree square. It is notable that in all datasets, areas where eddies frequently generate are also areas where eddies disappear from the altimetry maps. It is evident that the eastern boundary areas, including the major eastern upwelling boundary systems in the Canary and Benguela in the South Atlantic, as well as the western boundary near the Confluence Zone between the Malvinas and South Brazil currents, exhibit a higher number of eddy generations. Please refer to
Figure S1 of the Supplementary Material for a visual representation of the higher number of eddy disappearances in the western boundary systems.
Figure 2 shows frequency maps of eddy-eddy interactions (merging and splitting events) identified by TOEddies. It is important to note that the spatial distribution of merging and splitting events, as identified by TOEddies, also occurs in similar locations. This reinforces the necessity of considering eddy-eddy interactions for comprehensive understanding of the detected eddies’ dynamic evolution. Over the course of the observation period, approximately 3% of the detected eddies were found to be involved in merging and splitting events, with 52% of these classified as cyclonic eddies.
From the numerous mesoscale eddies identified across the global data sets over the various years of observation, we have chosen to focus on individual detections that are part of main eddy trajectories with lifetimes of at least 16 weeks. The TOEddies dynamical dataset detects over 25 million (25,117,786) eddy occurrences (lasting a minimum of 16 weeks) organized in 119,994 eddy trajectories globally. In terms of the same subset of tracked mesoscale eddies, TOEddies outperforms META3.2 and TIAN in terms of the number of total trajectories, with an increase of almost 2% and 18% (117,035 and 98,375). In comparison with the other datasets, GOMEAD reports a lower number of detected eddies (17,822).
Figure 3 compares the horizontal eddy characteristics of each Atlas. Histograms, of mesoscale eddy lifetimes, characteristic radii and velocities were plotted separately for cyclonic and anticyclonic eddies. However, when longer lifetimes are considered (more than 26 weeks), the predominance of anticyclonic over cyclonic eddies becomes apparent, as noted in Chelton
et al. [
10].
In the TOEddies and META3.2, the characteristic radii of anticyclonic eddies were estimated at km and km. These values of the equivalent average radius of the anticyclonic eddies in these atlases is 5% and 3% larger, respectively, in comparison to that of the cyclones. In TIAN dataset, anticyclonic eddies sizes are slightly larger, with an average radius of km while cyclones are 7% smaller in size. However, the relative size of of the eddies in the TIAN atlas remains larger than those identified in META3.2 and TOEddies. In general, the GOMEAD dataset identifies significantly larger structures (with an estimated average km). We note that in this atlas, eddy radii smaller than ≤ 30 km were not included to avoid small-scale features that are not accurately captured by altimetry.
To identify areas where these differences are noticeable, we present in
Figure 4 the geographical distribution of the radii of eddies. These maps were calculated by averaging the
for each daily detected mesoscale eddy that falls within bins of
. For a suitable comparison, zonal averages of the eddy radius are also computed in
Figure 4e. In terms of the spatial radius distribution, smaller eddies are detected near the poles while larger ones near the equator. This aligns with the first baroclinic Rossby radius, which varies with latitude [
10,
63]. However, the absolute values of the eddy radius vary considerably across the datasets. The mean zonal radii from the GOMEAD dataset are higher, estimated at approximately ~150 km in the equatorial bandwidth of 10
S to 10
N. In contrast, the TOEddies, META3.2 and TIAN datasets detect lower eddy radii of the order of 100-120 km. At latitudes lower than 40
S higher than 40
N, the TIAN dataset identifies larger structures of approximately 60 km, while the TOEddies and META3.2 estimates indicate smaller structures (~40 km).
In terms of intensity, the mean characteristic velocities in the TOEddies dataset reached almost cm/s, while eddies in META3.2 and TIAN indicated slightly higher and lower velocities, cm/s and cm/s respectively. It is worth noting that there are significant variations in the characteristics of the eddies, indicating that their sizes and intensities could differ significantly between observation periods. Furthermore, a comparison of all datasets reveals that cyclonic eddies display higher standard deviations in intensity than anticyclonic eddies.
3.2. Characterization of Main Eddy Pathways
Figure 5 depicts eddy trajectories from the TOEddies atlas, based on their estimated lifetimes. The cyclonic and anticyclonic trajectories are presented separately, with blue and red colors, respectively. To facilitate a comparative analysis, we have selected similar thresholds as those chosen in Chelton
et al. [
10] for the eddy lifetimes. This results in lifetimes that exceed 52, 78 and 104 weeks respectively. For instance, the selection of eddy trajectories that live longer than 78 weeks (more than 1.5 year) with TOEddies dataset (
Figure 5b) results in 2007 anticyclonic and 1339 cyclonic trajectories. In the North Atlantic, we find an equal eddy mixture of long-lived cyclones and anticyclones. However, in the Indian Ocean, we predominantly observe long-lived cyclones. These cyclones account for 40% of the total long-lived cyclones (for lifetimes ≥ 104 weeks) and are among the longest propagating eddies found in the TOEddies Atlas.
Figure 6 shows the same selection of eddy trajectories (with lifetimes more than 78 weeks) with the META3.2, TIAN, and GOMEAD atlases. While both the META3.2 and TIAN atlases follow a comparable number of persistent trajectories, their total is 53% and 41% lower, respectively, than that of TOEddies. For example, the META3.2 database includes 995 (773) anticyclonic (cyclonic) eddies with a lifetime exceeding 78 weeks, representing 56% (44%) of the total eddies. Similarly, the TIAN dataset contains 810 (564) anticyclonic (cyclonic) eddies, representing 59% (41%) of the total eddies. This discrepancy is primarily attributable to the lack of long-duration trajectories in the North and South Pacific. It is worth noting that the GOMEAD dataset identifies fewer trajectories than the other atlases. In fact, it contains 63 anticyclonic and 20 cyclonic eddies for this selection.
In alignment with Chelton
et al. [
10], all atlases indicate that the majority of long-lived oceanic eddies propagate in a westerly direction, influenced by the
-effect. Only a minority of eddies propagate eastward, particularly in regions dominated by strong eastward currents. This eastward propagation is most notably observed in the Southern Ocean, specifically within the intense Antarctic Circumpolar Current (ACC) [
10,
64,
65]. In addition, a distinct pattern of deflection has been observed, with anticyclonic eddies tending to drift northward and cyclonic eddies southward (see
Figure S2 of Supplementary Material). The proportion of eastward-propagating eddies is notably larger in the TIAN dataset. When lifetimes of less than 4 weeks are considered, the distribution of both westward and eastward eddies can reach as high as 50%, indicating an almost equal distribution. However, when eddies persist for at least 16 weeks, this ratio falls significantly to around 35%. TOEddies and (META3.2) contain 20,061 and (30,440) eastward eddies, accounting for only 20% (35%) of the total eddies in the datasets.
It is also worth noting that there are differences in the behaviour of long-distance propagating eddies between the eddy datasets.
Figure 7 illustrates the trajectories of eddies from each dataset that were tracked for over 26 weeks and have propagated over 1,100 km. The distance was calculated for each eddy trajectory as the centroid distance between their initial and final positions, measured in kilometers. Long-lived, far-propagating eddies are of considerable interest to many studies due to their significant role in trapping and transporting water masses, along with heat, carbon, and oxygen. This process, in turn, influences global climate, marine connectivity, and ecosystem functioning [
1,
7,
45,
66]. The reliability of such estimates hinges on the precision with which mesoscale eddy temporal evolution and their en route interactions can be characterized. For example, the long-propagating Agulhas Rings leave a visible surface signature in the South Atlantic, which is reflected in all datasets. However, there are slight differences in the overview of the main eddy pathways depicted in each atlas, with some cases showing significant discrepancies. Such examples are visible mostly in the Pacific Ocean, where TOEddies detects more long-propagating eddies in the North Pacific, while only a portion of them is found in the TIAN dataset and META3.2 dataset (~11% and 46% fewer long-propagating trajectories, respectively). Large variations can also be observed in the South Pacific and North Atlantic.
To investigate in greater detail the similarities between long-lived eddies, we have focused our investigation on eddies with lifetimes of at least 26 weeks. We have then specifically targeted only those eddies that exhibited a consistent spatiotemporal evolution across all datasets. Given that the TOEddies dataset tracks a greater number of long-lived and long-propagating eddies, it was selected as the reference atlas. We then assessed the degree of similarity between the trajectories from the various datasets and the reference one. Eddies were classified as "similar" if, during the same temporal range, the average distance between their barycenters did not exceed a specified threshold, that we defined as ≥ 0.5. Our analysis revealed that the proportion of common eddy trajectories between TOEddies and the various datasets was approximately 72% for META3.2, 60% for TIAN and only 25% for GOMEAD.
3.3. Characterization of Main Eddy Interactions
It is crucial for any dataset aiming to represent mesoscale variability to have the capability to accurately track the temporal evolution of mesoscale eddies. It should be noted, however, that these large-scale mesoscale eddies are not isolated in the turbulent oceanic fields. Both anticyclonic and cyclonic eddies may undergo complex interactions along their dynamical evolution and can experience multiple merging or splitting events during their propagation. Such events modify the primary eddy pathways and are purported to be associated with substantial water transfers. It is, therefore, essential that merging and splitting events of both eddy types be identified so that the evolution of eddies can be understood.
The ability of TOEddies to determine the occurrence of eddy merging and splitting events enables the construction of unique eddy networks associated with specific eddy origins. In accordance with the methodology detailed in Laxenaire
et al. [
1,
5,
45],
Figure 8 illustrates three eddy-network reconstructions as a case study. These are associated with the Agulhas Rings corridor, eddies originating from the North Pacific upwelling system, and eddies from the Australian western boundary. The trajectories in black, which originated from the area delineated by the dashed line, serve as the reference trajectories and are defined as order zero in the network (see [
1]). The order number is increased with each additional interaction required to trace a reference trajectory in either direction. Consequently, these networks comprise all eddy trajectories that have encountered at least one merging or splitting event during their lifetime and, depending on their order, have connections to eddies of specific origins. The reconstruction of eddy networks indicates that long-lived and long-propagating eddies frequently interact with each other and have the potential to transport water from various regions of generation further away. To investigate the discrepancies among the different eddy atlases in tracking throughout the lifespan of eddies, an exhaustive analysis of two distinct long-lived eddies has been conducted. The TOEddies algorithm incorporates the co-location of the eddies identified from the altimetry gridded field with available in-situ measurements, thereby providing a valuable resource for in-depth studies of tracked eddies. To gain deeper insight into the vertical characteristics of these eddies and how they evolve over time, we have identified individual eddy trajectories that were sufficiently sampled by Argo floats across the years of observation. In particular, we have selected one anticyclonic eddy (A0) originating from the Agulhas leakage and one cyclonic eddy (C0) originating from the Australian western boundary, which were present in all datasets (
Figure 9).
In
Figure 9a,c, we present the specific trajectory network reconstruction of A0, which includes all eddies that have merged with and split from A0 during the three years of its lifespan. Based on the TOEddies dataset, it can be concluded that A0 is the result of a splitting event that occurred in the Cape Basin on September 11, 2010 at (6.92
E, 32.88
S).
Figure 10a) shows that A0 originated from another anticyclone (A1) that was tracked back in the Agulhas retroflection as early as on November 19, 2009 (15.17
E, 37.40
S). During the period between October 2011 and January 2012, a number of complex interactions were observed in the Cape Basin, as illustrated in
Figure 10b–d. After March 2011, A0 was observed crossing the Walvis Ridge and entering the South Atlantic, continuing westward at a consistent pace over 169 weeks (more than three years), reaching 7 December 2013.
From October 2010 to September 2013, 20 Argo floats collected data of A0 at different radial distances from the core of the eddy.
Figure 9a illustrates the temporal evolution of the A0 characteristic radii as computed by TOEddies applied to the ADT maps. In addition, the estimated distances of the Argo floats from the eddy core (magenta points,
Figure 9a,b) are provided. The eddy defined by the
contour remains relatively constant, with a median value of 80 km and a standard deviation (STD), of 18.1 km. However, the outermost contour defining the eddy,
, shows important variations, ranging from 26 to 202 km and an STD of 34.3 km. Both META3.2 and TIAN identified the presence of eddy A0, as illustrated in
Figure 9i. There is a noticeable overlap in the description of the main eddy pathway across all datasets. However, the TIAN algorithm identified a section of the eddy before its interaction with anticyclone A1, whereas the META3.2 dataset incorporated a portion of eddy A2 into the main trajectory.
Figure 9e,g shows the temporal evolution of the anticyclone’s characteristic radii and velocity across the various datasets. The temporal evolution of the eddy radius demonstrates a high level of similarity across the datasets, with mean differences with TOEddies of less than 6 km in META3.2 and 8 km in TIAN. Furthermore, the eddy
shows a consistent decline over time, a trend evident in all datasets. We observe a systematic decrease (in average 0.05 m/s), in the mean eddy intensity, as measured by TIAN, which is likely attributable to the use of SLA fields. However, while the decay of surface properties in the eddy indicates a distinct dissipation process, only the TOEddies atlas provides direct access to this information by integrating available hydrographic properties from Argo floats.
Figure 12a presents the temporal evolution of the density anomaly of the eddy A0 from Argo floats trapped within its core from 24 October, 2010 to 08 June, 2013. Only profiles situated within the eddy outermost radius of the eddy from its center were selected (
Figure 9a). The integration of Argo vertical profiles with the eddy detection based on satellite altimetry suggests that A0 is not undergoing dissipation. Instead, the data suggests that the eddy is experiencing a progressive deepening of its vertical structure and a clear separation from the ocean surface. Dynamical topography results from the vertical integration of the thermohaline properties of the water column. A reduction in eddy intensity may be linked to alterations in the thermohaline properties of the upper water column through eddy cooling as observed by [
67] or eddy subsidence at depth (as in this case). The latter case was initially documented for another Agulhas ring in [
5,
45] showing that the eddy subducted to become an intensified subsurface eddy. Therefore, when the eddy signal disappears from altimetry maps, it is possible that it has not simply dissipated. Instead, it may indicate that the eddy has penetrated more deeply and become disconnected from the surface.
Meanwhile, the Cyclone C0 was initially identified by TOEddies on June 24, 2011, off the western coast of Australia (112.9
E, 27.57
S) and was subsequently tracked as it propagated southwestward into the Indian Ocean for a period exceeding four years. The reconstruction of the TOEddies network also revealed multiple instances of merging and splitting along this cyclonic eddy trajectory. A few months after its formation, on February 25, 2012, a merging event (
Figure 11b) was detected with a short-lived cyclone (less than a month). On January 9, 2013 (
Figure 9c), C0 merged with another cyclonic eddy that originated from the western border of Australia and propagated westward. By June 14, 2014, C0 had already drifted 2,226 km, while being sampled by 22 different Argo floats, providing 138 vertical profiles at varying radial distances from the center of the eddy (magenta dots in
Figure 9b). On February 7, 2016, the eddy reached 61.28
E, 37.58
S and merged with another cyclone, which continued its westward propagation till February 26, 2018, reaching 33.82
E, 33.93
S.
To facilitate comparison between datasets, we located Cyclone C0 in the META3.2, TIAN, and GOMEAD atlases. META3.2 dataset has identified three separate cyclones (instead of one) that appear to be following a similar westward trajectory, as illustrated in
Figure 9b. The second cyclone in the META3.2 dataset was identified just a few days after the last detection of the first cyclone in the same dataset. The TOEddies identified this interaction as a merging of two cyclones. Similarly, Cyclone C0 in the TIAN dataset was identified as two distinct cyclonic eddies with no prior connection between them. The TIAN atlas was unable to link the two trajectories due to a significant variation in eddy size during the period in question (25 August 2012). Furthermore, the eddy velocity was found to be slightly lower (0.12 m/s) in intensity compared to that of TOEddies. GOMEAD also classified these cyclones as two distinct eddies, though with shorter trajectories.
Figure 12 provides an illustration of the value of integrating satellite altimetry data with the eddy subsurface properties derived from the extensive Argo vertical profiles. This approach offers a more comprehensive understanding of the dynamics and evolution of eddies. The figure illustrates the presence of a pronounced inverted temperature anomaly signal in the upper layers for C0. Furthermore, the analyzed data indicate that the core of A0 is situated between 200 and 1,000 m, exhibiting consistent and markedly distinct properties that are largely independent of seasonal variations in the mixing layer. The presented evidence suggests that these eddies are subsurface intensified. These findings are consistent with those of previous studies that employed the TOEddies atlas to examine a range of Atlantic eddies [
5,
7,
45]. These examples demonstrate the necessity of this integrated approach to fully grasp the complex vertical and horizontal structure of mesoscale eddies, particularly when considering their role in large-scale oceanic exchanges. Future work will aim to explore these vertical structures in more detail to gain a deeper understanding of their dynamical behavior throughout their lifecycle.
Figure 12.
Temporal evolution of anticyclone A0 and cyclone C0 vertical structure as obtained by Argo floats trapped inside the eddy core () (shown as magenta points in panels a and b. Vertical profiles of temperature T () and temperature anomalies () are shown in panels c-f.
Figure 12.
Temporal evolution of anticyclone A0 and cyclone C0 vertical structure as obtained by Argo floats trapped inside the eddy core () (shown as magenta points in panels a and b. Vertical profiles of temperature T () and temperature anomalies () are shown in panels c-f.