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  • View in gallery
    Fig. 1.

    A section along 140°W from the background solution, illustrating the structure of the ocean model

  • View in gallery
    Fig. 2.

    Spatial patterns of the first four SVDs, showing ΔT1 (contours) and Δτ (arrows) patterns. Both fields are nondimensional

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    Fig. 3.

    Structure of the interannual solution at the peak of its warm phase, showing ΔT1 (contours) and Δτ (arrows) anomalies. Units for ΔT1 are 1°C

  • View in gallery
    Fig. 4.

    Phase (θ) evolution of Δd (contours) and Δv1 (vectors) for the interannual solution. Units for Δd are 1 cm

  • View in gallery
    Fig. 5.

    Phase (θ) evolution of Δd (contours) and Δv1 (vectors) for the decadal solution. Units for Δd are 1 cm

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    Fig. 6.

    Phase (θ) evolution of ΔT1 (contours) and Δτ (vectors) for the decadal solution. Units for ΔT1 are 1°C

  • View in gallery
    Fig. 7.

    Standard deviation of ΔT1 variability for the decadal solution averaged over one oscillation. Units are 1°C

  • View in gallery
    Fig. 8.

    Time series of dominant terms from Eq. (22) averaged over region W. The curves indicate total advection (ADV), total surface heat flux (QS), convective overturning (QC), the sum over all tendency terms (TOT), and ΔT1

  • View in gallery
    Fig. 9.

    Time series of dominant terms from Eq. (22) averaged over region E. The curves indicate total advection (ADV), total surface heat flux (QS), and the dominant terms that contribute to QS, namely, latent heat flux due to ΔW (LHW) and the rest of the latent heating due to ΔT1 (LHT), the sum over all tendency terms (TOT), and ΔT1

  • View in gallery
    Fig. 10.

    Phase (θ) evolution of Δd (contours) and Δv1 (vectors) for the decadal solution with air–sea feedback east of 180° (dashed line) suppressed. Units for Δd are 1 cm

  • View in gallery
    Fig. 11.

    Phase (θ) evolution of Δd (contours) and Δv1 (vectors) for the coupled run with air–sea feedbacks in the northeast and southwest quadrants suppressed and Δτ masked to the west of 180°. Units for Δd are 1 cm. Dashed lines denote quadrant borders

  • View in gallery
    Fig. 12.

    Time series of anomalies of M1(yd) (×), M2(yd) (○), E(yd) (thick dashed), W (dashed), and T1 (solid). Results shown are for (a) the decadal solution, (b) an ocean-only solution forced by winds from the decadal solution confined poleward of 20°N, (c) an ocean-only solution forced by winds at full strength equatorward of 20°N, and (d) the sum of the curves in (b) and (c). Units for M1, M2, E, and W are 1 Sv (1 Sv ≡ 106 m3 s−1), and for T1 are 1°C

  • View in gallery
    Fig. 13.

    Time series of T1 (thick dashed), NPI (thin dashed), and E(yd) (solid) in the coupled run with self-sustained interannual (ϕ1 = 1.3) and decadal (ϕo = 1.3) oscillations. Units for temperature and transport are 1°C and 0.5 Sv

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    Fig. 14.

    Time series of T1 (blue), and temperature anomalies in regions W (green) and E (red) in the coupled run with self-sustained interannual (ϕ1 = 1.3) and damped decadal (ϕo = 1.2) oscillations and stochastic forcing. Units are 1°C

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    Fig. 15.

    Time series of T1 (blue), and temperature anomalies in regions W (green) and E (red) in the coupled run with a self-sustained interannual (ϕ1 = 1.3) and stochastic forcing, but no decadal mode (ϕo = 0). Units are 1°C

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Interannual and Decadal Variability in an Intermediate Coupled Model of the Pacific Region

Amy SolomonInternational Pacific Research Center, University of Hawaii at Manoa, Honolulu, Hawaii

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Julian P. McCreary Jr.International Pacific Research Center, University of Hawaii at Manoa, Honolulu, Hawaii

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Richard KleemanCourant Institute, New York, New York

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Barry A. KlingerOceanographic Center, Nova Southeastern University, Dania Beach, Florida

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Abstract

Processes that cause decadal variability in an intermediate coupled ocean–atmosphere model of the Pacific basin, both at northern midlatitudes and in the Tropics, are studied. The model's ocean component is a variable-temperature 3½-layer system. Its atmospheric component consists of two basic parts: an empirical model, constructed from patterns obtained by the singular value decomposition (SVD) statistical technique that determines wind stress anomalies from model sea surface temperature (SST), and a simple representation of the planetary boundary layer to calculate the surface heat flux anomalies. A third part specifies stochastic wind stress forcing from observed variability. In addition, the model is specifically designed to separate tropical and extratropical interactions, such that the Tropics can force the extratropics through the atmosphere but the extratropics can only feed back to the Tropics through the ocean.

Solutions develop two types of oscillations: an ENSO-like interannual mode and a decadal mode. As in many models of ENSO, the interannual mode is driven by positive, ocean–atmosphere feedbacks near the equator, and time-delayed negative feedback is provided by off-equatorial Rossby waves. For parameter choices that amplify midlatitude coupling by 30% (ϕo = 1.3), a self-sustained decadal oscillation develops in the North Pacific without any tropical interactions. Diagnostic analyses show that it is maintained by ocean-to-atmosphere feedbacks in the northwest and subtropical northeast Pacific, and by atmospheric teleconnections from those regions to the northeast ocean. For weaker coupling (ϕo = 1.2), the decadal mode is damped. In this case, the mode can be sustained by atmospheric teleconnections from the Tropics associated with the interannual mode, but not by extratropical stochastic forcing. Although including stochastic forcing does generate variability at decadal timescales, a distinct decadal spectral peak only exists when the decadal mode is active.

Decadal variability is carried to the equator by variations in the transport, rather than temperature, of the North Pacific subtropical cell. These variations modulate near-equatorial SST by altering the amount of cool, thermocline water that upwells in the eastern equatorial Pacific, which in turn feeds back to the interannual mode.

+ Current affiliation: George Mason University, Fairfax, Virginia, and the Center for Ocean–Land–Atmosphere Studies, Calverton, Maryland

Corresponding author address: Dr. Amy B. Solomon, CIRES/Climate Diagnostics Center, University of Colorado, 216 UCB, Boulder, CO 80309-0216. Email: amy@cdc.noaa.gov

Abstract

Processes that cause decadal variability in an intermediate coupled ocean–atmosphere model of the Pacific basin, both at northern midlatitudes and in the Tropics, are studied. The model's ocean component is a variable-temperature 3½-layer system. Its atmospheric component consists of two basic parts: an empirical model, constructed from patterns obtained by the singular value decomposition (SVD) statistical technique that determines wind stress anomalies from model sea surface temperature (SST), and a simple representation of the planetary boundary layer to calculate the surface heat flux anomalies. A third part specifies stochastic wind stress forcing from observed variability. In addition, the model is specifically designed to separate tropical and extratropical interactions, such that the Tropics can force the extratropics through the atmosphere but the extratropics can only feed back to the Tropics through the ocean.

Solutions develop two types of oscillations: an ENSO-like interannual mode and a decadal mode. As in many models of ENSO, the interannual mode is driven by positive, ocean–atmosphere feedbacks near the equator, and time-delayed negative feedback is provided by off-equatorial Rossby waves. For parameter choices that amplify midlatitude coupling by 30% (ϕo = 1.3), a self-sustained decadal oscillation develops in the North Pacific without any tropical interactions. Diagnostic analyses show that it is maintained by ocean-to-atmosphere feedbacks in the northwest and subtropical northeast Pacific, and by atmospheric teleconnections from those regions to the northeast ocean. For weaker coupling (ϕo = 1.2), the decadal mode is damped. In this case, the mode can be sustained by atmospheric teleconnections from the Tropics associated with the interannual mode, but not by extratropical stochastic forcing. Although including stochastic forcing does generate variability at decadal timescales, a distinct decadal spectral peak only exists when the decadal mode is active.

Decadal variability is carried to the equator by variations in the transport, rather than temperature, of the North Pacific subtropical cell. These variations modulate near-equatorial SST by altering the amount of cool, thermocline water that upwells in the eastern equatorial Pacific, which in turn feeds back to the interannual mode.

+ Current affiliation: George Mason University, Fairfax, Virginia, and the Center for Ocean–Land–Atmosphere Studies, Calverton, Maryland

Corresponding author address: Dr. Amy B. Solomon, CIRES/Climate Diagnostics Center, University of Colorado, 216 UCB, Boulder, CO 80309-0216. Email: amy@cdc.noaa.gov

1. Introduction

Observational studies of decadal variability in the Pacific sector suggest that North Pacific decadal variability (PDV) and ENSO decadal variability (EDV) are related (Trenberth 1990; Latif et al. 1997; Kleeman and Power 1999). For example, the results of Wang (1995) suggest that concurrent with the 1970s “climate shift” in the North Pacific (Nitta and Yamada 1989; Trenberth 1990) there was an interdecadal change in the background state of the tropical Pacific that changed the onset of ENSO events, limiting predictability in coupled models (Ji et al. 1996). There is evidence that these conditions form part of a large-amplitude decadal variation in Pacific sea surface temperature (SST) extending back to the 1950s (Latif et al. 1997). At the present time, there is considerable debate as to the causes of both PDV and EDV. Are they generated at midlatitudes or the Tropics? Are they separate phenomena, or dynamically linked?

a. North Pacific decadal variability

One hypothesis for PDV is that it results from a self-sustained coupled mode of oscillation in the subtropics and midlatitudes. Such modes require a systematic relationship between oceanic and atmospheric variables. In the time-delay oscillator, for example, they result from ocean-to-atmosphere positive feedback in one region (region 1) with atmospheric teleconnections to another region (region 2); subsequently, atmosphere-to-ocean interactions in region 2 lead to negative feedback in region 1 via oceanic teleconnections, typically by the propagation of Rossby waves.

A mode of this sort is present in the solutions to a coupled general circulation model (GCM) reported by Latif and Barnett (1994, 1996). In these solutions, the mode appears to be generated by ocean-to-atmosphere feedback in the western North Pacific, which remotely influences the Aleutian low pressure system via atmospheric teleconnections. Anomalous winds associated with these pressure variations then generate oceanic Rossby waves that slowly propagate across the basin, eventually providing the negative feedback necessary to reverse the oscillation (Neelin and Weng 1999; Muennich et al. 1998). Latif and Barnett (1994, 1996) and Kleeman et al. (1999, hereafter KMK), who used an intermediate coupled model, concluded that positive feedbacks due to both wind stress and heat flux anomalies were important for the mode's excitation, whereas subtropical gyre adjustment and advection (both of which have decadal timescales) were likely responsible for determining its period. Pierce et al. (2000b), using a coupled GCM, concluded that coupled ocean–atmosphere modes were important for determining the strength and frequency of decadal variability in the Kuroshio Extension region.

Such relationships have so far been difficult to detect observationally in the North Pacific, due to the shortness of the available records and to the presence of large-amplitude, high-frequency (periods less than 1 yr) atmospheric variability. Indeed, a number of studies suggest that at high frequencies the North Pacific is predominantly forced by the atmosphere; they include analyses based on lagged cross correlations between observed SST and atmospheric variables (e.g., Davis 1976; Frankignoul 1985; Deser and Timlin 1997) and modeling studies using thermodynamic models, both 1D systems (e.g., Hasselmann 1976; Barsugli and Battisti 1998; Frankignoul 1999) and AGCMs coupled to mixed-layer oceans (e.g., Bladé 1997). As discussed next, however, there are studies of low-frequency variability that support various aspects associated with coupled modes.

Several studies point toward the existence of ocean-to-atmosphere coupling in one region with atmospheric teleconnections to another. Nakamura and Izumi (2002) found that warm interannual-to-decadal atmospheric temperature anomalies at the top of the planetary boundary layer (PBL) in the northwest Pacific (Kuroshio Extension region) are associated with enhanced storm track activity and a weakening of the Aleutian low. Nakamura et al. (1997) and Nakamura and Yamagata (1999) reported two modes of North Pacific decadal variability based on an empirical orthogonal function (EOF) analysis of low-pass SST data in the northwest Pacific. Atmospheric and SST fields throughout the basin were then obtained by regression with the time series for each EOF. The SST field associated with the first EOF (EOF1) was confined to midlatitudes, with most of its amplitude centered on the subarctic front. In contrast, the SST pattern corresponding to the second EOF (EOF2) extended over much of the basin; in northern subtropics and midlatitudes, it had a distinctive dipolelike structure, with anomalies of opposite sign on either side of the subtropical front, and it also had significant amplitude throughout the Tropics in both hemispheres. To investigate where the atmospheric circulations associated with each mode were forced, Nakamura and Yamagata (1999) determined the wave-activity flux, W, of stationary Rossby waves on the climatological mean flow based on 500-hPa geopotential height anomalies. For EOF1, W was divergent in the central North Pacific in the latitudinal band of the storm track and the subarctic front, whereas for EOF2 it was divergent in the eastern North Pacific above the subtropical front (see Fig. 4 of Nakamura and Yamagata 1999), indicative of external forcing by SST anomalies in each region. In both cases, the predominant direction of the flux vectors was from the divergent regions into the northeast Pacific, suggestive of atmospheric teleconnections into that area.

Recently, Nonaka and Xie (2003) reported evidence of direct ocean-to-atmosphere interaction in the region of the Kuroshio, both south of Japan and its extension into the North Pacific. The authors analyzed SST and wind stress data from satellite microwave measurements, finding that increased (reduced) wind speeds are associated with warm (cold) SST anomalies (SSTAs), that is, the two fields are positively correlated. They concluded that warm SSTAs strengthen the surface winds by reducing the static stability of the PBL, and vice versa. Specifically, an increase in SST intensifies vertical turbulence, thereby mixing stronger winds from aloft to the sea surface. The authors note that this result contrasts with the negative SST–wind correlations that are often observed in regions of weak currents, such as in the North Pacific south of the Aleutian low, the negative relationship considered to be indicative of atmosphere-to-ocean forcing. It is noteworthy that a similar mechanism has been invoked to account for positive SST–wind correlations in the Southern Ocean (O'Neill and Chelton 2002, manuscript submitted to J. Climate).

There is also observational support that remotely forced oceanic Rossby waves account for a significant amount of decadal variations in the Kuroshio Extension region (Deser et al. 1999; Miller and Schneider 2000), since they cannot be explained by contemporaneous local forcing (Xie et al. 2000). Moreover, Schneider and Miller (2001) used a simple, linear, Rossby wave equation forced by observed wind stress curl to demonstrate that SSTs in the western North Pacific can be skillfully predicted at lead times of up to 3 yr. The mechanisms responsible for generating the Rossby waves is not yet known.

The lack of strong observational support for a well-defined decadal oscillation in the North Pacific motivated Barnett et al. (1999) and Schneider et al. (2002) to conclude that the decadal variability in their coupled GCM was generated by stochastic wind stress variability, rather than by a self-sustained coupled mode. Weng and Neelin (1999) came to a similar conclusion based on solutions to their intermediate midlatitude coupled model. It is not yet clear, however, just how effective stochastic forcing is in driving the large-scale changes noted previously.

b. ENSO decadal variability

Several mechanisms have been proposed for the generation of EDV. They include nonlinearities in ocean–atmosphere coupling within the Tropics (e.g., Timmermann and Jin 2002), ENSO-like ocean-to-atmosphere positive feedback with time-delayed negative feedback provided by subtropical Rossby waves (e.g., Knutson and Manabe 1998; Yukimoto et al. 2000), atmospheric teleconnections from midlatitudes to the Tropics (e.g., Barnett et al. 1999; Pierce et al. 2000a), and oceanic teleconnections from the subtropics to the equator by variations in western boundary current transports (Lysne et al. 1997).

Two other oceanic mechanisms involve variations in the temperature (Gu and Philander 1997) or transport (KMK) of the Pacific subtropical cells (STCs). The STCs are shallow (z ≲ −500 m) meridional circulation cells in which water flows out of the Tropics within the surface layer, subducts in the subtropics, flows equatorward within the thermocline, and upwells in the eastern equatorial ocean (Bryan 1991, see his Fig. 2; McCreary and Lu 1994; Liu et al. 1994; Blanke and Raynaud 1997; Rothstein et al. 1998; Lu et al. 1998).

Gu and Philander (1997) hypothesized that North Pacific SST anomalies are subducted into the thermocline to join the north STC, and are subsequently advected to the equatorial Pacific with a time lag of the order of a decade, thereby providing a delayed negative feedback (the vT′ hypothesis). This idea received observational support from Deser et al. (1996), who were able to follow the equatorward movement of a subsurface anomaly for some distance. Recent solutions using oceanic GCMs, however, suggest that most of this subtropical signal recirculates in the subtropical gyre, with little ever reaching the equator (Schneider et al. 1999; Nonaka et al. 2000). As proposed by Gu and Philander (1997), then, the STC pathway may not provide a sufficiently strong interaction to account for ENSO decadal variability.

KMK used an intermediate coupled model to study PDV and EDV. Their solutions developed two modes of oscillation: an ENSO-like interannual mode (∼4 yr) and a decadal one (∼13 yr). The decadal mode was generated in northern midlatitudes, and was similar in structure to the Latif and Barnett (1994) decadal mode. It was found to influence the equatorial cold tongue by altering the transport of the ocean model's northern STC, thereby modulating ENSO on decadal timescales (vT′ hypothesis). The STC transport was determined largely by the Ekman transport across the edge of the tropical warm pool, thereby linking subtropical wind variability to equatorial SST anomalies. These ideas are supported by the modeling study of Nonaka et al. (2002); in their wind-driven solutions, there is a close connection between equatorial SST anomalies and subsurface heat transports across 11°S and 15°N at decadal timescales. They are also supported by the observational study of McPhaden and Zhang (2002), who suggest that the STC has been spinning down since the 1970s, reducing the amount of cold water that upwells in the Tropics and hence increasing equatorial SST.

c. Present research

In this paper, we investigate the causes of PDV and EDV in an updated version of the KMK intermediate coupled model. Our purpose is to explore further the processes that might be involved in generating PDV, and in communicating that variability into the Tropics to cause EDV. The coupled model is described in detail in section 2. Its ocean component is a version of the 3½-layer, reduced-gravity model developed by Lu et al. (1998) that allows layer temperatures to vary. Its atmospheric component consists of an empirical model based on the SVD statistical technique that generates wind stress anomalies from SST anomalies, a simple model of the planetary boundary layer that provides the heat flux forcing for the ocean, and externally prescribed forcing by stochastic wind stress.

Essential parts of the empirical model are structure functions that specify regions 1 (θk ≠ 0) and 2 (θk = 0) where ocean-to-atmosphere coupling is active and absent, respectively. The functions are specified to eliminate atmospheric teleconnections from the extratropics to the Tropics, so that the only means for such communication is through the oceanic North Pacific STC [section 2c(1)v]. They are varied in a series of test runs in order to identify key regions of ocean-to-atmosphere coupling in the North Pacific [section 4a(4)]. They also allow atmospheric teleconnections to be defined in the model, namely, as an atmospheric response in region 2 generated by coupling in region 1.

As we shall see, for sufficiently large coupling coefficients the model can separately develop two self-sustaining modes of oscillation: a tropical interannual mode (section 3) and a midlatitude decadal one (section 4). We discuss in detail the feedbacks that maintain the latter oscillation, demonstrate that it can generate EDV by changes in the STC transport (section 4a) and describe solutions with stochastic forcing (section 4c). Finally, we discuss solutions in which both oscillations simultaneously exist (section 5); interestingly, there is a parameter range in which an otherwise damped decadal oscillation is sustained by atmospheric teleconnections from the Tropics.

2. The coupled model

a. Model ocean

Most of the equations of motion for the ocean model are provided in Lu et al. (1998), and so only model details relevant to this study are discussed here. Relevant aspects of the model's STC dynamics are also reviewed.

Figure 1 schematically illustrates the structure of the coupled ocean–atmosphere model. The ocean model consists of three active layers with thicknesses hi, velocities vi and temperatures Ti (i = 1, 2, 3 is a layer index), overlying a deep, inert layer of temperature T4 = 3°C where the pressure gradient field is assumed to vanish. Each of the layers corresponds primarily to a single water mass type, namely, surface water, thermocline water, and upper-intermediate water in layers 1, 2, and 3, respectively. The across-interface velocities, w1 and w2, allow water to transfer between layers, and they represent all the model's vertical mixing processes (Lu et al. 1998). Heat and momentum are conserved during such transfers.

Temperatures Ti are allowed to vary within each layer. They are determined by integrating the equation,
i1520-0442-16-3-383-e1
where ρo = 103 kg m−3, cpo = 4187 J kg−1 K−1, δi1 is the Kronecker δ-symbol, w+i = max(wi, 0), wi = min(wi, 0), and w0 = w4 = 0. From left to right, the terms represent the rate of change of temperature Tit due to horizontal advection, surface heat flux into the ocean Qo, heat flux due to convective overturning Qc, Laplacian and biharmonic mixing with coefficients κ2 = 2 × 107 cm2 s−1 and κ4 = 2 × 1021 cm4 s−1, and vertical mixing from above and below. The formulation of the last two terms ensures that vertical mixing conserves heat, Qo is specified below in Eqs. (4), (12), (19), and Qc is determined as in McCreary and Lu (1994).
For our purposes, w1 is the important mixing velocity since it determines the locations of the ascending and descending branches of the model STCs. The primary processes that contribute to w1 are upwelling we and subduction ws. According to the Kraus–Turner (1967) model, wind stirring entrains (upwells) water into the mixed layer whenever it becomes sufficiently thin. We parameterize this process by
i1520-0442-16-3-383-e2a
where He = 50 m, te = 1 day, and S is a step function (McCreary and Kundu 1988). We parameterize detrainment (subduction) by
i1520-0442-16-3-383-e2b
where Hs = He and ts = te. Subduction is confined primarily to the subtropics where there is a strong meridional SST gradient, and to represent this property we suppress detrainment equatorward of latitudes ±yd, where yd = 18° (McCreary and Lu 1994). Thus, these “subduction cutoff latitudes” define the boundaries between the subtropics and Tropics in our model. According to (2a) and (2b), h1 necessarily remains close to He poleward of ±yd, and so simulates a mixed layer of nearly constant thickness.
In solutions forced by steady winds, a measure of the strength of the northern (southern) STC is the zonally integrated surface-layer meridional transport,
i1520-0442-16-3-383-e3
where y′ = ±yd, and xw(y′) and xe(y′) are the longitudes of the western and eastern boundaries of the basin (McCreary and Lu 1994; Lu et al. 1998). These transports drain warm surface (layer-1) water from the Tropics, and the resulting mass loss is necessarily balanced by an upwelling transport of cool thermocline (layer-2) water near the equator W, and the convergence of layer-2 water M2(y′).

McCreary and Lu (1994) showed that much of M1(y′) is determined by the Ekman transport E(y′). Thus, the model contains an explicit process by which subtropical zonal winds, τx(x, y′), affect the amount of thermocline water that upwells along the equator. Note that STC strength is not determined by midlatitude wind stress curl, as might be expected. It is true that an increase in midlatitude wind curl does increase subduction by a proportionate amount, but the additional subducted water can recirculate within the subtropical gyres and need not flow into the tropical ocean. It will do so only if the wind curl anomaly also acts to increase the Ekman divergence out of the Tropics, according to (3).

When the winds are not steady, the simple notion of a closed STC in which M1(y′) = W = M2(y′) breaks down. Klinger et al. (2002) recently explored time variability of the STC by forcing the KMK ocean model with various switched-on and oscillatory, idealized wind stress fields. They found that M2(yd) lagged M1(yd) by up to 5 yr, a consequence of the slow geostrophic adjustment of the thermocline by wave propagation. As we shall see, however, the steady-state concepts still help in the interpretation of our decadal solutions (section 4b).

b. Background state

To determine the background state for the coupled solutions, the ocean model is first spun up to equilibrium using annual-mean Hellerman and Rosenstein (1983) wind stress, τ*, multiplied by a factor of 0.7 since these winds are believed to be too strong in the Tropics (Harrison 1989), and a surface heat flux Qo given by
i1520-0442-16-3-383-e4
where H1 = 100 m, th = 30 days, and T* is the annual-mean SST field from Reynolds and Smith (1994). This solution is spun up for 100 yr or more, by which time it has adjusted close to equilibrium. The resulting SST field, T1, provides the background SST field for the atmospheric model. The background wind and heat flux fields are τ* and Qr(T1).

Other background fields needed by the model atmosphere are wind speed W* and air temperature Ta. The W* field is the annual-mean wind speed field from the Comprehensive Ocean–Atmosphere Dataset (COADS). The Ta field is determined by solving (14) with T1 in the equation for Qs, (13b), replaced by T1.

c. Model atmosphere

The model atmosphere consists of two basic parts: an empirical model that produces wind stress anomalies Δτ from model SST anomalies ΔT1 = T1T1, and a boundary layer model that generates heat flux anomalies ΔQ and ΔT1, Δτ, and air temperature anomalies ΔTa. A third part specifies stochastic wind stress forcing from observed wind stress variability.

1) Empirical model

The empirical model is constructed from simultaneous relationships between observed wind stress and SST anomalies determined by the singular value decomposition (SVD) statistical technique. The advantage of this approach is that it builds observed patterns of ocean–atmosphere variability directly into the system. Its limitation is that cause and effect are confused, since the model explicitly assumes that wind stress patterns are always generated as a response to SST anomalies. To address this limitation, we include structure functions θk, defined later in Eqs. (8) and (11), to suppress ocean-to-atmosphere interaction in specific regions. Section 2c(1)ii provides a general discussion of the issue, focusing on our use of simultaneous, rather than lagged, SVDs.

(i) SVDs

The datasets used to calculate the SVDs are monthly Global Sea Ice and Sea Surface Temperature (GISST) data for SST (Parker et al. 1994) and monthly COADS data for wind stress (as analyzed and corrected for biases by da Silva et al. 1994a,b) for the 40-yr period from 1949 to 1989. The data are interpolated from a 1° × 1° grid onto a 5° × 4° grid, and the domain is the Pacific basin from 55°S to 55°N.

The SVDs are calculated following Bretherton et al. (1992). Let S(t) be the observed SST anomalies and W(t) be the observed zonal and meridional wind stress anomalies, both written as column vectors at N spatial grid points. The covariance matrix between these two fields is defined as
StWTt
where the operator 〈q〉 denotes the time average of q(t), and the transpose operation is denoted by a superscript T. Note that, since W has dimension 2N, the dimension of 𝗖 is N × 2N.
The SVD technique represents 𝗖 in the form
i1520-0442-16-3-383-e6
where lk and rk are eigenfunctions of (𝗖𝗖T)lk = σ2klk and (𝗖T𝗖)rk = σ2krk, normalized so that lTjlk = rTjrk = δjk. The eigenvalues σ2k are the total squared covariance explained by each eigenfunction pair, and, for convenience, they are ordered from the largest (σ21) to smallest (σ2N) value. We refer to lk and rk as patterns for observed SST and wind stress anomalies, respectively, associated with the kth eigenvectors (SVDk). In addition, rk can be divided into two parts (in the same order that W was constructed), yielding patterns for zonal and meridional wind stress anomalies, rxk and ryk.

Figure 2 displays the first four SVDs determined from monthly mean data, which contain 51%, 9%, 5%, and 4% of the squared covariance, respectively. SVD1 captures the ENSO interannual variation, having a large amplitude in the equatorial region and a teleconnection pattern to midlatitudes (Alexander 1992; Deser and Blackmon 1995; Lau and Nath 1996). SVD2 has a broad SST minimum in the central North Pacific, with southeasterly wind stress in the eastern ocean; it is very similar to the preferred spatial pattern of internal atmospheric variability found in observations [section 2c(3)] and in stand-alone atmospheric GCMs forced by fixed SSTs (see, e.g., Fig. 15 in Neelin and Weng 1999), and closely resembles one of the SVDs determined from wind stress and SST tendency [section 2c(1)ii]. SVD3 consists of an anticyclone in the eastern North Pacific, with a prominent zonal-wind component in the subtropics (10°–30°N) across much of the basin; SST/wind stress patterns similar to SVD3 developed in the coupled GCM of Latif and Barnett (1994, 1996), and the wind pattern resembles the response of an atmospheric GCM coupled with a slab ocean model to an imposed SST perturbation in the Kuroshio Extension region (Yulaeva et al. 2001). Prominent features of SVD4 are similar to the negative of those in SVD3, but they are shifted poleward by about 10° and westward by about 30°. Modes 5–7 predominantly have a midlatitude, large-scale character, and the higher-order modes exhibit small-scale (noisy) structures.

(ii) Discussion

A number of studies have demonstrated that simultaneous cross correlations between SST and atmospheric variables can result from prior forcing by atmospheric noise (e.g., Frankignoul 1985; correspondence between Frankignoul, 1999, and Barnett and Latif, 1999, 2000). If our SVDs are determined solely by this mechanism, then their patterns result entirely from atmosphere-to-ocean processes and there is a fundamental inconsistency with the formulation of our empirical model. Here, we report on additional sets of SVDs that we obtained to investigate this issue, and to explore how to minimize the influence of atmospheric noise in our model.

We obtained sets of SVDs using data that were temporally averaged by J-month running-mean filters (with J = 3, 5, and 7) and seasonally stratified, centered on either January or July. For each J, the first four wintertime SVDs are all very similar to the monthly mean SVDs shown in Fig. 2, whereas the summertime SVDs are not. (Differences between corresponding patterns in the monthly mean and wintertime SVDs are largely attributable to the influence of summertime variability in the monthly mean SVDs.) Thus, the monthly mean SVDs capture patterns of wintertime variability that can persist for up to 7 months and vary interannually. Averages of 7 months would be expected to enhance correlations due to ocean-to-atmosphere feedbacks relative to atmosphere-to-ocean feedbacks, which decorrelate on timescales less than 10 days.

We also obtained lagged auto- and cross correlations of the SST and wind stress time series for each SVD [sk and wk defined in (9) below]. Cross correlations for all the wintertime SVDs except SVD3 and SVD4 fall off rapidly, becoming zero at lags close to ±1 yr. In contrast, the cross correlations for wintertime SVD3 and SVD4 become zero at lags of about ±2 yr, remain negative until ±10 yr, and attain relative minima between about ±6 and ±8 yr. Thus, the wintertime SVDs 3 and 4 are associated with decadal variability with a period of 12–16 yr. The cross correlations for SVD3 at a lag of −8 yr exceeds the 99% significance level based on a Student's t test. The decadal signal is also seen in the cross correlations for monthly mean SVD3 when only wintertime data is considered.

To help identify prominent patterns of atmosphere-to-ocean forcing during winter, we obtained sets of SVDs (labelled SVDk′) between wind stress W(t) and SST tendency, ΔS(t) ≡ S(t + n) − S(tn), where t is January and the overbar designates smoothing by a 3-month running-mean filter. Atmosphere-to-ocean forcing is expected to be predominant in regions where SVDk closely resembles SVDk′; conversely, ocean-to-atmosphere feedback may be active in regions where they differ (Wallace et al. 1990; Deser and Timlin 1997). The resulting SVDs are almost unchanged for n = 1, 2, and 3 months. SVD1′ is similar to SVD1 in Fig. 2 north of 20°N but the sign of the SST anomaly is reversed in the equatorial band, consistent with the existence of ocean-to-atmosphere forcing in the Tropics and atmospheric teleconnections to midlatitudes. SVD2′ resembles SVD2 in Fig. 2 north of 10°N and is weak elsewhere, and it is even more similar to SVD2 determined from J = 3 wintertime data. SVD2′ is also similar to the dominant North Pacific SST-tendency modes reported by Wallace et al. (1990) and Deser and Timlin (1997). We conclude that SVD2 is largely determined by atmosphere-to-ocean forcing, and for this reason do not include it in the model atmosphere [section 2c(1)v]. SVD3′ does not resemble SVD3 at all, particularly in the northwest Pacific where SVD3′ is weak and SVD3 is strong. SVD4′ is concentrated in the eastern and central North Pacific, with little amplitude in the northwest ocean. That SVD3 does not resemble either SVD3′ or SVD4′ thus allows for the possibility that it is influenced by ocean-to-atmosphere coupling, particularly in the northwest region.

Finally, we explored the use of lagged SVDs, in which SST leads the atmospheric variables by n months, as a means for removing the effects of atmospheric noise from the model atmosphere. Although the method is physically appealing, it is problematic from the view point of time series analysis, since the use of n-month lagged data alone is not a good filter of n-month noise. Despite this reservation, we constructed a version of the coupled model using SVDs determined when winds lagged SST by n = 1 month (lag-1 SVDs). SVD1 was not much changed from its lag-0 counterpart, but SVD3 and SVD4 were. As a result, the coupled solution was able to generate a self-sustaining decadal oscillation only when the amplitude factor ϕo (defined below) was increased to 4.0. The weakening of the decadal mode in this solution could have resulted from elimination of spurious atmosphere-to-ocean feedbacks in the system. It may also have occurred because high-frequency noise was aliased into the structures of SVD3 and SVD4, a conclusion supported by the similarity between the lag-0, monthly mean, and wintertime SVDs noted earlier.

(iii) Specification of Δτ
We assume that model wind stress and SST anomalies are related just as in the observed SVDs. Let Δτa(xi, yj, t) represent the model wind stress anomaly at time t and observational data point (xi, yj), where superscript a is either x or y to denote the zonal or meridional wind component. There are Nx grid points in the zonal direction, Ny grid points in the meridional direction, and N = NxNy. We then synthesize Δτa(xi, yj, t) from the series of observed wind stress SVDs, rak(xi, yj), according to
i1520-0442-16-3-383-e7
where
i1520-0442-16-3-383-e8
is the projection of the model SST anomaly ΔT1(xi, yj, t) onto lk(xi, yj) modified by the structure function θk, N is the number of SVDs retained in the model, and ck is the coupling coefficient that links the temperature and wind stress patterns associated with SVDk [section 2c(1)iv]. To be used by the ocean model, Δτa must be interpolated onto the model grid at each time step of the integration; likewise, to evaluate (8) ΔT1 must be interpolated onto the observational grid.

The structure functions, θk(xi, yj) and ϕk(xi, yj), are specified to limit the area over which ocean-to-atmosphere and atmosphere-to-ocean coupling occurs, respectively [section 2c(1)v]. In so doing, θk can artificially weaken ak(t), and the factor in the denominator of (8) is included to compensate for this tendency.

(iv) Coupling coefficients
Time series of expansion coefficients for the temperature and wind stress patterns associated with SVDk are
sktlTkSwktrTkW
respectively. The two time series are similar, but not identical, the cross correlation between them being 〈skwk〉/(〈w2k1/2s2k1/2). If we seek a best-fit relationship of the form wk = cksk, then a least squares analysis yields
i1520-0442-16-3-383-e10
for the coupling coefficient between wk and sk. It is worth noting that other choices for ck have been used in previous studies; for example, Neelin and Weng (1999) and KMK set ck = 〈w2k1/2/〈s2k1/2, which yields significantly larger coefficient values than (10) does.
(v) Specification of N, θk, and ϕk

We carried out a large number of test runs to determine appropriate structure functions and a value for N. To simplify the model dynamics, we seek to use as few SVDs as possible. Solutions with N = 3 were not able to develop a decadal oscillation. Solutions for N ≥ 4 are all very similar to each other, their interannual and decadal oscillations virtually unchanged. Furthermore, this property also holds when SVD2, which is likely to be determined mostly by atmosphere-to-ocean forcing [section 2c(1)ii]. is dropped from the model atmosphere.

Based on these tests, as well as our analyses of SST-tendency SVDs [section 2c(1)i], unless specified otherwise we take N = 4 and choose θk and ϕk for k = 1 and 2 to be
i1520-0442-16-3-383-e11a
and for k > 2 to be
θkSyϕkϕoSy
where ϕo = 1.3. With these choices for θk, the denominator of (8) has the values 0.61, 0.64, and 0.66 for k = 1, 3, and 4, respectively. Solutions for other choices of θ3 and θ4, which subdivide the North Pacific into separate quadrants, are discussed in section 4a(4).

As noted above, SVD1 clearly represents variability associated with ENSO. It is generally accepted that ENSO is driven by ocean-to-atmosphere interactions confined near the equator, which in turn cause atmospheric teleconnections from the Tropics to the extratropics (e.g., Lau and Nath 1996). The choices for θ1 and ϕ1 in (11a) build in both of these properties. The choices for θk and ϕk in (11c) specify that all ocean-to-atmosphere coupling is confined poleward of 12°N, and that there are no atmospheric teleconnections back to the near-equatorial band. The differences between (11a) and (11c) allow a clean separation in the model atmosphere between near-equatorial and extratropical coupling, and as we shall see the two parts generate interannual and decadal oscillations, respectively.

Setting ϕo = ϕ1 = 1.3 effectively strengthens coupling in the model by 30%. We chose this value for our main run because it is slightly above the minimum value that allows the system to develop self-sustaining interannual and decadal oscillations. A possible reason that an increase is required for ϕ1 is that the tropical coupling associated with ENSO is not entirely contained in SVD1, some of it being spread into SVD2 and SVD3 (Fig. 2). A similar spreading may account for the need to increase ϕo. On the other hand, both modes of oscillation may be damped (Thompson and Battisti 2000; Barnett et al. 1999; Schneider et al. 2002), and so we report solutions for smaller values of ϕo and ϕ1 as well.

2) Atmospheric boundary layer model

The atmospheric boundary layer model determines the anomalous heat flux ΔQ into the ocean as a function of T1, boundary layer air temperature Ta, and wind speed W. It is given by
QQT1TaWQT1TaW
where
QQsQlQlw
Qlw is outgoing longwave radiation, which is a function of T1 and surface humidity as parameterized in Kleeman and Power (1995),
QsacpCsTaT1
is the sensible heat flux, and
QlacpCEqaqsT1
is the latent heat flux. Note that Q does not involve shortwave radiation fluxes, Qsw, so that the model neglects feedback of T1 onto cloud cover. In Qs and Ql, Cs and CE are drag coefficients (evaluated following Large and Pond 1981, 1982), ρa is the density if surface air set equal to 1.3 kg m−3, and cp = 1004.64 J kg−1 K−1 is the specific heat of the atmosphere. The specific humidity of the air is taken to be qa = rqs (Ta), where r is the relative humidity set equal to 0.8, and qs is the saturation specific humidity.
Air temperature Ta is determined by integrating the equation
i1520-0442-16-3-383-e14
where κa = 3 × 106 m2 s−1 following Kleeman and Power (1995), and H = 1 km is the thickness of the planetary boundary layer (assumed constant). Including diffusion in the model allows a physically realistic scale-dependent heat flux response to SST anomalies (see Kleeman and Power, 1995, for further discussion of this point). Including sensible heat fluxes allows for the rapid adjustment of boundary layer air temperature to changes in SST. Test runs with a more sophisticated atmospheric boundary layer model indicated that these were the dominant processes that needed to be considered in our anomaly coupled model. The equation is solved over the model domain. Over land the lower boundary temperature is fixed to climatology.
The wind speed that is used to calculate Qs and Ql is
WWW,
where the wind speed anomaly ΔW is determined from Δτ according to
i1520-0442-16-3-383-e16
τ = τ* + Δτ, Cd = 1.4 × 10−3, and ρa = 1.3 kg m−3.

3) Stochastic forcing

For some of the solutions reported in sections 4c and 5, a stochastic wind stress anomaly Δτ′ in the North Pacific is included as a part of the wind stress anomaly Δτ that forces the model. It is determined from W according to
i1520-0442-16-3-383-e17
where ei is an EOF of W in the region north of 12°N, wi(t) is the principal component of ei, and bi(t) is a time series of random numbers with 〈b2i1/2 = 1 that is varied every 30 days. The first 40 EOFs explain 99% of the variance of W, and EOF1 closely resembles the wind stress pattern of SVD2 (Fig. 2). Thus, Δτ′ is a representation of observed atmospheric variability north of 12°N on timescales of 30 days and longer.

d. Coupling

In the coupled model, the ocean model passes T1 to the atmospheric model, and the atmospheric model returns τ and Qo. The total wind stress field that drives the ocean model is
τττ
and the total heat flux is
QoQrT1Q.
Note that when T1 = T1, and there is no externally imposed stochastic forcing Δτ′, τ and Qo reduce to the forcing fields for the background state as they should.

e. Numerics

The model basin is an idealized representation of the Pacific basin from 55°S to 55°N. The ocean model uses a standard Arakawa C-grid with a resolution of Δx = 1°, Δy = 0.5°, and the equations of motion are integrated forward in time with a time step of Δt = 72 min. The time step used for Eq. (14) is 24 min, so that it is called 3 times for each ocean model time step. Initial layer thicknesses are H1 = 50 m, H2 = 150 m, and H3 = 450 m. As the integration proceeds, layer thicknesses vary but total mass (summed over all layers) does not.

Both the background integrations and the anomaly coupled integrations are run for at least 100 model years. The model is computationally very efficient, which made it possible to carry out many (literally hundreds) test runs.

3. Interannual solutions

To investigate the basic dynamics of the model's interannual mode, we isolate it by retaining only SVD1 in the model atmosphere, that is, by setting N = 1 in (7). For the model parameters listed in section 2c, the system then develops only an interannual oscillation with a period of 4.3 yr, and, according to (11a), it exists independent of extratropical (|y| > 12°N) feedbacks.

Figure 3 shows ΔT1 and Δτ at the peak of the warm phase of the interannual oscillation. (Since N = 1, Δτ is just a replot of the wind vectors in SVD1 in Fig. 2a.) The pattern is dominated by SST anomalies in the Niño-3.5 (5°S–5°N, 180°–120°W) region, consistent with the peak of an ENSO event. Unlike observed ENSO, however, SST anomalies in the eastern equatorial ocean have an opposite sign to those in Niño-3.5. This difference is likely due to SVD1 not completely representing ENSO wind variability, as equatorial wind anomalies are associated with the other SVDs as well (Fig. 2). There is also a significant extratropical response, due to atmospheric teleconnections, with about half the observed amplitude.

Model sea level is given by
dαT1T4h1T2T4h2T3T4h3
where α = 0.00025°C−1 is the temperature expansion coefficient. Figure 4 plots sea level anomalies (Δd = dd where d is the sea level of the background state) and layer-1 current anomalies (Δv1) over half of the primary cycle; the other half (corresponding to phases θ = 180°, 225°, 270°, and 315°) essentially being the negative images of corresponding panels in the figure. The phase θ = 0° is chosen to coincide with maximum equatorial ΔT1. Figures 4a and 4b, θ = 0° and 45°, respectively, show the expected response to equatorial westerlies confined in the central Pacific: There is an upward tilt to the east along the equator to balance the wind, regions of shallow Δd on either side of the equator driven by Ekman suction, and an eastward equatorial current associated with anomalous downwelling near 135°W. Figure 4 also exhibit westward propagation of off-equatorial Δd: Regions of positive off-equatorial Δd that appear near 140°W at θ = 0° shift westward from θ = 45° to 135°, and they reach the western boundary at θ = 180° where they are intensified by the near-equatorial winds.

All the expected features of the ENSO time-delayed oscillator are therefore present in the solution. The essential aspect of this paradigm is that the wind stress anomalies that are responsible for the amplification of an ENSO event also lead to its demise (so that regions 1 and 2 are in close proximity): They excite off-equatorial Rossby waves that reflect at the western boundary as equatorial Kelvin waves, which subsequently trigger negative ocean-to-atmosphere feedbacks in the eastern and central oceans. In our solution, evidence for this reflection is the region of −Δd in the eastern, equatorial ocean from θ = 0° to θ = 90°, a period of time when wind anomalies predominantly have a westerly component along the equator (the exception being the weak easterlies in the eastern ocean): Because the equatorial ocean is close to equilibrium at a period of 4.3 yr, the layer-1 pressure change along the equator (a close proxy to the change in d) is given by p1e = p1w + (1/g) xexw (τx/h1) dx, where p1e and p1w are the pressures at xe and xw, respectively; since the the integral is positive, the only way p1e can be negative is for p1w to be even more negative, which can only result from remote forcing. The region of −Δd is associated with a westward equatorial current that advects cool water westward, weakening the warm T1 anomaly in the Niño-3.5 region and leading to the termination of the model ENSO by weakening the positive projection of ΔT1 onto SVD1.

With ϕ1 = 1.3, the interannual signal is thus self-sustaining. When ϕ1 is increased to 1.4, the amplitude of the oscillation is increased, but its period and horizontal structure do not change. When ϕ1 is reduced to 1.2, however, the oscillation is damped and the solution eventually adjusts to a steady state.

4. Decadal solutions

In this section, we isolate the decadal mode by deleting SVD1 from the model atmosphere, by starting the sum in (7) at k = 3. For the model parameters of section 2c, the solution develops a self-sustained decadal signal, with a primary peak at 12.8 yr and a secondary one at 6.4 yr, which, according to (11c), is necessarily generated by extraequatorial processes in the North Pacific (y > 12°N). For convenience, we refer to this solution as the main run. We first describe the response of the main run at midlatitudes, identifying the processes that maintain it (section 4a). Then, we discuss its equatorial response, which must be remotely forced by processes poleward of 12°N (section 4b). Finally, we report the influences of stochastic forcing in solutions with self-sustained and damped decadal modes (section 4c).

a. Midlatitude response

1) Description

Figure 5 plots sea level anomalies (Δd) over half of the primary cycle. A striking characteristic is the westward propagation north of 25°N. At θ = 0° and 45°, a region of negative Δd develops in the northeast Pacific that first strengthens locally and then expands westward. It continues to propagate westward throughout the second half of the cycle, as illustrated by the negative anomalies in the figure. Near the western boundary, the anomaly strengthens and divides into two parts. The southern one continues to propagate westward and to weaken, and the northern one first intensifies in a region centered near 43°N, 160°E, before shifting northward and dissipating sometime after θ = 360°.

Figure 5 also plots the layer-1 flow-field anomalies (Δv, arrows). The Δd contours are approximate geostrophic streamlines for the model's layer-1 flow. Throughout most of the basin, the currents tend to be parallel to Δd contours, indicating that they are largely geostrophic. There are also ageostrophic currents, the most prominent examples being the southeastward flow across Δd contours in the θ = 0° and 45° panels, a consequence of anomalous Ekman drift.

Figure 6 plots the corresponding evolution of ΔT1. It has a more complicated structure than Δd, likely because T1 is affected by both ocean dynamics (advection and convection) and surface heat fluxes. Moreover, the relationships among ΔT1, Δd, and Δv1 change in different regions. For example, in the eastern and central North Pacific, the strong northward current between regions of positive and negative Δd appears to generate warm ΔT1 by advection. In contrast, the large area of cool ΔT1 in the eastern subtropics from θ = 90° to 180° does not seem to be determined by advection, Δv1 there being much weaker. We infer that ΔT1 there is instead determined by surface fluxes, an idea that is confirmed in section 4a(2). Finally, sometimes Δd appears to be centered on ΔT1 regions, and Δv1 circulates around them, a result of the factor of T1T4 in (20). This situation is particularly clear for the northward-shifting anomaly along the western boundary.

Figure 6 also plots the wind anomaly (Δτ, arrows). Its time evolution consists primarily of large-scale circulations that form in the northeast Pacific, expand locally, and then shift westward. For example, the anticyclone that forms in the far northeastern corner of the basin at θ = 0° expands southward and strengthens from θ = 45° to 135°. As indicated by the cyclone in the panels, during the second half-cycle the anticyclone continues to move westward, shifts poleward, and finally moves out of the basin in the northwest corner. A comparison of Figs. 2 and 6 shows that the westward shift is associated with a switching from SVD4 to SVD3: SVD4 dominates Δτ at θ = 45°, SVD3 is strongest at θ = 135°, and thereafter the negative of SVD4 emerges, allowing the westward movement of the anticyclone to continue. Note in Fig. 6 that the winds are quite strong in the subtropics and even extend into the Tropics. As we shall see, these winds are important for generating EDV in the solution.

A comparison of Δτ, Δd, and ΔT1 maps suggests that the ocean responds to Δτ in two prominent ways. The Δd field clearly responds to the Ekman pumping associated with this forcing, with anticyclones (cyclones) being roughly collocated with regions of positive (negative) Δd. In the eastern and central subtropics, cold (warm) ΔT1 corresponds to τ anomalies that tend to strengthen (weaken) the northeast trade winds, suggesting that they may result from changes to the surface heat flux caused by ΔW.

All the preceding properties are consistent with the following scenario for the cause of the solution's decadal oscillation. Suppose initially that there is a ΔT1 in the northwest Pacific that forces Δτ through atmospheric teleconnections in the northeast Pacific. These anomalous winds generate Δd locally via Ekman pumping and excite Rossby waves that subsequently propagate across the basin. The Rossby waves are strengthened by the westward shift of Δτ and eventually cause a basin-wide adjustment of Δd and Δv1. This adjustment alters ΔT1 in the northwest Pacific through advection, particularly in the western boundary current, and through atmospheric teleconnections it generates a Δτ in the northeast region of the opposite sign. The analyses reported in the next two sections support this scenario. In addition, they point toward the importance of ocean–atmosphere coupling in the eastern subtropics.

Recall that the model was not able to generate a decadal mode when SVD4 was omitted from the empirical atmosphere, that is, with N = 3 in (7). To check the sensitivity of this property to the types of SVDs used, we constructed the empirical model using the J = 3 wintertime SVDs defined in section 2c(1)ii. For the choices for N, θk, and ϕk listed in section 2c(1)v, the resulting coupled solution was almost unchanged from the one described here. For reasons that are not clear, however, the model was also able to develop a decadal oscillation when N = 3, pointing toward the critical importance of SVD3, rather than SVD4, in the dynamics of the decadal mode.

2) Thermodynamics

Figure 7 shows the standard deviation of ΔT1 averaged over one period of the oscillation. Relative maxima are in the northwest (43°N, 156°E), the subtropical northeast (31°N, 144°W), the midlatitude northeast (41°N, 144°W), and the Tropics (0°N, 135°W). Hereafter, we use the labels W, E, N, and T to refer to 16° longitude by 8° latitude boxes centered on each of these points. Since Δτ is forced by ΔT1 outside the Tropics, the first three boxes are key regions to look for ocean-to-atmosphere feedbacks. Here, we carry out analyses to determine the processes that cause ΔT1 in each of them.

Subtracting the time average of (1) from (1) itself, yields an equation for the T1 anomaly field,
i1520-0442-16-3-383-e21
where each qj is one of the heating terms on its right-hand side, Δqjqj − 〈qj〉 and J is the number of terms. Multiplying (21) by ΔT1 yields
i1520-0442-16-3-383-e22
The positive (negative) terms on the right-hand side are responsible for the instantaneous growth (decay) of T1 anomalies regardless of their sign.

Figure 8 plots the dominant terms in Eq. (22) averaged over region W, showing advection (ADV), total surface heat flux (QS), and convective overturning (QC). Interestingly, QS acts to damp ΔT1, so that ocean dynamics determine ΔT1. Indeed, both advection and convective overturning provide the positive feedback that amplifies ΔT1, consistent with the study of Schneider et al. (2002). Plots of terms in (21) (not shown) indicate that the convection is triggered by anomalous advection, with the anomalous currents preceding convection by 4–6 months, and that the switching mechanism (delayed negative feedback) for ΔT1 is also provided by anomalous advection. Calculation of the terms for region N (not shown) demonstrates that, as for region W, ADV is the dominant growth mechanism with QS providing the decay, but there is no heat anomaly due to QC.

Figure 9 plots the dominant terms from Eq. (22) averaged over region E, showing advection, total surface heat flux, and two parts of the latent heat flux, namely, the part due to ΔW (LHW) and the remainder due to ΔT1(LHT). Integrated over one cycle, only QS provides a positive contribution, and so acts to amplify ΔT1 locally; moreover, the positive contribution results from LHW, a result noted by KMK. Conversely, the other terms (as well as LHW for part of the cycle) are negative when integrated over one oscillation cycle, and so tend to dampen it. Near region E, then, local air–sea feedback via LHW intensifies ΔT1, whereas ocean dynamics (ADV) tends to dampen it. In a similar analysis of (21), the term analogous to LHT is also dominant when ΔT1 = 0 (not shown), an indication that the switching mechanism arises from remotely forced winds.

3) Ocean-only solutions

To explore the influences of local and remote forcing in the main run, we obtained solutions to a series of model runs where the ocean model was forced by versions of Δτ saved from the coupled run. In one of those tests, we forced the model using Δτ only east of 160°W, setting Δτ to zero west of 160°W. Figure 10 illustrates the evolution of Δd for this run over half of a cycle. Consistent with the coupled run (Fig. 5), the forced response develops an anticyclonic gyre in the eastern ocean that subsequently propagates westward. One obvious difference between the forced and coupled solutions is that Δd is considerably weaker in the western ocean in the ocean-only solution. Another is that the westward propagation is a bit faster in the coupled solution. This can be seen in the northward current between positive and negative Δd regions, which is shifted farther to the west in the coupled solution. We conclude that oceanic Rossby waves, generated by wind curl in the northeastern ocean, are important for causing the westward propagation in the coupled solution. In addition, wind forcing in the north-central and northwestern regions maintains and strengthens the waves, particularly because of the simultaneous westward shift of the forcing.

4) Masked runs

To determine the locations of key ocean-to-atmosphere feedbacks, we obtained a series of coupled runs with feedbacks suppressed in specific regions by adjusting θk and ϕk in (11c). Here, we report solutions in which the basin is divided into quadrants by the lines x = 170°W and y = 30°N, and either ΔT1, Δτ, or both are masked in one or more quadrants.

A solution with ΔT1 masked in the northeast and southwest quadrants still oscillates provided that ϕo is increased to 1.5. In contrast, solutions with ΔT1 masked separately in the southeast and northwest quadrants never oscillate regardless of the value of ϕo. Expanding upon these results, we obtained a test solution with ΔT1 masked in the northeast and southwest quadrants and with Δτ masked in both western quadrants. With ϕo increased to 1.5, the solution oscillates with the same period as the main run but with a weaker amplitude; when ϕo is increased to 2.5, the solution also has a similar amplitude. Figure 11 shows the evolution of Δd and Δv1 over one-half of the decadal oscillation for the latter solution, and the similarity to Fig. 5 is striking; moreover, it also reproduces ΔT1 from the coupled run just as well (not shown).

These results suggest that the solution in Fig. 11 captures the essential physics of the decadal oscillation in the main run. In particular, it points toward the importance of ocean-to-atmosphere coupling in the northwest midlatitudes and northeast subtropics. We interpret the coupling in the former region to represent an influence of SST on the location of the storm track, which causes anomalous atmospheric circulation in the northeast midlatitudes though atmospheric teleconnections. Its necessity is consistent with the prior observational and modeling work indicating that northwest SST anomalies are related to wind anomalies in the northeast (see section 1 and Yulaeva et al. 2001). We interpret coupling in the latter region to represent the ability of subtropical SST anomalies to maintain the atmospheric circulation in the northeast and to broaden it southward into the subtropics, consistent with the analysis of atmospheric wave-activity flux reported by Nakamura and Yamagata (1999). The potential importance of coupling in the northeast subtropics has been noted by others (e.g., Nakamura and Yamagata 1999; Nakamura and Izumi 2002; KMK; F.-F. Jin 2001, personal communication). Indeed, KMK were able to obtain a decadal oscillation without any coupling in the northwest quadrant, likely a consequence of their coupling coefficients ck being considerably larger than ours.

b. Equatorial response

Figure 6 shows a strong ΔT1 signal near the equator, with a maximum amplitude of about 1°C near 130°W. Since Δτ is suppressed near the equator by Eq. (11c), this equatorial variability must be caused by oceanic teleconnections forced north of 12°N. Here, we demonstrate that the teleconnection occurs through changes in the strength of various branches of the North Pacific STC, and report the sensitivity of solutions to Δτx along the subduction cutoff latitude, yd = 18°N, and to the value of yd itself.

Figure 12a shows anomalies of M1(yd) (solid curve with ×), M2(yd) (solid curve with ○), E(yd) (thick dashed curve), the upwelling-transport anomaly between layers 1 and 2 near the equator W (dashed curve), and ΔT1 averaged in the Niño-3.5 region T1 (solid curve) for the main run. The W curve covaries with T1, indicating that T1 results largely from changes in the amount of cool water that upwells into layer 1. An analogous plot for T2 (the average of ΔT2 in the Niño-3.5 region) has an amplitude of only about 0.1°C, so that T1 is not caused by the advection and upwelling of subsurface temperature anomalies, as in the Gu and Philander (1997) hypothesis. The ΔM1(yd) curve has a similar shape to both ΔE(yd) and W, and leads W by about 2 yr. These properties suggest that both W and T1 are driven by changes in M1(yd) and hence the strength of the North Pacific STC, as proposed by KMK. Transport ΔM1(yd) also has a similar shape to ΔM2(yd), a property that is not consistent with quasi-steady changes in the STC for which ΔM1(yd) ≈ −ΔM2(yd). As discussed next, this difference exists because the response is not at all quasi-steady, involving the propagation of Rossby waves about the basin.

To isolate the part of the wind field that drives the tropical circulation, we carried out two ocean-only runs, one forced by winds saved from the coupled run that were confined poleward of yd (extratropical winds; Fig. 12b) and at their full strength equatorward of yd (tropical winds; Fig. 12c). Given the latitudinal resolution of the atmospheric grid (Δy = 4°), this separation was accomplished by linearly ramping the winds from 20°–28°N to zero when y > 28°N (y < 20°N) for the tropical (extratropical) winds. Figure 12d plots the sum of curves from the two forced runs; they closely track those of the coupled run, demonstrating that the STC variability responds nearly linearly to the winds.

A comparison of the curves in Figures 12a–c, demonstrates that most of the equatorial response in the coupled solution is driven by tropical winds, the exception being for ΔM2(yd). In particular, note that the extratropical winds force relatively weak W and T1 with opposite signs to those in the main run. In addition, when the extratropical winds are excluded (Fig. 12c), W lags ΔM1(yd) by approximately 2 yr but leads −ΔM2(yd) by about 1 yr. This sequence indicates that winds across yd drive ΔM1(yd) that drives W, which in turn spins up a ΔM2(yd) of the opposite sign to ΔM1(yd), consistent with the conclusions of Klinger et al. (2002). This relationship is unclear in the coupled run due to ΔM2(yd) also being forced by extratropical winds.

Recall from the discussion of (3) that the STC strength in steady solutions depended on E and hence on Δτx along the subduction latitude yd. To test the sensitivity of solutions to Δτx(yd), we obtained a test run with ϕk = S(y − 19°) so that Δτ was set to zero equatorward of 19°N and Δτx(yd) = 0. With ϕo unchanged, the resulting solution developed an oscillation with the same period but with a considerably weaker amplitude than in the main run, suggesting that ΔT1 from 12°–19°N plays a role in the oscillation dynamics. Indeed, ΔT1 is large in this region in the main run, and it projects significantly onto both SVD3 and SVD4 temperature patterns. Increasing ϕo by 30%, however, resulted in a decadal oscillation with the same amplitude and timescale as the main run, indicating that ΔT1 in this region is not of critical importance. In this run, however, the peak-to-peak maximum amplitude of T1 at the equator reduced from 1° to 0.2°C (similar to the weak T1 for the midlatitude-forced solution in Fig. 12b). We conclude that, consistent with steady-state theory, Δτx(yd) does affect the STC strength and T1 significantly.

Finally, we obtained a solution with yd increased from 18° to 25°N. This solution had a decadal oscillation with the same structure and period as the main run, and T1 also did not change much. The reason for this similarity is that E(yd) is not much changed, a consequence of Δτx being stronger at 25°N and therefore compensating for the increase in f.

c. Damped mode and stochastic forcing

Solutions are sensitive to the value of ϕo. For example, when ϕo is increased to 1.4 the amplitude of the oscillation is 70% larger. Conversely, when it is reduced to 1.2 the oscillation rapidly decays away and the solution adjusts to a steady state.

To investigate the nature of the coupled system when the mode is damped, we obtained a series of solutions with ϕo = 1.2, including additional forcing by the SVD1 wind pattern (Fig. 2) with an amplitude such that T1 is approximately equal to 1°C and periods P varying from 2 to 24 yr. After an initial adjustment, the solutions all oscillated with a period P, with the largest amplitude occurring when P = 16 yr, somewhat longer than the period of the self-sustained mode (12.8 yr) due to the damping. In addition, the solution with P = 24 yr developed a secondary peak at P/2, a result of the excitation of the model's decadal mode by nonlinearities. These properties indicate that the system is a weakly nonlinear, damped oscillator, in which the damped mode responds resonantly to the forcing.

There is considerable interest at present regarding the possible generation of midlatitude decadal variability by stochastic forcing (e.g., Saravanan and McWilliams 1997; Moore 1999). We examined the influence of such forcing in our model by including it as an externally prescribed wind stress anomaly Δτ′, as outlined in section 2c(3). With Δτ′ included and ϕo = 1.3, the self-sustained oscillation remained and the peak at a 13.5-yr period continued to exceed the 99% significance level based on a first-order autoregressive process (AR1) null hypothesis; however, the amplitude of the decadal spectral peaks of ΔT1 in regions E and W decreased to 20% of their values without Δτ′, apparently because the stochastic forcing altered ΔT1 enough to weaken the coupling associated with SVD3 and SVD4 significantly. With Δτ′ and ϕo = 1.2, the spectrum of ΔT1 in regions E and W became indistinguishable from an AR1 spectrum calculated with the same variance and lag-1 autocorrelation as the model output. In our model, then, the addition of stochastic forcing tends to inhibit, rather than to enhance, decadal variability.

5. Solutions with both modes

In this section, we report solutions when both tropical and extratropical feedbacks are allowed, that is, with ϕk and θk specified as in Eqs. (11). These solutions are able to develop both interannual and decadal oscillations. The basic structure and dynamics of each oscillation are unchanged from those discussed in sections 3 and 4, so here we focus on interactions between the two signals.

Figure 13 shows the temporal behavior of the coupled oscillation when ϕo = 1.3, plotting curves for E(yd), T1, and the North Pacific index (NPI, the average temperature anomaly in the region 29°–55°N, 160°E–140°W). All three curves have both interannual and decadal variability. The structure and amplitude of E(yd) are very similar to those in the main run (Fig. 12a), showing only a weak influence of the interannual signal. In contrast, the interannual modulation of NPI, caused by atmospheric teleconnections from the Tropics, is large. (The amplitude of NPI is small because it straddles regions where ΔT1 has opposite signs. See Figs. 6 and 7.) Perhaps most striking, T1 is dominated by decadal variability, with one out of every three oscillations of the interannual mode being suppressed (reversed). The interannual and decadal signals are in fact phase-locked with a period ratio of 1:3, a property noted by KMK in their solutions with stronger midlatitude coupling. As discussed in section 4, this model EDV results entirely from STC transport variability.

When ϕo is reduced to 1.2, the decadal oscillation is damped in the absence of tropical forcing (section 4c). When tropical feedback is allowed, however, atmospheric teleconnections from the Tropics are sufficient to maintain it, albeit with a smaller amplitude: NPI, E(yd), and T1 curves are similar in structure to those in Fig. 13 but their amplitude is smaller by about 33%. Interestingly, the interannual and decadal signals are no longer precisely phase-locked, likely a result of the weakened decadal signal. As a result, T1 has a slowly varying beat pattern with a period longer than 100 yr.

Figure 14 illustrates the coupled solution when ϕo = 1.2 and with stochastic forcing by Δτ′, showing curves for T1 and temperature anomalies in regions E (TE) and W (TW). Consistent with the results in section 4c, the decadal oscillation is much weaker, but it is still visible in all three curves. (Curves TE and TW actually have a larger amplitude than NPI in Fig. 13 because they are centered in regions where ΔT1 is of one sign and achieves a relative maximum.) In TE and TW, the decadal signal and higher-frequency noise is most apparent. In T1, the decadal variability is much weaker than in Fig. 13, so that it now appears as an irregular modulation of a strengthened interannual signal. Finally, Fig. 15 shows T1, TE, and TW for a solution with stochastic forcing and ϕo = 0, for which there is no extratropical decadal mode. The interannual signal is now most apparent in the TE and TW curves, with no indication of a distinct decadal peak. In T1, the interannual signal is even stronger than in Fig. 13, and decadal variability occurs at longer periods.

For all these solutions, there is strong two-way coupling between the Tropics and extratropics. Suppose initially that a decadal signal is generated at midlatitudes (e.g., by forcing the model with the SVD3 wind anomaly pattern for some time). This signal is subsequently transmitted to the Tropics via oceanic teleconnections through variations in STC transport, where it moderates, or even dominates, tropical interannual variability. This modulation is in turn transmitted back to midlatitudes via atmospheric connections, where it has the proper phasing to modify the self-sustained decadal signal or to reinforce a damped one. Extratropical stochastic forcing weakens the amplitude of the decadal mode, allowing the interannual mode to dominate in the Tropics as it should.

6. Summary and discussion

We have explored the causes of PDV and EDV in an intermediate coupled ocean–atmosphere model of the Pacific region. Its ocean component is a variable-temperature, 3½-layer model (Fig. 1). Its atmospheric component consists of three parts: an empirical model that utilizes SVDs between observed wind and SST anomalies to determine Δτ from the model ΔT1 field [Eqs. (7) and (8)]; a simple representation of the planetary boundary layer that determines ΔQ [section 2c(2)]; and a prescribed stochastic wind stress forcing Δτ′ [Eq. (17)]. The structure functions, ϕk and θk, included in (7) and (8), are an integral part of the empirical model. They specify regions 1 (θk ≠ 0) and 2 (θk = 0) where ocean-to-atmosphere coupling is active and absent, and thereby allow a model definition of atmosphere teleconnections (i.e., an atmospheric response in region 2 generated in region 1). For dynamical simplicity, only SVD1, SVD3, and SVD4 are used, since solutions to atmospheric GCMs suggest that their SST and wind stress patterns are dynamically, as well as statistically, linked [section 2c(1)i]. SVD2 is not used because it closely resembles SVD2′, the corresponding SST-tendency SVD [section 2c(1)ii], and hence is likely to be determined mostly by atmosphere-to-ocean forcing. SVD1 and SVD3 are essential for generating the interannual and decadal modes, respectively.

Simultaneous cross correlations between SST and atmospheric variables can result from prior forcing by atmospheric noise (Frankignoul 1985, 1999). Thus, the patterns in our SVDs could result entirely from atmosphere-to-ocean forcing, potentially a fundamental inconsistency in the formulation of our empirical atmosphere (section 2c(1)ii]. The similarity of our monthly mean and 7-month averaged SVDs, however, shows that the former captures patterns that can persist for up to 7 months and vary interannually. We conclude that the possibility that ocean-to-atmosphere processes are involved in their structure cannot be ruled out. Moreover, cross correlations of time series associated with wintertime SVD3s suggest that they are associated with decadal variability not just high-frequency noise, although this result lacks statistical significance. We also explored the use of lag-1 SVDs as a means for weakening atmosphere-to-ocean forcing, but concluded that lagging the fields aliased high-frequency variability into the structure of SVD3 and SVD4.

Solutions are able to develop two modes of oscillation, namely, interannual and decadal modes with periods close to 4 and 12 yr. The interannual mode is isolated by including only SVD1 in the statistical atmosphere, that is, by setting N = 1 in (7). The resulting solution develops an interannual oscillation that resembles ENSO, including atmospheric teleconnections to midlatitudes. Consistent with the time-delay oscillator theory of ENSO in a self-sustaining regime, off-equatorial Rossby waves reflect from the western boundary as equatorial Kelvin waves, weakening |ΔT1| in the eastern ocean, and thereby triggering the onset and termination of warm and cold events.

The decadal oscillation is isolated by excluding SVD1 from the statistical atmosphere, by starting the summation in (7) at k = 3. For the parameter choices listed in section 2c, solutions develop a self-sustained decadal mode, which at midlatitudes has a structure similar to the Latif and Barnett (1994) mode. Our analyses suggest that a midlatitude time-delay oscillator is responsible for this mode, with positive feedback present in both the northwest midlatitudes and northeast subtropics and delayed negative feedback occurring via Rossby wave propagation.

To illustrate the cool phase of the decadal cycle, suppose initially that a cool ΔT1 appears in the northwest Pacific. This anomaly drives atmospheric teleconnections that modify τ in the northeast Pacific, creating an anticyclone there (θ = 0° and 45°, Figs. 6a and 6b, respectively). The southern part of the anticyclone acts to strengthen the northeast trades, cooling T1 by latent heat changes driven by wind speed changes. This cooling in turn strengthens the anticyclone, extending it southward through its projection onto primarily SVD3 (θ = 90° and 135°, Figs. 6a and 6b, respectively). Delayed negative feedback results from changes in oceanic circulation forced by the anticyclone and the subsequent propagation of oceanic Rossby waves across the basin (Fig. 5). The arrival of these waves in the northwest Pacific triggers a switch in ΔT1 to a warm phase, which is maintained through advection and convective overturning.

The potential importance of coupling in the northwest midlatitudes has been noted by others (Xie et al. 2000; Miller and Schneider 2000), and interpreted as an influence of SST anomalies there on the location of the storm track (Nakamura and Izumi 2002; Yulaeva et al. 2001). The importance of interactions in the northeast subtropics has also been reported. For example, the atmospheric forcing of SST anomalies in the northeast subtropics has been demonstrated in a number of studies (Barnett et al. 1999; Pierce et al. 2000b, among others). Very recently, it has been shown that the response of an atmospheric GCM to an SST anomaly imposed in the northeast subtropics is a cyclone located northwest of the anomaly that enhances the initial perturbation through latent heat and shortwave fluxes (F.-F. Jin 2001, personal communication), similar to our coupled solution.

For smaller values of coupling (ϕo = 1.2), the decadal mode is no longer self-sustained, and the decadal response of the system reduces to that of a weakly nonlinear, damped oscillator. Stochastic forcing by a wind stress anomaly Δτ′ [section 2c(3)] is unable to maintain the decadal mode or to generate a spectral peak at decadal timescales (section 4c). On the other hand, the decadal signal can be maintained when tropical coupling is included (ϕ1 = 1.3) through atmospheric teleconnections from the Tropics (section 5).

Model EDV is linked to PDV by variations in the transport of the North Pacific STC (section 4b). According to (11c), these transport variations arise necessarily via changes in wind stress forcing north of 12°N. Additional tests reported in section 4b indicate that the equatorial response is forced primarily by winds south of 28°N, and moreover that wind variability along yd = 18°N is particularly important. In response to easterly wind anomalies along yd, for example, more warm surface water diverges from the tropical ocean. After a period of adjustment (about 2 yr), more cool water upwells in the eastern Pacific to supply water for the surface divergence and the cold tongue strengthens, which in turn helps to maintain the easterly anomalies. This strengthened cold tongue modifies the tropical ocean–atmosphere coupling that generates the model ENSO (section 5). In the real ocean, a strengthened cold tongue prevents atmospheric convection in the western Pacific from shifting as far eastward, thereby decreasing the amplitude or likelihood of ENSO warm events. Note that this mechanism is not the one hypothesized by Gu and Philander (1997), since it is transport rather than temperature that varies; indeed, variations in equatorial T2 are too small to account for T1. Extratropical stochastic forcing also affects EDV through its effect on the STC transport, producing more pronounced decadal variability when there is an active decadal mode (Fig. 14) than when there is not (Fig. 15).

In conclusion, our intermediate model provides a useful step in the hierarchy of coupled systems that is necessary to understand the causes of PDV and EDV. Among other things, it identifies potential key regions of ocean-to-atmosphere interaction (i.e., the northwest midlatitudes and northeast subtropics) and demonstrates the capability of STC transport variability for generating EDV. On the other hand, the model's dynamical simplicity is also a limitation, as it neglects a number of potentially important processes. These processes include the lack of a seasonal cycle, the ocean model's simplistic mixed-layer physics [Eqs. (2a) and (2b)], and the lack of a time-varying Indonesian Throughflow, which can affect how much of the STC variability actually reaches the equator. Perhaps most serious is the statistical nature of the model atmosphere. As a logical next step in model development, we plan to replace the statistical atmosphere with one that is both dynamically based and computationally efficient.

Acknowledgments

We thank Axel Timmermann and Fei-Fei Jin for helpful discussions. This research was supported by NOAA through Grant NA76GP0353 and by the Frontier Research System for Global Change through its sponsorship of the International Pacific Research Program (IPRC).

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Fig. 1.
Fig. 1.

A section along 140°W from the background solution, illustrating the structure of the ocean model

Citation: Journal of Climate 16, 3; 10.1175/1520-0442(2003)016<0383:IADVIA>2.0.CO;2

Fig. 2.
Fig. 2.

Spatial patterns of the first four SVDs, showing ΔT1 (contours) and Δτ (arrows) patterns. Both fields are nondimensional

Citation: Journal of Climate 16, 3; 10.1175/1520-0442(2003)016<0383:IADVIA>2.0.CO;2

Fig. 3.
Fig. 3.

Structure of the interannual solution at the peak of its warm phase, showing ΔT1 (contours) and Δτ (arrows) anomalies. Units for ΔT1 are 1°C

Citation: Journal of Climate 16, 3; 10.1175/1520-0442(2003)016<0383:IADVIA>2.0.CO;2

Fig. 4.
Fig. 4.

Phase (θ) evolution of Δd (contours) and Δv1 (vectors) for the interannual solution. Units for Δd are 1 cm

Citation: Journal of Climate 16, 3; 10.1175/1520-0442(2003)016<0383:IADVIA>2.0.CO;2

Fig. 5.
Fig. 5.

Phase (θ) evolution of Δd (contours) and Δv1 (vectors) for the decadal solution. Units for Δd are 1 cm

Citation: Journal of Climate 16, 3; 10.1175/1520-0442(2003)016<0383:IADVIA>2.0.CO;2

Fig. 6.
Fig. 6.

Phase (θ) evolution of ΔT1 (contours) and Δτ (vectors) for the decadal solution. Units for ΔT1 are 1°C

Citation: Journal of Climate 16, 3; 10.1175/1520-0442(2003)016<0383:IADVIA>2.0.CO;2

Fig. 7.
Fig. 7.

Standard deviation of ΔT1 variability for the decadal solution averaged over one oscillation. Units are 1°C

Citation: Journal of Climate 16, 3; 10.1175/1520-0442(2003)016<0383:IADVIA>2.0.CO;2

Fig. 8.
Fig. 8.

Time series of dominant terms from Eq. (22) averaged over region W. The curves indicate total advection (ADV), total surface heat flux (QS), convective overturning (QC), the sum over all tendency terms (TOT), and ΔT1

Citation: Journal of Climate 16, 3; 10.1175/1520-0442(2003)016<0383:IADVIA>2.0.CO;2

Fig. 9.
Fig. 9.

Time series of dominant terms from Eq. (22) averaged over region E. The curves indicate total advection (ADV), total surface heat flux (QS), and the dominant terms that contribute to QS, namely, latent heat flux due to ΔW (LHW) and the rest of the latent heating due to ΔT1 (LHT), the sum over all tendency terms (TOT), and ΔT1

Citation: Journal of Climate 16, 3; 10.1175/1520-0442(2003)016<0383:IADVIA>2.0.CO;2

Fig. 10.
Fig. 10.

Phase (θ) evolution of Δd (contours) and Δv1 (vectors) for the decadal solution with air–sea feedback east of 180° (dashed line) suppressed. Units for Δd are 1 cm

Citation: Journal of Climate 16, 3; 10.1175/1520-0442(2003)016<0383:IADVIA>2.0.CO;2

Fig. 11.
Fig. 11.

Phase (θ) evolution of Δd (contours) and Δv1 (vectors) for the coupled run with air–sea feedbacks in the northeast and southwest quadrants suppressed and Δτ masked to the west of 180°. Units for Δd are 1 cm. Dashed lines denote quadrant borders

Citation: Journal of Climate 16, 3; 10.1175/1520-0442(2003)016<0383:IADVIA>2.0.CO;2

Fig. 12.
Fig. 12.

Time series of anomalies of M1(yd) (×), M2(yd) (○), E(yd) (thick dashed), W (dashed), and T1 (solid). Results shown are for (a) the decadal solution, (b) an ocean-only solution forced by winds from the decadal solution confined poleward of 20°N, (c) an ocean-only solution forced by winds at full strength equatorward of 20°N, and (d) the sum of the curves in (b) and (c). Units for M1, M2, E, and W are 1 Sv (1 Sv ≡ 106 m3 s−1), and for T1 are 1°C

Citation: Journal of Climate 16, 3; 10.1175/1520-0442(2003)016<0383:IADVIA>2.0.CO;2

Fig. 13.
Fig. 13.

Time series of T1 (thick dashed), NPI (thin dashed), and E(yd) (solid) in the coupled run with self-sustained interannual (ϕ1 = 1.3) and decadal (ϕo = 1.3) oscillations. Units for temperature and transport are 1°C and 0.5 Sv

Citation: Journal of Climate 16, 3; 10.1175/1520-0442(2003)016<0383:IADVIA>2.0.CO;2

Fig. 14.
Fig. 14.

Time series of T1 (blue), and temperature anomalies in regions W (green) and E (red) in the coupled run with self-sustained interannual (ϕ1 = 1.3) and damped decadal (ϕo = 1.2) oscillations and stochastic forcing. Units are 1°C

Citation: Journal of Climate 16, 3; 10.1175/1520-0442(2003)016<0383:IADVIA>2.0.CO;2

Fig. 15.
Fig. 15.

Time series of T1 (blue), and temperature anomalies in regions W (green) and E (red) in the coupled run with a self-sustained interannual (ϕ1 = 1.3) and stochastic forcing, but no decadal mode (ϕo = 0). Units are 1°C

Citation: Journal of Climate 16, 3; 10.1175/1520-0442(2003)016<0383:IADVIA>2.0.CO;2

*

School of Ocean and Earth Sciences and Technology, University of Hawaii at Manoa, Contribution Number 6067 and International Pacific Research Center Contribution Number 179.

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