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Seasonal variation of mesoscale eddy intensity in the global ocean
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Yongcan Zu1, 2, 3, Yue Fang1, 2, 3, *, Shuangwen Sun1, 2, 3, Libao Gao1, 2, 3, Yang Yang1, 2, 3, Guijun Guo1, 2, 3
Acta Oceanologica Sinica | 2024, 43(1) : 48 - 58
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Acta Oceanologica Sinica | 2024, 43(1): 48-58
Physical Oceanography, Marine Meteorology and Marine Physics
Seasonal variation of mesoscale eddy intensity in the global ocean
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Yongcan Zu1, 2, 3, Yue Fang1, 2, 3, *, Shuangwen Sun1, 2, 3, Libao Gao1, 2, 3, Yang Yang1, 2, 3, Guijun Guo1, 2, 3
Affiliations
  • 1 First Institute of Oceanography/Key Laboratory of Marine Science and Numerical Modeling, Ministry of Natural Resources, Qingdao 266061, China
  • 2 Laboratory for Regional Oceanography and Numerical Modeling, Laoshan Laboratory, Qingdao 266237, China
  • 3 Shandong Key Laboratory of Marine Science and Numerical Modeling, Qingdao 266061, China
Published: 2024-01-25 doi: 10.1007/s13131-023-2278-3
Outline
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Mesoscale eddies are a prominent oceanic phenomenon that plays an important role in oceanic mass transport and energy conversion. Characterizing by rotational speed, the eddy intensity is one of the most fundamental properties of an eddy. However, the seasonal spatiotemporal variation in eddy intensity has not been examined from a global ocean perspective. In this study, we unveil the seasonal spatiotemporal characteristics of eddy intensity in the global ocean by using the latest satellite-altimetry-derived eddy trajectory data set. The results suggest that the eddy intensity has a distinct seasonal variation, reaching a peak in spring while attaining a minimum in autumn in the Northern Hemisphere and the opposite in the Southern Hemisphere. The seasonal variation of eddy intensity is more intense in the tropical-subtropical transition zones within latitudinal bands between 15° and 30° in the western Pacific Ocean, the northwestern Atlantic Ocean, and the eastern Indian Ocean because baroclinic instability in these areas changes sharply. Further analysis found that the seasonal variation of baroclinic instability precedes the eddy intensity by a phase of 2–3 months due to the initial perturbations needing time to grow into mesoscale eddies.

seasonal variation  /  mesoscale eddy  /  intensity  /  baroclinic instability  /  global ocean
Yongcan Zu, Yue Fang, Shuangwen Sun, Libao Gao, Yang Yang, Guijun Guo. Seasonal variation of mesoscale eddy intensity in the global ocean[J]. Acta Oceanologica Sinica, 2024 , 43 (1) : 48 -58 . DOI: 10.1007/s13131-023-2278-3
Oceanic mesoscale eddies are coherent rotating vortices of water with radius scales in the order of 10–100 km and lifetimes of several days to months that are nearly omnipresent mesoscale phenomena in the global ocean (Chelton et al., 2011b; Faghmous et al., 2015). Most mesoscale eddies propagate westward, and their propagation distances can reach thousands of kilometers (Chelton et al., 2011b). Mesoscale eddies can induce strong thermohaline anomalies and vertically extend up to a depth of thousands of meters (Chu et al., 2014; Sun et al., 2017; Zu et al., 2019). These characteristics of mesoscale eddies make them play a significant role in transporting oceanic mass (Zhang et al., 2014), heat and salt (Chen et al., 2012; Dong et al., 2014; Yang et al., 2015), pollutants (Chen et al., 2021), nutrient and marine phytoplankton (Chelton et al., 2011a; Frenger et al., 2018; Zhou et al., 2023), and regulating local atmospheric systems (Frenger et al., 2013). Influenced by the seasonality of the upper ocean, eddy properties not only have seasonal variation (Shum et al., 1990; Andersson et al., 2011), but some tracers (e.g., chlorophyll) trapped by eddies also change with seasonality (Gaube et al., 2014). Compared with the eddy trapping component, the eddy stirring component is distinctly larger in most areas (Sun et al., 2019). As one of the most fundamental properties of an eddy, the eddy intensity has a significant effect both on the eddy trapping component and the eddy stirring component of eddy-induced material transport (Gaube et al., 2014; Zu et al., 2019). Therefore, clarifying the seasonal feature of eddy intensity is essential to evaluate the impact of eddies on air-sea interactions and marine ecosystems.
Using satellite altimeter products and eddy detection algorithms, previous studies have analyzed eddy properties (such as size, lifetime, number, amplitude) in the regional and global oceans. On a regional scale, many studies have focused on the seasonal variation of eddy generation numbers in different areas of the global ocean, including the Pacific Ocean (Chaigneau et al., 2009; Kurczyn et al., 2012; Liu et al., 2012), the Atlantic Ocean (Chaigneau et al., 2008, 2009; Schütte et al., 2016), the Indian Ocean (Halo et al., 2014), and the Southern Ocean (Frenger et al., 2015). These studies show that the seasonal characteristics of generated eddies are diverse within corresponding regional oceans, which indicates that the size and location of the study regions greatly disturb the results of statistical analysis for eddy properties. Aguedjou et al. (2019) also pointed out that eddy amplitude has a strong seasonal cycle in the North Brazil Current retroflection, while it does not show significant variability in the North Equatorial Countercurrent area because of the different mechanisms of eddy generation in these two adjacent regions. In the Leeuwin Current system, more and stronger eddies tend to be generated in austral winter, while in the South Indian Countercurrent system, eddy properties generally reach their peaks in austral spring (Zhang et al., 2020). Zu et al. (2022) reported that the eddy amplitude in an area to the southwest coast of Java Island has prominent seasonality—eddies in this area are relatively weak during the first half of the year but tend to enhance in August and peak in October. They deduced that the seasonality of eddy amplitude is due to eddy development under the conditions of seasonal energy supply mainly from baroclinic instability. In some smaller regions, the seasonal variations of eddy amplitude are more complex. For instance, in the Sulu Sea, there are more cyclonic eddies with a larger amplitude during boreal winter, while there are more anticyclonic eddies with a larger amplitude during boreal summer (He et al., 2017). In offshore regions, the mechanisms responsible for eddy generation may be multiple and more complex, e.g., the interaction of large-scale currents with bottom topography, coastline geometry or islands, local baroclinic instability, and instability of coastal currents (Chaigneau et al., 2009; He et al., 2017). On a global scale, Martínez-Moreno et al. (2022) pointed out that a strong seasonal cycle is observed in the spatially coherent eddy field based on hemispherical averages, in which the eddy amplitude peaking in September for the Northern Hemisphere and January in the Southern Hemisphere. They related the seasonal variation of eddies to the wind forcing at time lags of 3−6 months and further highlighted that the inverse energy cascade is important for the observed seasonal cycle of coherent eddy properties. However, the spatial pattern of seasonal variation is not clarified in their work. From the above findings, it can be inferred that the seasonal spatiotemporal variations in eddies may be non-uniform in the global oceans. Therefore, it is necessary to simultaneously examine the spatial pattern and temporal pattern of seasonal variation in eddies.
There are multiple variables representing the intensity of mesoscale eddies, such as eddy amplitude (the absolute difference between the average sea surface height (SSH) at the eddy boundary and the extreme value of SSH in the eddy interior (Chelton et al., 2011b), eddy rotational speed and eddy kinetic energy (EKE). Generally, eddy amplitude dominates the rotational speed of the eddy. As the rotational speed increases, the eddy nonlinearity is easier to get stronger. Here, the eddy nonlinearity parameter refers to the ratio (u/c) between the maximum rotational speed of eddies (u) and their propagation speed (c) (Chelton et al., 2011b). A u/c >1 implies that the eddies are nonlinear and thus can trap materials in their core (Chelton et al., 2011b; Kurian et al., 2011). Figure 1 displays the climatological field of u and propagation speeds c of eddies in every 2°×2° grid, which shows that most eddies are nonlinear (u/c >1). No matter eddy rotational speed or eddy amplitude, they can be tracked in the eddy lifetime and the energy represent by them is coherent, while the EKE is discrete. Meanwhile, considering the direct effect of rotational speed on the nonlinearity of an eddy, we select rotational speed, a more intuitive term “intensity”, to represent eddy intensity in this study. Although eddy intensity is crucial to evaluating the transport of substances induced by eddies, its seasonal spatiotemporal characteristics on a global scale are still poorly understood. This study will analyze the spatiotemporal characteristics of eddy intensity at a seasonal scale from a global ocean perspective. The paper is organized as follows. Section 2 introduces the tracked eddy data set and relevant oceanic data. The results of seasonal variations in eddy intensity are presented in Section 3 and its main mechanism is discussed in Section 4. The paper is concluded with a summary in Section 5.
The delayed time mesoscale eddy trajectory atlas data set 3.2 (META 3.2) is distributed by Archiving, Validation, and Interpretation of Satellite Oceanographic (AVISO). The META 3.2 based on the all-sat merged absolute dynamic topography (ADT) fields is the latest version of the data set, which is generated and quality-controlled following the methodology developed by Mason et al. (2014) and further described in Pegliasco et al. (2022). The data set contains the positions of tracked eddies (eddy centers) as well as their properties (radius, amplitude, and rotational speed). The latter is identical to the “eddy intensity” analyzed in this study. The eddy data set spans the period from January 1993 to February 2022, covering the global ocean between 82.5°S to 82.5°N. In this study, the eddies shorter than 4 weeks and with amplitudes smaller than 1 cm are removed to exclude noise signals. The rotational speed is defined as the maximum of the average geostrophic speeds around all of the closed SSH contours inside the eddy (Chelton et al., 2011b). Besides, the daily all-satellite merged absolute geostrophic current with horizontal resolution (1/4)° × (1/4)° published by Copernicus Marine Service is also utilized.
The global ocean potential temperature and salinity (T-S) profiles are from the EN4.2.2 version of the Met Office Hadley Centre, mainly merging WOD09 and Argo float profiling data. Based on observational T-S profiles, the EN4.2.2 objective analysis monthly data set describes the ocean hydrographic conditions on a 1° spatial grid, with a vertical resolution of approximately 10−11 m from the surface to 110 m, and continues to 5350 m with decreasing vertical resolution (Good et al., 2013).
First, we divide the global ocean into 2° × 2° regular grids and then count all instantaneous eddies within the corresponding grids every month. The instantaneous eddies refer to the eddies detected from the ADT snapshot for a certain moment. The monthly eddy intensity data can be obtained by calculating the mean values of the rotational speeds of all instantaneous eddies over every grid in the calendar month from January 1993 to December 2021. To more efficiently ascertain the temporal and spatial variations in eddy intensity globally, we applied an empirical orthogonal function (EOF) analysis approach to eddy intensity anomalies. The anomalies were computed by removing the climatology value which was averaged from the whole time series for each grid. To lessen the spatial discretization in grid points, spatial smoothing with 3 grid lengths was applied in the eddy intensity fields before operating the EOF. This method can effectively eliminate discrete noise signals and extract spatial change trends. The smoothing method is also necessary when considering the very low explained variance of the EOF for the raw data (figure not shown). The spatial pattern and time pattern are not sensitive to a changing grid length. Moreover, to filter out the interference of intraseasonal signals and interannual and interdecadal variations, a 3−24 months bandpass filter was also applied to the eddy intensity fields. In this study, we define spring as April to June (AMJ) and autumn as October to December (OND) in the Northern Hemisphere and vice versa in the Southern Hemisphere.
We use the Eady growth rate (EGR) to indicate baroclinic instability in the ocean (Eady, 1949; Smith, 2007), which is quantified as
$ \mathrm{E}\mathrm{G}\mathrm{R}=f\sqrt{\frac{1}{H}{\int }_{-H}^{0}\frac{{\mathrm{d}}z}{{R}_{i}\left(z\right)}}, $
$ {R}_{i}=\frac{{N}^{2}}{{\left|\partial U/\partial z\right|}^{2}}, $
where f is the Coriolis parameter, N is the buoyancy frequency (or Brunt-Väisälä frequency) calculated by using the Thermodynamic Equation of SeaWater 2010 (TEOS-10), $ {{R}}_{{i}} $ is the Richardson number and H is the water depth. $ \partial {U}/\partial {z} $ is the vertical shear of the horizontal velocity, using the thermal wind balance from
$ \left|\frac{\partial U}{\partial z}\right|=\frac{g}{{\rho }_{0}f}\sqrt{{\left(\frac{\partial \rho }{\partial x}\right)}^{2}+{\left(\frac{\partial \rho }{\partial y}\right)}^{2},} $
where $ {\rho } $ is the density of seawater, $ {{\rho }}_{0} $ is the reference density of seawater, and g is the gravitational acceleration. In the open oceans, the upper 200 m is the depth where remarkable seasonal variations in the ocean are concentrated (Zhai et al., 2008; Qiu and Chen, 2013). Therefore, we will focus on the depth-averaged values of EGR in the upper 200 m.
The barotropic conversion rate (BTR) is used to analyze the barotropic instability, which is defined as (Böning and Budich, 1992; Zhang et al., 2016)
$ \mathrm{BTR}=-\left(\overline{{u}'{u}'}\frac{\partial \overline{u}}{\partial x}+\overline{{u}'{v}'}\left(\frac{\partial \overline{v}}{\partial x}+\frac{\partial \overline{u}}{\partial y}\right)+\overline{{v}'{v}'}\frac{\partial \overline{v}}{\partial y}\right). $
BTR is the conversion rate between mean kinetic energy (MKE) and EKE. Positive BTR implies part of the MKE of the mean flow is transferred to the EKE due to the barotropic instability. We use the absolute geostrophic velocity published by Copernicus Marine Service to represent currents in the upper layers. The transient components of velocity and density (e.g., $ {u}^{\prime} $) are defined as variability of periods shorter than 120 d, and the residual low-frequency variations with periods larger than 120 d (e.g., $\bar{u} $) are treated as the basic state.
When conducting linear Pearson’s correlation analysis of two-time series (x 1 and x 2), the effective degrees of freedom (DOF) are estimated following Bretherton et al. (1999):
$ \mathrm{D}\mathrm{O}\mathrm{F}={N}_{s}\frac{1-{r}_{1}{r}_{2}}{1+{r}_{1}{r}_{2}} , $
where N s is the sample number, r 1 and r 2 are the autocorrelation coefficients of x 1 and x 2 at lag one. DOF is the number of ways or dimensions that an independent value can move without violating constraints. All data are detrended before correlation coefficients are calculated.
To compare with the spatial patterns of seasonal variation, the climatological distributions of eddy intensity are first examined, which vary greatly across the globe (Fig. 1a). The regions with high values are primarily distributed in the strong current areas, such as the areas in the Kuroshio extension, the Gulf Stream, the Agulhas Stream, and the Somali Stream, which is consistent with the pattern of surface EKE in the work of Martínez-Moreno et al. (2022). In the subtropical regions, the zonal distribution of eddy intensity is different. At low latitudes, however, eddy intensity is also relatively strong, which is different from the distribution of eddy amplitude (Fig. S1). This may be due to the common effect of the small Coriolis force and the strong equatorial currents in the equatorial regions.
To extract the seasonal spatiotemporal characteristics, the EOF method is applied to the monthly anomaly of eddy intensity. The spatial and temporal patterns of the first EOF mode (EOF1) of eddy intensity anomaly are displayed in Figs 2a and b, respectively. One can see that the eddy intensity shows a distinct seasonal variation (Fig. 2b). It reaches a peak in boreal spring while attaining a minimum in boreal autumn, which can be intuitively revealed by the mean annual cycles of the time pattern in Fig. 2c. Spatially, the conspicuous areas are primarily located in the tropical-subtropical transition zones within latitudinal bands between 15° and 30° in the main open oceans, except for 20° to 35° in the southern Atlantic Ocean (Fig. 2a), which is different from the regions of strong climatological eddy intensity displayed by Fig. 1a. An important feature is that the eddy intensity shows the most intense seasonal variations in the tropical-subtropical transition zones of the western Pacific Ocean, the northwestern Atlantic Ocean, and the eastern Indian Ocean, which are indicated with thick solid rectangular boxes in Fig. 2a.
It is also noted that the spatial pattern in EOF1 is nonhomogenous in zonal distributions, which is in accord with those of climatological eddy intensity. In some regions of a half hemisphere, the amplitudes of seasonal variations are opposite or very slight. To compare with the spatial differences of seasonal variations, we selected four regions with opposite or slight seasonality (shown by the thin dotted rectangular boxes in Fig. 2a) and calculated their regional mean values of eddy intensity (Fig. S2). Their seasonal variations are consistent with the change of magnitude in the corresponding region in the spatial pattern in Fig. 2a. For instance, the eddies with strong intensity in the western Arabian Sea have a remarkable seasonal variation, reaching a peak in the latter half of the year (Fig. S2a). In this region, the positive increment can also be inferred from the large amplitude with a negative signal in the spatial pattern (Fig. 2a) multiplied by negative values in the time pattern in the latter half of the year (Fig. 2c). From the spatial pattern, it can be seen that seasonal spatial variations in eddies are non-uniform in the one-half hemisphere. Therefore, for the regions where eddies change strongly in opposite directions, their seasonal characteristics derived from regional averages are varied.
The spatial pattern of EOF1 is consistent with the maximum difference distribution (Fig. S3) of eddy intensity between spring and autumn, verifying the results of the EOF method for eddy intensity anomaly representing its seasonal spatiotemporal variations. Multiplying the spatial pattern and temporal pattern of EOF1 can obtain the monthly change in eddy intensity. This monthly change is smaller than the corresponding values calculated from raw data due to the smooth and filter methods applied in Fig. 2. From the raw data (Fig. S1), we can conclude that the regionally averaged eddy intensity in every spring is approximately 4.22 cm/s stronger than that in every autumn in the latitudinal bands between 15° and 30° in the northwestern Pacific Ocean (120°E−170°W). In the same latitudinal band of the western Indian Ocean (70°E−115°E), this quantity is approximately −4.59 cm/s. The maximum intensity in the seasonal cycle is approximately 1.3 times larger than the minimum counterpart in these two regions. The seasonal difference in eddy intensity represents the change in the energy source for eddy generation and development (through energy transfer) in the background.
Considering the effect of eddy polarity on the seasonality, we have calculated the climatological intensity of anticyclonic eddies (AEs) and cyclonic eddies (CEs), and their seasonal differences (Fig. 3). First of all, their spatial patterns of the climatological field are basically the same in the global scale (Figs 3a and b). In some regional areas, such as the Southeast of the North Pacific Ocean, the climatological intensity of AEs is stronger than that of CEs. There are also areas where CEs are greater than AEs, such as the Bay of Bengal and the western Arabian Sea. For the seasonal variations of AEs and CEs, it can be seen that the spatial patterns of both are also basically the same on the global scale (Figs 3c and d), especially in the areas that this study focuses on (boxes in Fig. 2a). Differences exist in some regions, such as the Southeast of North Pacific Ocean. Although there are some differences in some regional areas, it does not affect the main conclusion of this section.
In the open oceans, eddy generation is mainly caused by baroclinic instability, which further affects eddy development (Robinson and McWilliams, 1974; Stammer, 1998; Smith, 2007). To investigate the impact of baroclinic instability on eddy intensity at the seasonal scale, EOF analysis on the EGR of upper ocean layers averaged from the surface to 200 m depth is conducted, and its first mode is displayed in Fig. 4. The spatial pattern of EOF1 of EGR (Fig. 4a) is highly consistent with that of eddy intensity. The temporal pattern of EOF1 in Fig. 4b indicates that EGR has obvious seasonal variation, consistent with previous studies (Qiu, 1999; Zhai et al., 2008). Different from the seasonal variation of eddy intensity, however, EGR reaches a peak in boreal winter while attaining a minimum in boreal summer (Fig. 4c). The spatial pattern of EOF1 is also verified by the maximum difference distribution (Fig. S4) of EGR between winter and summer.
After filtering, EOF1 of the original data mainly represents the seasonal signals. Compared to other modes, EOF1s of eddy intensity and EGR are both significant at the 95% confidence level tested by the Monte Carlo method (Livezey and Chen, 1983). In addition, when EOF is applied to a regional field, the variance contribution rate of EOF1 is significantly increased, and the spatiotemporal characteristics of the modes are unchanged (figures not shown). This indicates that EOF applied on a global scale does not lose the seasonal signals of the main mode.
To further verify the results of EOF and analyze the relationship between eddy intensity and EGR, the original time series averaged from four regions (Fig. 2a) with strong seasonality in the northwestern Pacific Ocean, the northwestern Atlantic Ocean, the eastern Indian Ocean, and the southwestern Pacific Ocean are selected. The monthly time series (Fig. S5) of eddy intensity and EGR reveal obvious seasonal cycles and a lead-lag relationship between eddy intensity and EGR. The mean annual cycles in Fig. 5 further distinctly display the prominent seasonal variations of eddy intensity and EGR. The peaks of eddy intensity and EGR occur in the spring and winter in the Northern Hemisphere, respectively. For the maximum values of eddy intensity and EGR in the Southern Hemisphere, the corresponding seasons turn to autumn and summer, respectively. The seasonal cycle amplitude (the difference between the maximum and minimum of 12 monthly averages of the mean annual cycle) reaches 5.2 cm/s, 2.4 cm/s, 5.0 cm/s, and 4.2 cm/s for eddy intensity in the northwestern Pacific Ocean, the northwestern Atlantic Ocean, the eastern Indian Ocean, and the Southwestern Pacific Ocean, representing ~23%, ~14%, ~23%, and ~25% of the mean values, respectively. For EGR, the seasonal cycle amplitude reaches 0.09 d−1, 0.06 d−1, 0.09 d−1, and 0.08 d−1 in these four regions, representing ~78%, ~59%, ~56%, and ~67% of the mean values, respectively. The difference in the percentage between eddy intensity and EGR implies that the ratios of the energy converted to eddy through EGR are different between seasons in the annual cycle. Lagged cross-correlation analysis calculated from the monthly time series shown in Fig. S5 indicates that the seasonal variation of eddy intensity lags behind that of EGR in phase by 2−3 months (Fig. 6). Specifically, in the northwestern Pacific Ocean, the northwestern Atlantic Ocean, and the southwestern Pacific Ocean, the correlation coefficients between eddy intensity and EGR reach the largest values which are 0.77, 0.68, and 0.84, respectively, when EGR takes lead by 3 months. In the eastern Indian Ocean, the maximum correlation coefficient (0.79) is achieved when the lead time turns to 2 months. A two-tailed Student’s t-test estimated from the effective DOF (62, 85, 65, and 61 in the North Pacific Ocean, the North Atlantic Ocean, the South Indian Ocean and the South Pacific Ocean) calculated from the time series as described in the method section, suggests that all of the correlations are significant at the 95% confidence level.
Barotropic instability is also an important mechanism for mesoscale eddy generation (Zu et al., 2022). To check the role of barotropic instability in the seasonal variation of eddy intensity, we calculated the BTR by using absolute geostrophic velocity. Figure 7 shows the seasonal difference of BTR and its smoothed field. It can be seen that BTR changes sharply in strong currents regions (such as the Kuroshio extension, the Gulf Stream region, the western Arabian Sea, the Antarctic Circumpolar Current areas in the Southern Ocean), and some offshore areas. However, in the regions with strong seasonal variation of eddy intensity, the seasonal changes of BTR are not significant, which is different from that in baroclinic instability (Fig. 3 or Fig. S4). This indicates that barotropic instability plays a less important role in seasonal variation of eddy intensity than baroclinic instability on a global scale.
Baroclinic instability develops in the flow where both rotation and stratification are important, as they are at the oceanic mesoscale and act to convert the mean available potential energy to EKE (Smith, 2007). At the seasonal scale, the EKE maximum lags behind the instability peak due to the approximately 2 months required for the initial perturbations of baroclinic instability to grow into finite amplitude eddies under geostrophic turbulence (Qiu et al., 2014; Chang and Oey, 2014). This is also the reason why the eddy intensity needs 2−3 months to reach the maximum after the instability peak. N2 represents the vertical gradient of water density, while vertical shear represents the horizontal gradient of water density derived from the thermal wind relation. Both of them together control the three-dimensional motions of water particles and then affect changes in baroclinic instability. The stratification has a vertical damping effect, and its seasonality in the upper layer affects the intensity of the surface signal of eddies (Bashmachnikov and Carton, 2012; Bashmachnikov et al., 2014). Qiu (1999) reported that the seasonal variation of baroclinic instability is subject to background stratification, which is strongly influenced by local heating/cooling in the North Pacific Subtropical region. For mesoscale eddies, regardless of cyclonic or anticyclonic type, their dynamic structures are the same in the open oceans. The most critical part is the horizontal geostrophic flow, which induces the vertical movement of water in the eddy center under the action of divergence or convergence. The vertical movement of water is the necessary condition for eddy generation, i.e., eddies are not easy to generate or develop when their vertical motions are suppressed. Meanwhile, the vertical shear of currents provides the energy source for the baroclinic instability to persist throughout the year (Stammer, 1997; Qiu, 1999; Qiu et al., 2014) and tends to force the generation of eddies (Zhang et al., 2020).
The spatial differences in eddy intensity are mainly caused by the change in EGR, which may be attributed to the meridional gradients of the upper oceanic stratification and the zonal gradients of vertical shear. In the meridional direction, the uneven distribution of heat caused by the solar shortwave radiation leads to the meridional gradients of the upper oceanic stratification, while the zonal gradients of vertical shear are due to the current fields with different intensity between eastern and western basins in the zonal direction. Although stratification and vertical shear together affect the generation and development of eddies, their contributions to the seasonal variation of baroclinic instability on the global scale still need to be further analyzed with high-resolution models in future research.
In addition, different from the seasonal variations, the trends of seasonal eddy intensity increase significantly in the strong currents regions (such as Kuroshio extension, Gulf Stream region, and Southern Ocean (Antarctic Circumpolar Current areas)) in the last three decades (Fig. S6), which may relate to the acceleration of upper ocean currents under global warming (Hu et al., 2020; Peng et al., 2022; Shi et al., 2023).
Using the latest satellite-altimetry-derived eddy trajectory data set, we documented the seasonal spatiotemporal variations of mesoscale eddy intensity in the global ocean. The results show that it has remarkable seasonal variations, reaching a peak in spring while attaining a minimum in autumn in the Northern Hemisphere and the opposite in the Southern Hemisphere. The conspicuous areas are primarily located in the tropical-subtropical transition zones within latitudinal bands between 15° and 30° in the main open oceans, except for 20°S to 35°S in the Southern Atlantic Ocean. In the tropical-subtropical transition zones of the western Pacific Ocean, the northwestern Atlantic Ocean, and the eastern Indian Ocean, the eddy intensity shows the strongest seasonal variations.
The seasonality in EGR is mainly responsible for the seasonal variations of eddy intensity. The spatial pattern of seasonal variation in EGR is highly consistent with that in eddy intensity. However, there is a lead-lag relationship between the temporal series of both. In the western Pacific Ocean and the northwestern Atlantic Ocean, the seasonal variation of eddy intensity lags behind that of EGR in phase by 3 months, while it turns to 2 months in the eastern Indian Ocean. The delay of the eddy intensity maximum in spring behind the instability peak in winter is due to the time (2−3 months) required for the initial perturbations of baroclinic instability to grow into finite amplitude eddies.
The altimetric Mesoscale Eddy Trajectory Atlas product (META3.2 DT allsat, doi: 10.24400/527896/a01-2022.005.220209) was produced by SSALTO/DUACS and distributed by AVISO+ with support from CNES, in collaboration with IMEDEA. The detailed link to the data information and access is as follows: https://www.aviso.altimetry.fr/en/data/products/value-added-products/global-mesoscale-eddy-trajectory-product/meta3-2-dt.html. The EN4.2.2 dataset is from Met Office Hadley Centre, which is open-access on the website: https://www.metoffice.gov.uk/hadobs/en4/download-en4-2-2.html. The absolute geostrophic current (doi: 10.48670/moi-00148) is published by Copernicus Marine Service and the access address is https://data.marine.copernicus.eu/product/SEALEV EL_GLO_PHY_L4_MY_008_047/services.
  • The National Key R&D Program of China under contract No. 2022YFC2807604; the Basic Scientific Fund for National Public Research Institutes of China under contract Nos 2022S02, 2022Q03 and 2018S02; the Marine S&T Fund of Shandong Province for Pilot National Laboratory for Marine Science and Technology (Qingdao) under contract No. 2018SDKJ0105-3; the National Natural Science Foundation of China under contract Nos 41876030, 41976021, 41876231, 4190060432 and 41706220; the program Impact and Response of Antarctic Seas to Climate Change under contract No. IRASCC 01-01-01A; the Taishan Scholars Project Fund under contract No. ts20190963.
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Year 2024 volume 43 Issue 1
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doi: 10.1007/s13131-023-2278-3
  • Receive Date:2023-06-03
  • Online Date:2025-11-15
  • Published:2024-01-25
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  • Received:2023-06-03
  • Accepted:2023-11-09
Funding
The National Key R&D Program of China under contract No. 2022YFC2807604; the Basic Scientific Fund for National Public Research Institutes of China under contract Nos 2022S02, 2022Q03 and 2018S02; the Marine S&T Fund of Shandong Province for Pilot National Laboratory for Marine Science and Technology (Qingdao) under contract No. 2018SDKJ0105-3; the National Natural Science Foundation of China under contract Nos 41876030, 41976021, 41876231, 4190060432 and 41706220; the program Impact and Response of Antarctic Seas to Climate Change under contract No. IRASCC 01-01-01A; the Taishan Scholars Project Fund under contract No. ts20190963.
Affiliations
    1 First Institute of Oceanography/Key Laboratory of Marine Science and Numerical Modeling, Ministry of Natural Resources, Qingdao 266061, China
    2 Laboratory for Regional Oceanography and Numerical Modeling, Laoshan Laboratory, Qingdao 266237, China
    3 Shandong Key Laboratory of Marine Science and Numerical Modeling, Qingdao 266061, China

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* Yue Fang, Email:
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表12种不同金属材料的力学参数

Family
属数
Number of
genus
种数
Number of
species
占总种数比例
Percentage of
total species (%)

Genus
种数
Number of
species
占总种数比例
Percentage of total
species (%)
鹅膏菌科Amanitaceae 2 11 5.26 鹅膏菌属 Amanita 10 4.78
小菇科 Mycenaceae 2 12 5.74 丝盖伞属 Inocybe 5 2.39
多孔菌科 Polyporaceae 8 14 6.70 蜡蘑属 Laccaria 5 2.39
红菇科 Russulaceae 3 23 11.00 小皮伞属 Marasmius 6 2.87
小菇属 Mycena 11 5.26
光柄菇属 Pluteus 5 2.39
红菇属 Russula 17 8.13
栓菌属 Trametes 5 2.39
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