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VOLUME 11 MARCH 1998 JOURNAL OF CLIMATE q 1998 American Meteorological Society 297 Decadal Variability in the North Pacific as Simulated by a Hybrid Coupled Model W. XU AND T. P. BARNETT Scripps Institute of Oceanography, La Jolla, California M. LATIF Max-Planck Institute for Meteorology, Hamburg, Germany (Manuscript received 15 May 1996, in final form 8 May 1997) ABSTRACT In this study, a hybrid coupled model (HCM) is used to investigate the physics of decadal variability in the North Pacific. This aids in an understanding of the inherent properties of the coupled ocean–atmosphere system in the absence of stochastic forcing by noncoupled variability. It is shown that the HCM simulates a self-sustained decadal oscillation with a period of about 20 yr, similar to that found in both the observations and coupled GCMs. Sensitivity experiments are carried out to determine the relative importance of wind stresses, net surface heat flux, and freshwater flux on the initiation and maintenance of the decadal oscillation in the North Pacific. It is found that decadal variability is a mode of the coupled system and involves interaction of sea surface temperature, upper-ocean heat content, and wind stress. This interaction is mainly controlled by the wind stress but can be strongly modified by the surface heat flux. The effect of the salinity is relatively small and is not necessary to generate the model decadal oscillation in the North Pacific. There are some limitations with this study. First, the effect of a stochastic forcing is not included. Second, a weak negative feedback is needed to run the control experiment for a longer time period. These two areas will be addressed in a future investigation. 1. Introduction There are mainly two types of decadal variability in the North Pacific as summarized by Latif and Barnett (1996). The first type is associated with the most recent climate shift in the North Pacific, which occurred around 1977 (Venrick et al. 1987; Nitta and Yamada 1989; Gra- ham et al. 1994; Miller et al. 1994; Trenberth and Hurrell 1994). These authors agree that it is atmospheric forcing that drives the ocean variation, and the origins of the these changes can be traced to the abrupt shift of the tropical Pacific SST (sea surface temperature). The second type of decadal change is more oscillatory in nature. This oscillation involves air–sea feedbacks in midlatitudes. The possibility of unstable ocean–atmo- sphere interactions in midlatitudes on seasonal and lon- ger timescales was originally hypothesized in a series of papers by Namias (e.g., 1959, 1969) for the North Pacific and Bjerknes (1964) for the North Atlantic. Na- mias argued that SST anomalies in the North Pacific can change the transient eddy activity in the atmosphere, Corresponding author address: Dr. Weimin Xu, Department of Atmospheric and Oceanic Science, University of Wisconsin—Mad- ison, 1225 W. Dayton Street, Madison, WI 53706. E-mail: [email protected] which in turn changes the mean westerly flow rein- forcing the initial SST anomalies. Bjerknes found that the decadal cycle in the North Atlantic involves inter- actions of the westerly wind and the subtropical gyre. Similar results were obtained in the more recent obser- vational studies by Kushnir (1994), Deser and Black- mon (1993, 1995), and a coupled GCM (General Cir- culation Model) study by Delworth et al. (1993). Latif and Barnett (1994, 1996; hereafter LB94, LB96) showed that, based on the results of a coupled GCM and ob- servations, both Namias’s and Bjerknes’s may be im- portant in the decadal variation in the North Pacific– North American mode. Their conclusions are supported by Xu et al. (1998, manuscript submitted to J. Climate) and Tonimoto et al. (1993). Most of the CPU time used in running coupled at- mosphere–ocean GCMs is consumed by the atmospheric GCMs (90%). This, coupled with the current computer limitations, means that the extensive coupled runs re- quired to investigate decadal variability are difficult to carry out. More efficient atmospheric models, which can capture the essential physics of air–sea coupling, are needed to solve this problem and enhance our ability to model and study the long term climate variabilities. In this paper, we will construct a simple atmospheric model based on the data from a fully coupled ocean–

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Page 1: Decadal Variability in the North Pacific as Simulated by a ... · PDF fileDecadal Variability in the North Pacific as Simulated by a Hybrid Coupled Model ... in final form 8 May

VOLUME 11 MARCH 1998J O U R N A L O F C L I M A T E

q 1998 American Meteorological Society 297

Decadal Variability in the North Pacific as Simulated by a Hybrid Coupled Model

W. XU AND T. P. BARNETT

Scripps Institute of Oceanography, La Jolla, California

M. LATIF

Max-Planck Institute for Meteorology, Hamburg, Germany

(Manuscript received 15 May 1996, in final form 8 May 1997)

ABSTRACT

In this study, a hybrid coupled model (HCM) is used to investigate the physics of decadal variability in theNorth Pacific. This aids in an understanding of the inherent properties of the coupled ocean–atmosphere systemin the absence of stochastic forcing by noncoupled variability. It is shown that the HCM simulates a self-sustaineddecadal oscillation with a period of about 20 yr, similar to that found in both the observations and coupledGCMs.

Sensitivity experiments are carried out to determine the relative importance of wind stresses, net surface heatflux, and freshwater flux on the initiation and maintenance of the decadal oscillation in the North Pacific. It isfound that decadal variability is a mode of the coupled system and involves interaction of sea surface temperature,upper-ocean heat content, and wind stress. This interaction is mainly controlled by the wind stress but can bestrongly modified by the surface heat flux. The effect of the salinity is relatively small and is not necessary togenerate the model decadal oscillation in the North Pacific.

There are some limitations with this study. First, the effect of a stochastic forcing is not included. Second, aweak negative feedback is needed to run the control experiment for a longer time period. These two areas willbe addressed in a future investigation.

1. Introduction

There are mainly two types of decadal variability inthe North Pacific as summarized by Latif and Barnett(1996). The first type is associated with the most recentclimate shift in the North Pacific, which occurred around1977 (Venrick et al. 1987; Nitta and Yamada 1989; Gra-ham et al. 1994; Miller et al. 1994; Trenberth and Hurrell1994). These authors agree that it is atmospheric forcingthat drives the ocean variation, and the origins of thethese changes can be traced to the abrupt shift of thetropical Pacific SST (sea surface temperature).

The second type of decadal change is more oscillatoryin nature. This oscillation involves air–sea feedbacks inmidlatitudes. The possibility of unstable ocean–atmo-sphere interactions in midlatitudes on seasonal and lon-ger timescales was originally hypothesized in a seriesof papers by Namias (e.g., 1959, 1969) for the NorthPacific and Bjerknes (1964) for the North Atlantic. Na-mias argued that SST anomalies in the North Pacificcan change the transient eddy activity in the atmosphere,

Corresponding author address: Dr. Weimin Xu, Department ofAtmospheric and Oceanic Science, University of Wisconsin—Mad-ison, 1225 W. Dayton Street, Madison, WI 53706.E-mail: [email protected]

which in turn changes the mean westerly flow rein-forcing the initial SST anomalies. Bjerknes found thatthe decadal cycle in the North Atlantic involves inter-actions of the westerly wind and the subtropical gyre.Similar results were obtained in the more recent obser-vational studies by Kushnir (1994), Deser and Black-mon (1993, 1995), and a coupled GCM (General Cir-culation Model) study by Delworth et al. (1993). Latifand Barnett (1994, 1996; hereafter LB94, LB96) showedthat, based on the results of a coupled GCM and ob-servations, both Namias’s and Bjerknes’s may be im-portant in the decadal variation in the North Pacific–North American mode. Their conclusions are supportedby Xu et al. (1998, manuscript submitted to J. Climate)and Tonimoto et al. (1993).

Most of the CPU time used in running coupled at-mosphere–ocean GCMs is consumed by the atmosphericGCMs (90%). This, coupled with the current computerlimitations, means that the extensive coupled runs re-quired to investigate decadal variability are difficult tocarry out. More efficient atmospheric models, which cancapture the essential physics of air–sea coupling, areneeded to solve this problem and enhance our ability tomodel and study the long term climate variabilities.

In this paper, we will construct a simple atmosphericmodel based on the data from a fully coupled ocean–

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TABLE 1. A summary of the numerical experiments. All of theseforcings are anomalies.

Experiment Wind stress Heat flux Freshwater flux

E1 (Control)E2E3E4

YesYesNoYes

YesNoYesYes

NoNoNoYes

atmospheric GCM (ECHO, see LB94, LB96, and Xu etal. 1996, hereafter X96) and couple it to an OGCM(ocean GCM) following the methodology used in Bar-nett et al. (1993). The atmospheric model is an anomalymodel and statistical in nature. This type of coupledmodel is usually termed the hybrid coupled general cir-culation model (HCM), which has been used in the trop-ical Pacific by Neelin (1990), Barnett et al. (1993), andSyu et al. (1995).

The organization of the paper is as follows: section2 describes the OGCM and the construction of the at-mospheric model, as well as the data and the perfor-mance of the atmospheric model; section 3 describesthe design of numerical experiments to explore the de-cadal variability; section 4 evaluates the decadal vari-ability in the North Pacific as simulated by the HCMagainst complete coupled models and observations; andsection 5 presents the results of sensitivity experimentsdesigned to further the physical interpretation of theHCM. The paper is summarized and concluded in sec-tions 6 and 7, respectively.

2. Numerical models

a. The ocean model

The ocean model used in this study is based on aprimitive equation OGCM, HOPE (Hamburg OceanModel in primitive equations), simplified by the hydro-static and Boussinesq approximations (Wolff and Maier-Reimer 1997; LB94; LB96; X96). The HOPE model isa further development of the model used by Latif (1987),Barnett et al. (1991), Luksch and von Storch (1992),Latif et al. (1993a,b), and Latif et al. (1994).

The OGCM used has 20 levels in the vertical, with 10of them in the upper 300 m. It is a North Pacific (NP)basin model with realistic topography. The zonal reso-lution is about 2.88; the latitudinal resolution is variablewith a high resolution of 0.58 within 108 of the equatorand gradually increases to 2.88 poleward of 208. Theocean model includes a simple mixed-layer parameter-ization (Wolff and Maier-Reimer 1997), which increasesthe vertical viscosity and diffusivity by a specified wind-induced mixed-layer turbulence (0.002 m2 s21) if a ver-tical temperature difference between subsurface and sur-face is smaller than a preset DT (0.58C). About 14.6%of the solar radiation incident on the ocean surface isallowed to penetrate beneath the 20-m surface layer ofthe model (Paulson and Simpson 1977; Schneider et al.

1996). The horizontal domain is from 108 to 608N andfrom 1008 to 2608E. A sponge layer was added near thesouthern (between 38 and 108N) and northern (between608 and 708N) boundaries, where a Newtonian restoringterm was used for both temperature and salinity. [Themonthly mean SST and SSS (sea surface salinity) fromthe ECHO coupled model were used as the referencefields.] A sea-ice model has not been included yet.

b. The atmospheric model

The basic physical assumption in deriving a simpleatmospheric model is that the ocean is the importantsource of memory for the coupled system, and the at-mosphere can be effectively treated as a fast, adjustedcomponent.

The atmospheric model is a statistical model basedon 100 yr of data from the ECHO coupled model, whichconsists of the Hamburg version of the European centeratmospheric GCM (ECHAM3; Roeckner et al. 1992)and HOPE oceanic GCM. Four fields are used to con-struct the atmospheric model, that is, SST anomaly(SSTA), net surface heat flux anomaly, and zonal andmeridional wind stress anomalies. The model is similarto that of Barnett et al. (1993), with extension to thewhole NP and the inclusion of a surface heat flux anom-aly, which is important in midlatitudes (LB94; LB96;X96).

SST [T(x, t)] and atmospheric variables P(x, t) (windstress, surface heat flux, and freshwater flux) are ex-pressed in terms of ‘‘fixed-phase’’ empirical orthogonalfunctions (EOFs) for each individual month (i.e., thereis one atmospheric model for each calendar month,which is used to include some effect of the seasonalmodulation of the atmospheric response to a givenSSTA),

T(x, t) 5 a (t)e (x) (1)O n n

P 5 b (t) f (x), (2)O n n

where the spatial variable x is defined as the NP regionbetween 108 and 608N and between 1008 and 2608E, thetemporal variable t as the calendar months, a and b arethe EOF temporal coefficients, and e and f are the spa-tial coefficients.

The matrix of regression coefficients relating SSTAand atmospheric fields can be expressed as

^a b &n mC 5 , (3)mn 2^a &n

where ^ . . . & denotes a time average. The statistical es-timate of the atmospheric field is obtained from

a (t) 5 T(x, t)e (x), (4)On n

b (t) 5 C a (t), (5)Om mn n

and finally,

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FIG. 1. The time series of SSTA (8C) at the midlatitude North Pacific (258–358N; 1508–1808E) for E1 (solid line), the control case, including both wind stress and surface heat fluxanomalous forcings; E2 (dotted line), the anomalous wind stress forcing only case; E3(dashed line), the anomalous surface heat flux only case; E4 (dashed–dotted line), the anom-alous freshwater flux case, including anomalous wind stress, surface heat flux, and freshwaterflux forcings.

ˆ ˆP(x, t) 5 b (t) f (x), (6)O m m

where ( ) indicates a predicted variable. When SSTAˆis derived from the OGCM, its effect is transmitted di-rectly to the atmospheric model. In turn, the new anom-alous atmospheric forcings will be added back to theocean surface layer.

c. The data and performance of the atmospheric model

The 100-yr monthly mean SST, SSS, solar radiation,net surface heat flux, freshwater flux, and zonal and

meridional wind stress were archived from the ECHOcoupled GCM (LB94; LB96; X96). From this dataset,we derived the monthly anomaly data for constructingthe atmospheric model. The monthly mean data werefirst detrended and then low-pass filtered to removetimescales shorter than 7 yr. The monthly anomalies ofSST, net surface heat flux, freshwater flux, and zonaland meridional wind stress for the NP were used toconstruct the statistical atmospheric model. These pro-cedures ensure that the correlation between SSTA andanomalies in P(x, t) in the NP is mainly due to mid-

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FIG. 2. The correlation between the time series of SSTA in Fig. 1 (solid lines) and gridpoint SSTA for E1 at (a) lag 10, (b) lag 5, (c) lag2, and (d) lag 0. Dark (gray) indicates negative (positive) values.

latitude air–sea interaction with no direct tropical(ENSO) effect.

We calculated the net surface heat flux, freshwaterflux, and wind stress anomalies based on the SSTA fromthe ECHO model using the statistical atmospheric mod-el. (The first ten EOF modes were kept.) The correla-tions (0.85) between the predicted fields and the originalfields from the ECHO model are significant at the 1%level (0.4), and the predicted fields usually explain over70% of the total variance. Therefore, the statistical at-mospheric model captures some of the essential physicsimplied in the original data.

3. Design of the experiments

The OGCM was first run to an equilibrium state sothat no significant drift in both the basin mean and thegridpoint SST were found (see the appendix). The dailymean SST and SSS were saved and used to diagnosethe heat and freshwater fluxes at every time step. Thesediagnosed heat and freshwater fluxes were then used todrive the OGCM (Sausen et al. 1988), with the restoringterms in (A1) and (A2) removed (see the appendix). The

new SST and SSS forced by the diagnosed heat andfreshwater fluxes were very close to the SST and SSSin the experiment with restoring surface boundary con-ditions. The statistical atmospheric model was then cou-pled to the OGCM, that is, the anomalous fluxes (heat,momentum, and freshwater flux) from the time-depen-dent statistical atmospheric model were added back totheir mean fields to drive the OGCM.

In the first experiment (hereafter, control run or E1),only anomalous net surface heat flux and wind stressare used because they are the main forcing in the NPocean (LB94; LB96; X96). Since the statistical atmo-spheric model is driven purely by SSTA, and the initialcondition as obtained in the spinup had almost no SSTA,we specified the first EOF of annual SSTA scaled upto 18C (the maximum SSTA) as the initial SSTA to drivethe atmosphere model for 1 yr. (During this period, thestatistical atmospheric model was kept constant, butSSTA evolved with time.) At the end of the first year,the SSTA from the OGCM was fed back to the statisticalatmosphere model and free coupling started at year 2and continued until year 70.

We also carried out three additional experiments to

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FIG. 3. Same as Fig. 2 but for the zonal wind stress anomaly.

investigate the effects of anomalous wind stress, netsurface heat flux, and freshwater flux. The experimentsare summarized in Table 1. In the second experimentE2, the only response of the atmospheric model to agiven SSTA is the wind stress anomaly. In the thirdexperiment, E3, the only response of the atmosphericmodel to a given SSTA is the net surface heat fluxanomaly. Finally, we examined the effect of salinity onthe decadal variability in the NP by adding the fresh-water flux anomaly, E4, to the control run. The initialconditions for E2, E3, and E4 were those at the end ofyear 20 in E1. All the sensitivity experiments were thenrun for an additional 50 yr.

4. Physics of the decadal variability

This section examines the physics of decadal vari-ability in the control run E1 and is the basis for dis-cussing the sensitivity studies in the next section.

a. The evolution of SSTA

Figure 1a (solid line) shows the time series of SSTAin the western midlatitude North Pacific (258–358N;

1508–1808E, this region was chosen for its proximityto the model Kuroshio extension) for E1. The SSTAhas decadal variability with a timescale of ;20 yr.

Figure 2 shows the spatial pattern of the correlationbetween SSTA and the time series shown in Fig. 1 atdifferent lag times for E1. At lag 0 (Fig. 2d), thedominant pattern is similar to those of LB94 andLB96. The evolution of the dominant mode shown inFig. 2d is illustrated by the SSTA correlation patternat lags of 10, 5, and 2 yr prior to the time corre-sponding to panel 2d (lag 0). At lag 10 (Fig. 2a), thecorrelation pattern is very similar to that in Fig. 2dbut with the opposite polarity. Five years later (Fig.2b), the cold SST moved both northward and east-ward, and the western subtropical gyre started warm-ing. Favorite and McClain (1973) and Michaelsen(1982) found similar features in the observations. Atthe same time, cooling started in the NP equatorialcurrent region. Three years later (Fig. 2c), the SSTAin the western subtropical gyre became positive, whilethe SSTA in the southern subtropical gyre becamenegative. The evolution of SSTA in the HCM is sim-ilar to those found in a fully coupled ocean–atmo-spheric GCM and the observations (LB94; LB96;

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FIG. 4. Same as Fig. 2 but for the meridional wind stress anomaly.

X96). The evolution of heat content (averaged oceantemperature over the upper 400 m, not shown) showsa very similar spatial pattern to that of SSTA, exceptthat the heat content anomaly has somewhat strongerfeatures and is located a little southward of SSTA.The Hovmoeller diagrams (not shown) indicate thatonly the heat content anomaly shows westward prop-agation in the subtropics. All other quantities (in-cluding SSTA and wind stress anomalies) look moreor less like standing oscillations.

b. The atmospheric response

Figure 3 shows the correlation between zonal windstress anomalies and the SSTA time series shown in Fig.1a. The westerlies are weaker (stronger) than normal inthe NP north (south) of about 408N when SSTA is neg-ative in midlatitudes (lag 10). The opposite is true whenSSTA is positive in midlatitudes (lag 2, lag 0). Thestanding wave nature of the spatial pattern is particularlyclear in this illustration. Figure 4 shows the evolutionof meridional wind stress. There are southerly (north-erly) wind stress anomalies associated with positive(negative) SSTA, consistent with observations (Seckel

1993; White and Chen 1998, manuscript submitted toJ. Climate).

It is interesting to note that the relationship betweenSSTA and wind stress at lag 5, that is, the transientstage from cold midlatitude SSTA to warm midlatitudeSSTA (or vice versa), is different from that found at lag10, lag 2, and lag 0. The significant features at this stageare (a) the maximum cold SSTA moves to the Aleutianlow center which effectively changes the strength of theAleutian low; and (b) the SSTA has minimum north–south and east–west gradient so that large-scale atmo-spheric circulation anomalies are dominated by the vari-ation of the Aleutian low rather than by local mecha-nisms. We must emphasize that this does not mean thatthe ocean is purely driven by the atmosphere. In fact,2 yr before the transient phase (Fig. 5b), the SST ten-dency already had the potential to develop SSTA asshown in Fig. 2c. Therefore, the transient phase seemsto speed up the existing process (i.e., from Fig. 2b toFig. 2c).

The response of the atmosphere to SSTA has beenextensively investigated (e.g., Davis 1978; Frankignoul1985; Palmer and Sun 1985; LB94; LB96; Peng et al.1995; Lau and Nath 1994; Graham et al. 1994), though

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FIG. 5. The regression coefficient [8C (10 yr)21] between the time series of SSTA for E1 in Fig. 1 and gridpoint SSTA tendency forexperiment 1 at (a) lag 10; (b) lag 7; (c) lag 2; and (d) lag 0. Dark (gray) indicates negative (positive) values.

different studies may have reached somewhat differentconclusions. However, the main response of the atmo-sphere to SSTA is meridional (zonal) wind stress anom-aly at high (low) latitudes (White and Chen 1998, manu-script submitted to J. Climate).

The evolution of the wind stress curl (not shown)indicates that positive (negative) SSTA in the midlati-tude western NP is usually associated with a stronger(weaker) subtropical gyre and a weaker (stronger) sub-polar gyre (not shown) (Anderson and Gill 1975). Thisis consistent with LB94 and LB96 who suggested thatit is the stronger (weaker) subtropical gyre circulationwhich brings more (less) warm water to the midlatitudeNP and switches the SSTA from one phase to the other.

c. The mechanisms of SST evolution

We now explore the cause of SST evolution as shownin Fig. 2. The physical processes that may be importantin driving SSTA are (a) air–sea exchange, (b) horizontaladvection, and (c) vertical mixing and vertical advec-tion. In the following sections, we will calculate (a) and

(b) components directly and estimate (c) as a residualterm.

Figure 5 is the regressive SSTA tendency in half ofthe decadal cycle. At lag 10, the SSTA tendency is suchthat it pushes the negative midlatitude western NP SSTAboth northward and eastward. At the same time, the SSTbecomes warmer in the southern branch of the subtrop-ical gyre. At lag 7, the western part of the subtropicalgyre starts to warm up and the anomaly further developsand expands at lag 2. At lag 0, which is the maturephase shown in Fig. 2, the SST tendency is similar tothat at lag 10 (not exactly the same, since the period ofthe decadal cycle is not exactly 20 yr but with oppositepolarity.

Figure 6 shows the horizontal heat advection com-ponent of the SSTA tendency shown in Fig. 5. Thespatial pattern is very complex. However, there is a goodcorrelation between SST tendency and horizontal ad-vection in the western part of the the subtropical gyre,where the net surface heat flux (Fig. 7) seems to be outof phase with the SST tendency.

We calculated the wave (defined as V9 · =T) and gyre

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FIG. 6. Same as Fig. 5 but for horizontal heat advection [8C yr21).

(defined as V ·=T9) contributions to the horizontal heatadvection and found the dominance by wave propaga-tion consistent with the full coupled ECHO model re-sults (X96). However, V ·=T9 is comparable to V9 · =Tnear the southwest NP in the subtropical gyre recircu-lation region.

The effect of the surface heat flux (heat flux into oceanis defined as positive) on the evolution of SSTA isshown in Fig. 7. Since the mixed-layer depth is not wellsimulated in OGCMs (Sterl and Kattenberg 1994) com-pared to the observations (Levitus 1982; Deser et al.1997), we used a constant annual mean mixed-layerdepth of 30 m. At lag 10 (Fig. 7a), that is, the coldphase (when the midlatitude western NP has maximumnegative SSTA), the surface heat flux anomaly is neg-ative over most of the midlatitudes (i.e., positive air–sea feedback) due to the stronger westerly and/or north-erly winds. Five years later, the negative SSTA in themidlatitudes becomes weaker, and the heat flux anomalybecomes positive, so that less heat is extracted from theocean due to the weakening of westerly and strength-ening of southerly winds (Figs. 3, 4), and so warmingbegins.

Examination of the ECHO coupled model results andthe observations indicate that the weakening of negativemidlatitude SSTA and strengthening of positive SSTAin the southern subtropical gyre help to move the sub-tropical high pressure northward, which brings moistwarm air from the subtropics into the midlatitudes. Dur-ing this growth phase, SSTA grows and expands north-eastward rapidly, due partly to this feedback.

5. The sensitivity of decadal variabilityWe have shown above that the HCM reproduces some

features of the observed decadal variability and thosesimulated in a complete coupled circulation model(ECHO). This section further explores the mechanismsresponsible for the simulated variability through a seriesof sensitivity experiments. The sensitivity experimentswere started from the end of year 20 of the control case,E1.

a. The effect of wind stress

In E2, there is no direct surface heat flux from theatmosphere and the principal physical processes affect-

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FIG. 7. Same as Fig. 5 but for net surface heat flux (8C yr21).

ing SSTA are horizontal advection and vertical mixing–advection driven by the wind stress anomaly.

Figure 1 (dotted line) shows the time series of SSTAfor E2 at the same location as used for E1 in Fig. 1. Itshows a decadal variability with a timescale of about20 yr similar to that in the control case but with a smalleramplitude. This is consistent with the simulation byLuksch et al. (1990). Including anomalous heat flux sig-nificantly improves the simulation because of the pos-itive air–sea feedback, a point to be discussed below.

Figure 8 shows the correlation of SSTA from E2 withthe time series shown in Fig. 1b. The evolution of SSTAis similar to those of E1 (compare with Fig. 2), exceptthat the midlatitude SSTAs extend slightly more east-ward in E2. Although anomalous turbulent heat flux isessential in producing short timescale (monthly) SSTvariability (Luksch and von Storch 1992; X96), windstress forcing variation alone seems to be sufficient togenerate a large-scale SSTA in the midlatitude NorthPacific at interannual or decadal timescales (Haney1985; Luksch et al. 1990). The evolution of heat contentand wind stress curl (not shown) associated with theSSTA is also similar to E1.

As expected from the evolution of SSTA, the hori-

zontal heat advection in E2 (not shown) is similar tothat in E1. Although there is no surface heat flux forcingincluded, part of the surface heat flux effect is nowreplaced by the vertical advection and/or vertical mix-ing. It is important to note that the weaker nature of theSSTA patterns in E2 is likely due to omission of thepositive feedback between surface heat flux anomalyand SSTA.

In summary, we have shown that the wind stress forc-ing can generate decadal variability similar to that inthe control run, but with smaller amplitude. The changeof SSTA in the subtropical gyre by horizontal advectionand horizontal wave propagation can alter wind stress,which, in turn, affects SSTA through vertical mixing/advection in such a way that SSTA will be developedand expanded north and northeastward.

b. The effect of surface heat flux

The effect of the anomalous surface heat flux forcingis considered in E3. The timescale of the variability ofSSTA is 40 yr (Fig. 1, dashed line), about twice as longas that in E1 and E2. (We ran E3 for 150 yr, but theresults are basically the same as the first 50 yr shown

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FIG. 8. The correlation between the time series of SSTA for E2 in Fig. 1 (dotted lines) and gridpoint SSTA for at E2 (a) lag 10; (b) lag5; (c) lag 2; and (d) lag 0. Dark (gray) indicates negative (positive) values.

here.) The reason for the longer oscillating period isbecause the major negative feedback mechanism is geo-strophic heat advection induced by the surface heat fluxanomaly. This heat advection is much slower than Ek-man transport, vertical mixing, and wave propagationforced by wind stress. We also note that the SSTA ofE3 has a larger amplitude than that of E2. Part of thereason is because slow evolution in E3 allows the pos-itive air–sea feedback to drive SSTA over a longer pe-riod.

Figure 9 shows the SST evolution during 15 yr andcan be compared with E1 (Fig. 2). At yr 15, most ofthe North Pacific has negative SSTA except in thesouthern part of the subtropical gyre. Five years later,positive SSTAs appear in the southwestern and north-western North Pacific. Positive SSTAs are further de-veloped in the whole western North Pacific at yr 5. Atthe same time, some weak positive SSTAs appear inthe eastern NP. Positive SSTAs in the western and east-ern NP are further increased and expanded in the last5 yr before reaching the mature phase at lag 0. Theheat content anomaly is in phase with SSTA, sug-gesting propagation of SSTA downward into the ther-

mocline (figure not shown). This is because there ismainly one anomalous driving forcing, that is, surfaceheat flux.

To investigate the causes of decadal oscillation in E3,we calculated the combined EOFs between SSTA ten-dency and net surface heat flux, and horizontal advectionanomalies. Figure 10 shows the time series of thesecombined EOFs, which show that the EOF2 leads EOF1and that the heat flux modes (Fig. 11) lead the corre-sponding horizontal advection modes (Fig. 12). Thus,the horizontal advection is basically a response to thechange of SSTA forced by the surface heat flux. Detailedexamination reveals that the horizontal heat advectionby wave (V9 · =T) and gyre component (V ·=T9) arecomparable, with the former dominating in the centralNP, where gyre circulation is relatively weak.

The loading pattern of the two leading combined EOFmodes between SST tendency and surface heat flux areshown in Fig. 11. The upper (lower) panels are the 1st(2nd) EOFs. As expected, the surface heat flux anomalyis the major driving force in SST change. (Note thesefigures are not the correlation, their contours representtrue magnitudes.) We note that the spatial pattern of

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FIG. 9. The correlation between the time series of SSTA for E3 in Fig. 1 (dashed lines) and gridpoint SSTA for E3 at (a) lag 15; (b) lag10; (c) lag 5; and (d) lag 0. Dark (gray) indicates negative (positive) values.

EOF1 (EOF2) of SST tendency is similar (although notidentical) to those of SSTA during the mature (transient)phase shown in Fig. 9. Figure 12 shows the combinedEOF between SST tendency and horizontal heat advec-tion. The spatial patterns of the first two EOF modes ofSST tendency are similar to those in Fig. 11, and theyshow that horizontal advection mainly damps the SSTAexcept in some coastal regions (especially along theeastern and western coasts of the NP).

In summary, the decadal oscillation in E3 is mainlyheat flux driven, as expected, and is a stationary mode.Horizontal advection of SSTA drives the SST changein the western midlatitude North Pacific and, to a weakerextent, the eastern midlatitude North Pacific; however,it tends to be in the opposite phase to that of SST ten-dency in a large part of the central NP (away from theboundaries). The timescale of decadal variability drivenpurely by the net surface heat flux is about 40 yr, whichis about two times as long as E2 and E1, where thewind stress forcing mainly sets the timescale of decadaloscillation. The reason for longer timescale in E3 isassociated with the lack of Ekman transport, Rossby

wave propagation, and vertical mixing associated withwind stress forcing.

c. The effect of freshwater flux

In E4, a freshwater flux anomaly is added to E1. Wefound that the inclusion of the freshwater flux onlyslightly changed the amplitude of the decadal variability(Fig. 1d). Furthermore, it does not affect significantlythe timescale or the spatial pattern of SST evolution.Thus, freshwater flux may have a minor effect on thestrength of decadal variability but it does not affect thephasing of the variability. This is physically plausiblesince the major effect of freshwater flux is to compen-sate locally the effect of SSTA on seawater density.

6. Discussion

In the previous sections, we have shown that the NPdecadal variability can be simulated in a hybrid cou-pled model (HCM). The physics operating in the HCMmodel (the control run: with both wind stress and sur-

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FIG. 10. The time series of the combined EOFs (solid line: EOF1; dashed line: EOF2) forexperiment 3: (a) between SSTA tendency and net surface heat flux anomaly (Explained variance:EOF1: 78.4%, EOF2: 12.7%); (b) between SSTA tendency and horizontal heat advection anomaly(Explained variance: EOF1: 52.0%, EOF2: 22.2%).

face heat flux anomalies) were designed to be similarto that in the ECHO coupled model (LB94; LB96;X96). The spatial and temporal structures of the HCMare very similar to those from the ECHO coupled mod-el and the observations. Most importantly, the HCMgenerates sustained oscillations at decadal timescales.

There are two possible modes of variability in ourHCM. One is mainly controlled by wind forcing which

is described as a propagating mode. The other is a sta-tionary mode mainly driven by the heat flux anomaly.These two modes have different timescales. The winddriven oscillation has a period of about 20 yr while theheat flux driven oscillation has a period of about 40 yr.In the control run (which includes both wind and heatflux forcings), we find the oscillation timescale similarto that of wind forcing only. However, heat flux modifies

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FIG. 11. The spatial pattern of the combined EOFs between SSTA: tendency and net surface heat flux anomaly for E3. Dark (gray)indicates negative (positive) values.

the SSTA evolution and amplify the amplitude of SSTA.Freshwater flux is not important in NP decadal vari-ability. The HCM results are consistent with Miller etal. (1994, 1998, manuscript submitted to J. Climate)who used the observed wind stress and heat flux be-tween 1970 and 1988 to force an OGCM of the NPOcean.

There is room for future improvement in the OGCMused in this study. One improvement is to simulate stron-ger Kuroshio and midlatitude NP currents, and this mayrequire much higher resolution (i.e., much less diffusivemodels; cf. Jacobs et al. 1994). Also, the vertical mixingscheme and mixed layer physics should be improved asthey affect Ekman currents, vertical exchange, and ther-mocline depth (Sterl and Kattenberg 1994).

7. Conclusions

In this paper, we develop a hybrid coupled model(HCM) consisting of an oceanic general circulationmodel (HOPE) from the Max Planck Institute for Me-teorology and a statistical atmospheric model derived

from the 125-yr integration of the coupled general cir-culation model ECHO (Latif and Barnett 1994, 1996).

The hybrid coupled model is used to investigate thephysics of decadal variability in the North Pacific. It isshown that the HCM simulates decadal variability sim-ilar to that found in both the observations and coupledGCMs. In particular, the hybrid coupled model simulatesa self-sustained decadal oscillation, with a period ofabout 20 yr.

The sensitivity experiments indicate that the timescaleof the North Pacific decadal oscillation is mainly de-termined by wind stress forcing, and its amplitude canbe amplified or damped by surface heat and freshwaterfluxes, although the latter forcing is of secondary im-portance.

There are several important caveats in our study. Thenonstochastic atmosphere of the HCM may grosslyoversimplify reality. Therefore, the roles of stochasticforcing should be investigated in future studies. In ad-dition, some negative feedback is needed to run thecontrol experiment for an extended period. Until thisadditional physics is added to the HCM, we cannot

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FIG. 12. The spatial pattern of the combined EOFs between SSTA tendency and horizontal heat advection anomaly for E3. Dark (gray)indicates negative (positive) values.

explore the parameter space, especially the relativecoupling coefficients for wind stress and surface heatflux, where the oscillations appear to be self-sustaining.

Acknowledgments. We thank Drs. D. Cayan, S. Chen,M. Coe, C. A. Lin, Z. Liu, A. J. Miller, M. Morris, P.Niiler, D. Pierce, D. Rudnick, N. Schneider, S. Vavrus,W. White, and H. Zhang for helpful discussions. WXgreatly appreciate W. White for allowing us to use hisobservational results. It is a great pleasure to acknowl-edge the expert computational support of J. Ritchie, T.Tubb, and J. Soberani. Support is provided by the Officeof Global Programs of NOAA (NA 37GP0-518, NA47GP0-188) in concert with SIO/Lamont Consortiumon the Ocean’s Role in Climate. We greatly appreciatethe thoughtful comments by the two official reviewersand the editor.

APPENDIX

Spinup

We spun up the OGCM from the restart file at year100 taken from the ECHO run described in LB96,

Schneider et al. (1996), and Xu et al. (1996). We ex-perimented with different surface boundary conditionsfor SSS and SST. All the forcing fields were taken fromthe ECHO run, and the current OGCM is the same asthat in ECHO except for NP only. (We also tested thesame global OGCM but for a short time.) Intuitively,one would expect that the monthly mean SST and SSScould be reproduced by the monthly mean heat andfreshwater fluxes. So we first ran the ocean model withthe monthly mean wind stress, heat, and freshwater flux-es. We found that there was some drift of monthly meanSST from the ECHO results. The sponge layers usedhere at the edges of the coupled model basin shouldonly have had a very minor effect on the model results.Therefore, timescales shorter than one month (or otherunresolved physics) must be important in maintainingthe monthly mean SST and SSS in the ECHO run. In-deed, Miyakoda and Rosati (1984) and Rosati and Mi-yakoda (1988) also found that short timescale forcingshave some important effects on the long term mean SST.To eliminate the climate drift problem, we used bothmonthly mean SST, SSS, heat flux, and freshwater flux,as well as the monthly mean wind stress to drive the

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OGCM. The surface boundary conditions for SST andSSS can be written as

T 2 TA 1A T 5 HFLUX 1 (A1)HV z t R

S 2 SA 1A S 5 SFLUX 1 , (A2)HV z t R

where AHV is the vertical diffusivity coefficient; Tz andSz are the vertical temperature and salinity gradient inthe top level; HFLUX and SFLUX are the monthly meansurface heat and freshwater fluxes; TA and SA are themonthly mean SST and SSS taken from the ECHO run.The values of T1 and S1 are ocean temperature and sa-linity at the top level. The value of t R is the restoringtimescale, which was taken to be 15 days in the presentstudy. If the OGCM is perfect and HFLUX, SFLUX areidentical to the ECHO fluxes, then the second term inthe above equation should be 0 (Oberhuber 1993). How-ever, as we noted above, the OGCM produced differentresults from the ECHO. The addition of the second termsare used to keep the new SST (T1) and SSS (S1) closeto the monthly mean SST and SSS obtained from theECHO results.

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