1. Introduction
Subthermocline eddies have been observed in many parts of the global ocean, including those in the Mediterranean outflow (e.g., Richardson et al. 2000), in the Red Sea outflow (e.g., Shapiro and Meschanov 1991), in the California Undercurrent (e.g., Simpson and Lynn 1990), and in the Peru–Chile Undercurrent (e.g., Johnson and McTaggart 2010). These subthermocline eddies are largely invisible at the sea surface, but they may significantly affect the heat, freshwater, and other property transports in the ocean. Great interest in subthermocline eddies has been aroused because of their potentially important role in climate variability.
Sporadic in situ observations have shown evidence that subthermocline eddies also exist off east Mindanao in the Philippine Sea (e.g., Wijffels et al. 1995; Kashino et al. 1999; Firing et al. 2005; Kashino et al. 2005). Based on direct measurements from a single mooring implemented from October 1999 to July 2002, Kashino et al. (2005) showed that the circulation below and offshore of the Mindanao Current (MC) was dominated by eddy activities on time scales of 50–100 days, consistent with earlier speculation by Wijffels et al. (1995). The mooring data at 2.5°S, 142°E, around 760 m between September 1998 and October 2002, also revealed large power spectral density at periods between 20 and 60 days (Kawabe et al. 2008). By analyzing Lowered Acoustic Doppler Current Profiler (LADCP) measurements from two individual cruises, Firing et al. (2005) suggested that the northward subsurface flow near the east coast of Mindanao was actually part of a set of subthermocline eddies within about 300 km off the coast.
A question that may arise immediately from these earlier studies is how the observed low-salinity, high-oxygen subthermocline water off the Philippine coast is conveyed (Reid 1965; Qu and Lindstrom 2004), given that the mean current below and offshore the MC only reaches about 12°–13°N. Using results from an eddy-resolving ocean general circulation model (OGCM), Qu et al. (2012) recently reported that the northward intrusion of South Pacific water below and offshore the MC is largely due to subthermocline eddies. An ensemble of these subthermocline eddies can significantly enhance the northward property flux, explaining why water of South Pacific origin appears to extend farther northward than the mean current there.
Yet, because of the lack of long-term observations, these subthermocline eddies have not been carefully examined. Based on results from an eddy-resolving OGCM for the Earth Simulator (OFES), this study investigates the characteristics and in particular the pathway and energy source of subthermocline eddies in the western equatorial Pacific. Section 2 describes the configuration of OFES and provides a brief comparison with existing observations. Section 3 shows an example subthermocline eddy and its related property fields in the far western equatorial Pacific. The statistics of subthermocline eddies is shown in section 4, and the energy source of these eddies is discussed in section 5. Results are summarized in section 6.
2. Model description and validation
The OFES is based on the Modular Ocean Model, version 3.0 (MOM 3.0). Its domain covers a near-global region extending from 75°S to 75°N, with a horizontal resolution of 0.1° × 0.1°. The vertical resolution varies with a total of 54 levels from 5 m near the surface to 330 m near the bottom. The model topography was constructed from a
The OFES outputs have been analyzed by a number of earlier studies (Aoki et al. 2007; Qu et al. 2008; Dutrieux 2009; Kashino et al. 2009; Chen et al. 2010; Qu et al. 2012). These studies showed that the model reproduces nearly all of the observed features over the global ocean. In the far western tropical Pacific, Dutrieux (2009) compared the model results with available shipboard ADCP measurements, and suggested that the model represents reasonably well the regional circulation and its variability. Here, we provide additional examples of model–data comparison for the region. Figure 1 shows a comparison of the upper 220-m current between the model and mooring observations at 2.5°S, 142°E from July 1995 to July 1996. As one can see from this figure, the simulated velocities (Figs. 1d and 1e) are in good agreement with observations (Figs. 1a and 1b). The model reproduced nearly all the observed structures, including the seasonal cycle and the enhanced westward flow associated with the 1995/96 La Niña event. The correlations of upper 150-m zonal and meridional velocities between the model and the mooring data reach 0.78 and 0.70 with no time lag, respectively. The spectrum of model velocity (Fig. 1c) averaged for 150–220 m shows significant 20–30-day fluctuations, which are also markedly evident in observations [Fig. 1f and Kuroda (2000)].
Comparison of (a),(d) zonal velocity; (b),(e) meridional velocity; and (c),(f) their spectra averaged for 150–220 m at 2.5°S, 142°E from July 1995 to July 1996 for (left) mooring observations and (right) model results. The mooring data were from the Tropical Ocean Climate Study (TOCS) project of the Japan Agency for Marine-Earth Science and Technology (JAMSTEC; http://www.jamstec.go.jp/rigc/j/tcvrp/ipocvrt/adcp_data.html).
Citation: Journal of Physical Oceanography 43, 7; 10.1175/JPO-D-12-0187.1
Figure 2 shows the comparison of the subsurface for the period from September 1998 to November 1999. Here, the eddy-like, intraseasonal fluctuations are obvious in both the simulated and observed velocity fields. At ~760-m depth (Figs. 2c and 2d), for example, the two time series are well in phase despite significant differences in magnitude of the variability. The spectrum of ~760-m model velocity reveals 20–60-day fluctuations, which is consistent with the result of Kawabe et al. (2008). From these comparisons and those provided by previous studies (e.g., Masumoto et al. 2004; Sasaki et al. 2008; Dutrieux 2009), we feel that for the region studied the circulation from OFES is one of the best available in a model and the results presented in this study are mostly reliable.
Comparison of (a),(b) zonal velocity at different depths and (c),(d) velocity vector at ~760 m at 2.5°S, 142°E from September 1998 to November 1999 between mooring observations (a),(c) and model results (b),(d). Here, (a),(c) are after Zenk et al. (2005) and Kawabe et al. (2008), respectively.
Citation: Journal of Physical Oceanography 43, 7; 10.1175/JPO-D-12-0187.1
3. An example subthermocline eddy
The western equatorial Pacific is populated with eddies of various time scales not only in surface layer (e.g., Kashino et al. 1999, 2007, 2009) but also in the subthermocline (e.g., Firing et al. 2005; Kashino et al. 2005; Kawabe et al. 2008). As one can see from section 2 (Figs. 1 and 2), the subthermocline eddies in the western equatorial Pacific are also simulated by the OFES. As an example, Fig. 3 shows the temporal evolution from 13 March to 12 May 1985, and the vertical structure on 12 April 1985, of an individual subthermocline eddy located at 0.05°S, 139.15°E. The time–depth and longitude–depth profiles of salinity show a low-salinity lens in mid-April, when salinity is lowered by up to 0.08 psu (Figs. 3a and 3c). This low-salinity lens extends between the depths of about 500 and 650 m, with a core lying at about 550 m around 12 April, consistent with its South Pacific origin (e.g., Qu and Lindstrom 2004). This depth range roughly corresponds to a density range of σθ = 27.0–27.1 kg m−3. As shown in Figs. 3b and 3d, similar patterns are seen for potential temperature, in which a thermostad around the 5.9°–6.9°C isotherms lies between about 500 and 675 m, roughly coinciding with the maximum-salinity anomaly. Both isotherms and isohalines bow up to about 500 m above the core of the eddy but become relatively flat below it. These characteristics resemble those reported by earlier studies in other parts of the global ocean (e.g., Johnson and McTaggart 2010). According to Fig. 3 and the temperature/salinity structure in the other parts of the region studied, the main depth range of subthermocline eddies is around 600 m, and the low-salinity signature can extend upward to 500-m depth. Although the temperature/salinity measurements of the Triangle Trans-Ocean Buoy Network (TRITON; http://www.jamstec.go.jp/jamstec/TRITON/real_time/php/top.php) in the region studied only exist at the depths of 300, 500, and 750 m in the subthermocline, the data at 0°, 138°E can still reveal the existence of low-salinity events (Fig. 4), suggesting that subthermocline eddies are a prominent phenomenon of the region.
OFES-modeled profiles of (a),(c) salinity and (b),(d) potential temperature. Time–depth profiles at 0.05°S, 139.1°E during the period from 13 Mar to 12 May 1985 (top); longitude–depth profiles along 0.05°S in 15 Apr 1985 (bottom). White contours represent isopycnal surfaces of 27, 27.05, and 27.1 kg m−3.
Citation: Journal of Physical Oceanography 43, 7; 10.1175/JPO-D-12-0187.1
(a),(c) Salinity and (b),(d) temperature profiles at 0°, 138°E observed by TRITON from (top) 12 Jul to 11 Sep 2005 and (bottom) May 10 to 9 Jul 2006.
Citation: Journal of Physical Oceanography 43, 7; 10.1175/JPO-D-12-0187.1
4. Statistics
Eddy kinetic energy (EKE) calculated from the model outputs can be used as a measure of variability. Here, the EKE (per unit mass) is defined as
(a),(b),(c) EKE and the zonal and meridional components (EKEZ and EKEM) derived from the zonal and meridional velocities at 605 m at 6°S–8°N, 125°–147°E. (d),(e),(f) As in (a),(b),(c), but for EKE and the along- and cross-shore components (EKEAS and EKECS) north of New Guinea at 6°S–4°N, 128°–146°E. (f) The black line indicates the eddies' pathway parallel to the New Guinea coast for Figs. 7 and 8.
Citation: Journal of Physical Oceanography 43, 7; 10.1175/JPO-D-12-0187.1
Schematic diagram of influence of propagating eddies on velocity anomaly. Dotted circles symbolize eddies and arrow represents the propagating direction of eddies. Red and blue stars denote the high velocity anomalies generated by eddies in the direction perpendicular and parallel to the moving direction, respectively.
Citation: Journal of Physical Oceanography 43, 7; 10.1175/JPO-D-12-0187.1
The subthermocline eddies off the Mindanao coast can be traced southward to the New Guinea coast. To better illustrate the eddy activities along the New Guinea coast, the EKE associated with alongshore and cross-shore velocity deviations from the 30-yr-mean values,
Following the eddies' pathway parallel to the New Guinea coast at 605 m (marked by the black line in Fig. 5f), more than 80% of the total variance in
Hovmöller diagrams of (left)
Citation: Journal of Physical Oceanography 43, 7; 10.1175/JPO-D-12-0187.1
(a) Power spectral density (PSD) at 605 m, (b) PSD profile of 50–60-day-bandpassed
Citation: Journal of Physical Oceanography 43, 7; 10.1175/JPO-D-12-0187.1
5. Energy source
In addition to the station at 0°, 138°E discussed above, there are two other TRITON stations (0°, 147°E and 0°, 156°E) in the western equatorial Pacific. The mean salinities at 500 m of these three stations are very close (34.604, 34.607, and 34.609 psu), but their corresponding standard deviations are very different (0.0208, 0.0173, and 0.0177 psu), with the value at 0°, 138°E being significantly larger than those at the other two stations. This difference could be related to the fact that the station at 0°, 138°E is geographically much closer to the pathway of subthermocline eddies along the western boundary than the other two stations. As shown in the lag correlation maps of 50–60-day-bandpassed vorticity at 605 m relative to 0.675°S, 141°E (Fig. 9a) or roughly the middle of New Guinea Coast (the black line of Fig. 5f), most subthermocline eddies in the western tropical Pacific originate from the equatorial South Pacific. In most cases, they propagate northwestward along the New Guinea coast and cross the equator in the far western Pacific. Both Figs. 9a and 9b show that the subthermocline eddies originate from the region to the west of the Ninigo Group near ~1.25°S, 143°E but not from the east (e.g., central or eastern Pacific). These eddies propagate predominantly along the pathway marked by the red line in Fig. 9.
Lag correlation maps of 50–60-day-bandpassed vorticity relative to the vorticity at (a) 0.675°S, 141°E and (b) 0.025°S, 139°E. Triangles, red lines, and green lines indicate the relative location, pathway of eddies, and 605-m isobath, respectively.
Citation: Journal of Physical Oceanography 43, 7; 10.1175/JPO-D-12-0187.1
Firing et al. (2005) suggested that local wind forcing or instability of local upper-ocean currents cannot be the energy source of subthermocline eddies in the region studied. Kashino et al. (2005) reported that the MC intraseasonal variability was not well correlated with the atmospheric intraseasonal variability. The typical propagation speed of these subthermocline eddies (~0.12 m s−1) is significantly smaller than the propagation speed (larger than 1.2 m s−1) of the first baroclinic Rossby waves in the tropical ocean, suggesting that the formation of these subthermocline eddies is not associated with the β effect. The mean subthermocline current along the Mindanao coast is rather weak (Qu et al. 2012) and is unlikely the energy source of subthermocline eddies. The formation of subthermocline eddies may be related to intrinsic ocean variability (Kashino et al. 2007) and/or interaction of ocean currents with complex bathymetry. According to the time-mean energy budget (Masina et al. 1999), the barotropic conversion term can be written as
Horizontal patterns of time-mean (a) barotropic conversion and (b) baroclinic conversion at 605 m. Area with depth shallower than the depth of each panel is depicted as gray shading while that above the sea level is shaded by black color. Red lines indicate the pathway of eddies.
Citation: Journal of Physical Oceanography 43, 7; 10.1175/JPO-D-12-0187.1
The distributions of mean currents and 50–60-day-bandpassed EKECS at 507, 605, and 694 m are shown in Figs. 11a–c. Except for a stronger signal extending farther eastward at 605 m, the EKECS distributions at these three depths show essentially the same pattern, with a high EKECS band lying northwestward along the New Guinea coast, consistent with the distribution of along-pathway power spectral density shown in Fig. 8b. The high EKECS band is located just north of the northwestward-flowing New Guinea Coastal Undercurrent (NGCUC) (Lindstrom et al. 1987). Aside from the NGCUC, the formation of high EKECS band could also be related to the westward-flowing Lower Equatorial Intermediate Current (LEIC). The NGCUC gets weaker with depth, and the LEIC starts to appear at depths around 694 m. Possible interaction between the two currents was previously suggested by Kawabe et al. (2008).
Cross-shore component of 50–60-bandpassed EKECS (shading) and mean flow (vectors) patterns at the depths of (a) 527, (b) 605, and (c) 694 m, and (d) schema of major currents at 694 m around the Ninigo Group. Area with depth shallower than the depth of each panel is depicted as gray shading while that above the sea level is shaded by black color. Red lines indicate the pathway of eddies. The abbreviation of the Ninigo Group is N.
Citation: Journal of Physical Oceanography 43, 7; 10.1175/JPO-D-12-0187.1
On the other hand, the bottom topography in the vicinity of these two currents, being composed of the Manus Island (the largest island of the Admiralty Islands) and the Ninigo Group [a group of atolls, islands, and reefs including Awin Atoll, Suymasuma Island, Sama Group, Ninigo Islands (a very large atoll), Pelleluhu Group, Heina Group, Pupol Reef (a low lying reef), and Liot Island], is very complicated and likely provides a favorable condition for the generation of subthermocline eddies there. Figures 10 and 11a–c show the NGCUC and LEIC hit the seamounts near 142°E, cause barotropic instability, and generate high EKECS signals that propagate farther westward (Fig. 11d). We therefore suggest that interactions among the NGCUC, LEIC, and complex bottom topography associated with the Ninigo Group are primarily responsible for the generation of subthermocline eddies in the western equatorial Pacific.
6. Summary
In this study, we have provided the first quantitative evidence for the existence of subthermocline eddies in the western equatorial Pacific by examining the results from an eddy-resolving OGCM. Most subthermocline eddies in the region appear to originate from the equatorial South Pacific to the west of the Ninigo Group. These eddies convey relatively fresh South Pacific water westward to the western boundary. From there, they move northwestward along the New Guinea coast, cross the equator in the far western Pacific, and reach the coast of the Philippines, exerting notable impacts on the property distribution in the western equatorial Pacific. The dominant time scale of these eddies is about 55 days, with their strongest signature occurring near 600 m. Some of these eddies may be related to the instability of currents as is the case in many other parts of the ocean. Here, we emphasize the importance of bottom topography. We suspect that the generation of subthermocline eddies in the western equatorial Pacific is due in large part to the interactions among the NGCUC, LEIC, and complex topography associated with the Ninigo Group. The details need to be further investigated as more long-term observations become available.
Acknowledgments
This research was supported Taiwan National Science Council through Grants 100-2811-M-003-013 and 101-2811-M-003-017 and by U.S. National Science Foundation through Grants OCE10-29704 and OCE11-30050. The authors are grateful to C.-R. Wu and Y. Kashino for useful communication on the topic, to H. Sasaki and colleagues from the Earth Simulator for assistance in processing the OFES outputs, to the Japan Agency for Marine-Earth Science and Technology (JAMSTEC) for the Tropical Ocean Climate Study (TOCS) project ADCP mooring data and Triangle Trans-Ocean Buoy Network (TRITON) data, and to the two anonymous reviewers for their thoughtful comments on an earlier version of the manuscript.
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