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Precipitation in Boreal Summer Simulated by a GCM with Two ConvectiveParameterization Schemes: Implications of the Intraseasonal
Oscillation for Dynamic Seasonal Prediction
SUHEE PARK
National Institute of Meteorological Research, Korea Meteorological Administration, Seoul, South Korea
SONG-YOU HONG
Department of Atmospheric Sciences, and Global Environment Laboratory, Yonsei University, Seoul, South Korea
YOUNG-HWA BYUN
National Institute of Meteorological Research, Korea Meteorological Administration, Seoul, South Korea
(Manuscript received 3 June 2009, in final form 20 November 2009)
ABSTRACT
In this paper, the intraseasonal oscillation (ISO) and its possible link to dynamical seasonal predictability
within a general circulation model framework is investigated. Two experiments with different convection
scheme algorithms, namely, the simplified Arakawa–Schubert (SAS) and the relaxed Arakawa–Schubert
(RAS) convection algorithms, were designed to compare seasonal simulations from 1979 to 2002 on a seasonal
model intercomparison project (SMIP)-type simulation test bed. Furthermore, the wave characteristics (wave
intensity, period, and propagation) of the simulated ISO signal provided by the model with two different
convection schemes for extended boreal summers from 1997 to 2004 were compared to the observational ISO
signal. Precipitation in the boreal summer was fairly well simulated by the model irrespective of the convection
scheme used, but the RAS run outperformed the SAS run with respect to tabulated skill scores. Decomposition
of the interannual variability of boreal summer precipitation based on observations and model results dem-
onstrates that the seasonal predictability of precipitation is dominated by the intraseasonal component over the
warm pool area and the SST-forced signal over the equatorial Pacific Ocean, implying that the seasonal mean
anomalies are more predictable under active ISO conditions as well as strong ENSO conditions. Comparison of
the ISO simulations with the observations revealed that the main features, such as the intensity of precipitation
variance in the intraseasonal time scale and the evolution of propagating ISOs, were reproduced fairly well by
the model; however, the wave characteristics associated with the ISO signals were better captured by the
experiment with the RAS scheme than the SAS scheme. This study further suggests that accurate simulation of
the ISO can improve the seasonal predictability of dynamical seasonal prediction systems.
1. Introduction
Prediction of seasonal mean climate is one of the chal-
lenges of climate prediction (e.g., Anderson et al. 1999;
Shukla et al. 2000). Many studies have developed models
for seasonal prediction based on a statistical, dynamical,
or a hybrid approach combining statistical and dynamical
methods. The statistical method takes into account certain
indices associated with low-frequency components of the
climate systems. Statistical models have shown reasonable
skill when the seasonal mean lies close to the norm, but
have little skill in predicting extreme events such as the
severe drought of the 2002 Indian monsoon (Goswami
et al. 2006). Furthermore, it is difficult to provide a com-
plete physical description of seasonal climate anomalies
predicted by statistical models. Meanwhile, the dynamic
approach, which is based on general circulation models
(GCMs) (Kumar et al. 1996; Shukla et al. 2000) and
global–regional coupled dynamical downscaling models
(Nobre et al. 2001; Sun et al. 2006), makes it possible to
provide mechanisms for the evolution of climate anomalies
Corresponding author address: Dr. Song-You Hong, Dept. of
Atmospheric Sciences, College of Science, Yonsei University,
Seoul 120-749, South Korea.
E-mail: [email protected]
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DOI: 10.1175/2010JCLI3283.1
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in response to slowly varying external forcing. The hy-
brid statistical–dynamical approach applies statistical
methods to the past performance of a dynamic model
(Graham and Barnett 1995; Mo and Straus 2002).
An example of a dynamic model for seasonal prediction
is the fully coupled ocean–land–atmosphere dynamical
seasonal model that the National Centers for Environ-
mental Prediction (NCEP) has used to issue operational
seasonal forecasts since 2004 (Saha et al. 2006). This
dynamical modeling system has shown a better level
of skill in forecasting U.S. surface temperature and pre-
cipitation than statistical methods. In addition, European
researchers have an active seasonal-to-interannual pre-
diction project, known as the Development of a European
Multimodel Ensemble System for Seasonal to Interannual
Prediction (DEMETER; Palmer et al. 2004). Seven global
atmosphere–ocean coupled models are included in this
project and seasonal ensemble forecasts are used for crop
yield prediction. However, despite successful application
of the GCM to seasonal prediction in some regions (e.g.,
North America and Europe), dynamical prediction does
not yet guarantee overall better skill than the statistical
approach (Barnston et al. 2003).
The present skill of dynamical seasonal prediction is
limited by several factors, mainly the inherently nonlinear
characteristics of the atmosphere and the inaccuracy of
current GCMs (Anderson et al. 1999; Barnston et al.
2003), particularly over the Asian monsoon region (Kang
et al. 2004; Goswami et al. 2006). It has become clear that
external forcing, especially slowly varying anomalous
lower boundary forcing, is more important than infor-
mation from the atmospheric initial state for predicting
anomalous atmospheric circulation features on time scales
beyond a month or season. To address this, dynamical sea-
sonal prediction is based on the fact that slowly varying
boundary conditions, such as sea surface temperature
(SST) and snow cover, affect mainly global atmospheric
circulation and surface climate.
Meanwhile, the tropical intraseasonal oscillation (ISO),
also known as the Madden–Julian oscillation (MJO), is
the most important variability at the subseasonal time
scale, and is a dominant mode in the tropical region with
eastward periods of 30–60 days (Madden and Julian
1994). Several studies have reported that the ISO has an
influence on large-scale circulation and precipitation over
the subtropical and extratropical regions (e.g., Kang et al.
1989; Jones et al. 2004; Liess et al. 2005; Lorenz and
Hartmann 2006; Kim et al. 2006). Kang et al. (1989)
showed that the observational ISO anomaly, which starts
in the tropical Indian Ocean and ends south of Japan, is
closely related to variation in the East Asian summer
monsoon. Jones et al. (2004) examined the importance of
the MJO in the Northern Hemisphere weather forecasts,
and demonstrated that the MJO signal is important in
modulating weather variability. Liess et al. (2005) ana-
lyzed the upper limit of potential predictability of the
northern summer ISO, and found that the predictability
follows the eastward- and northward-propagating ISO
during the active and break phases of the Asian monsoon.
The analysis of Lorenz and Hartmann (2006) demon-
strated that the MJO could affect the North American
monsoon by modulating low-level circulation. Kim et al.
(2006) found that the eastward-moving upper-level di-
vergence over an active tropical convective area has a
subtropical counterpart in the upper-level divergence
region of the MJO, and deduced that vorticity advection
by vertical motion and the tilting of vorticity are sources
of midlatitude–MJO teleconnection. As reviewed by
Sperber and Waliser (2008), it is clear that the MJO has
wide-ranging impacts on the atmosphere–ocean–land
system, including Asian–Australian monsoon variabil-
ity, tropical cyclone activity, and weather patterns in the
extratropics. It is therefore very important to under-
stand, simulate, and forecast the MJO in climate models
and numerical weather forecast models.
In the present study, we examine the relation between
the seasonal mean of boreal summer climate and the
embedded ISO signal, both of which are simulated by
a GCM. The cumulus convection scheme is known to
have an important role in ISO simulation because the
coupling between convection and circulation is a key
process in the MJO (e.g., Wang and Schlesinger 1999; Lee
et al. 2003; Zhang and Mu 2005) and seasonal mean cli-
mate (e.g., Gregory et al. 1997; Donner et al. 2001; Byun
and Hong 2007). Therefore, in this study, we compare
seasonal simulations with two different cumulus convec-
tion schemes in a GCM, focusing on the seasonal mean
precipitation and a possible contribution of the ISO to the
seasonal mean. It is important to note that the purpose of
our study is not to judge the superiority of one scheme
over the other in simulating climatology, but rather to
identify a possible link between the ISO and the seasonal
mean climate. The experimental design and model de-
scription are presented in section 2. The skill of seasonal
simulations with two difference convection schemes is
presented in section 3, together with the simulated mean
ISO component embedded in the interannual variability
in precipitation. The characteristics of the simulated ISO
are discussed further in section 4. Summary statements
and concluding remarks are provided in section 5.
2. Model and experimental design
a. Model description
The atmospheric model used in this study is a version of
the NCEP Medium-Range Forecast (MRF) model with
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the physics package that was operational as of January
2000 (Kanamitsu et al. 2002a). The model employs a
horizontal resolution with spectral truncations of T62
(triangular truncation of wavenumbers at 62, roughly
corresponding to about 200 km) and a 28-layer terrain-
following sigma coordinate in the vertical dimension.
Model physics include long- and shortwave radiation,
cloud–radiation interaction, planetary boundary layer
processes, deep and shallow convection, large-scale con-
densation, gravity wave drag, simple hydrology, and ver-
tical and horizontal diffusions.
Two different cumulus parameterizations for deep
convection were utilized to conduct sensitivity experi-
ments. One was the simplified Arakawa–Schubert (SAS)
scheme (Pan and Wu 1995), which is in turn based on
Arakawa and Schubert (1974), as simplified by Grell
(1993) with a saturated downdraft. The other convection
scheme selected for this study was the relaxed Arakawa–
Schubert (RAS) scheme (Moorthi and Suarez 1992),
which was implemented in the recent NCEP seasonal
forecast model (Kanamitsu et al. 2002a). The main dif-
ferences between SAS and RAS lie in two components:
the clouds model and the treatment of downdrafts. The
SAS allows only one type of cloud, while RAS allows
a cloud ensemble with different tops; the SAS considers
saturated downdrafts based on empirical formulation,
which is absent in the current version of the RAS scheme.
These differences result in different precipitation pat-
terns and vertical heating and moistening profiles (Byun
and Hong 2004). Kanamitsu et al. (2002a) showed that
the RAS parameterization scheme performs better than
the SAS scheme with respect to the Pacific–North Amer-
ica (PNA) pattern in response to an idealized SST forcing
over the equatorial Pacific. For short- and medium-range
forecasts, the SAS has demonstrated good skill in pre-
dicting tropical precipitation (Kalnay et al. 1996).
b. Experimental design
First, Seasonal Model Intercomparison Project (SMIP)-
type experiments were performed using observed SST
data (Reynolds and Smith 1994). These experiments are
referred to ‘‘EXP-SAS’’ and ‘‘EXP-RAS’’ for runs with
the SAS and RAS schemes, respectively. Both integra-
tions were carried out with an approximate 4-week lead
time for the boreal summer [June–August (JJA)] over
a 24-yr period, from 1979 to 2002. Each experiment had
10-member ensembles. Initial conditions were taken
from the NCEP/Department of Energy (DOE) Global
Reanalysis 2 data (Kanamitsu et al. 2002b), starting from
0000 UTC 26 April and running to 30 April, with a 12-h
interval. Observed monthly precipitation data from the
Climate Prediction Center (CPC) Merged Analysis of
Precipitation (CMAP) data (Xie and Arkin 1997) were
used to evaluate the modeled precipitation. This set of
experiments was performed to evaluate seasonal precipi-
tation and the intraseasonal component of the total inter-
annual variability of precipitation simulated by the model.
Similar to the SMIP-type run, two integrations with
the SAS and RAS cumulus parameterization schemes
were conducted for the eight extended boreal summers
[May–September (MJJAS)] from 1997 to 2004. Both
integrations were performed for each year as a single run
starting from 0000 UTC 1 May. The purpose of these
experiments was to investigate the characteristics of wave
propagation and intensity of the ISO simulated by the
model. Therefore, the experiment was set up for each
year for a period that was sufficiently long to extract the
bandpass-filtered properties from the simulated model
results. To evaluate the characteristics of the ISO, the
Global Precipitation Climatology Project (GPCP) Geo-
stationary Operational Environmental Satellite (GOES)
precipitation index (GPI) daily rainfall estimates (Huffman
et al. 2001) and daily NCEP/DOE Reanalysis 2 data
were used as input data for precipitation and atmospheric
structure, respectively.
3. Seasonal simulations
a. Evaluation of the boreal summer climate
To investigate whether the model simulated the mean
seasonal climate reasonably well, summer mean pre-
cipitation and large-scale features were analyzed, and
the results are presented in Fig. 1. Based on the CMAP
data (Fig. 1a), the observed rainfall is concentrated in
three major areas: the Asian monsoon region, the west-
ern North Pacific monsoon region, and the intertropical
convergence zone (ITCZ). The monsoonal precipitation
associated with the Asian summer monsoon occurs mainly
over the Indian Ocean. Furthermore, this rainfall area is
directly connected with the Somali jet across the Indian
subcontinent. The western North Pacific monsoon is re-
lated to the Indonesian branch of the Walker circulation
over the warm pool region, and produces enhanced trop-
ical precipitation. Finally, the observed equatorial rainfall
along the ITCZ over the Pacific is associated with the
low-level easterly convergence zone.
Both the EXP-SAS and EXP-RAS experiments sim-
ulated the above-observed features fairly well (Figs. 1b,c).
The EXP-SAS experiment reproduced tropical precipi-
tation over the ITCZ over the Pacific and over the At-
lantic Ocean (Fig. 1b), but there were discernible defects,
including excessive rainfall in the trade wind region north
of the equator and underestimated precipitation over
the equatorial western Pacific near the Maritime Con-
tinent. This latter feature is closely connected with the
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northward shift of the convergence area over the west-
ern Pacific Ocean. This major problem over the western
equatorial Pacific was largely corrected for when the
RAS scheme was used (Fig. 1c). The precipitation pattern
over the equatorial central Pacific Ocean was similar to
the observations; however, the amount of precipitation
was still exaggerated relative to the equatorial low-level
easterly convergence.
The simulated global precipitation climatology and
interannual variability were evaluated quantitatively
and are shown in Fig. 2. It is clear that for all summers,
the results from the EXP-SAS run had a larger bias and
FIG. 1. Seasonal mean distributions of precipitation (shading, mm day21) and 850-hPa
wind (vectors, m s21) averaged for the boreal summer (June–August) from 1979 to 2002. (a)
The CMAP and the NCEP/DOE Reanalysis 2 data, (b) the EXP-SAS experiment, and (c) the
EXP-RAS experiment. Shading denotes areas with precipitation .3 mm day21 at 3 mm day21
intervals.
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root-mean-square error (RMSE) than those from the
EXP-RAS run. As shown in Fig. 2b, it is evident that the
two experiments showed similar patterns with regard to
interannual variations of anomaly correlation coefficients
(ACCs) of seasonal mean precipitation. For example,
both simulations showed a higher coefficient in the main
El Nino years, for example, 1982, 1986, and 1997. TEXP-
RAS showed better skill in simulating the seasonal
anomaly of precipitation than EXP-SAS. The mean value
of the ACC during the whole SMIP period was 0.27 for
EXP-SAS and 0.34 for EXP-RAS.
b. Forced versus intraseasonal variability in theseasonal mean precipitation
This section addresses the relationship between the
intraseasonal oscillation and seasonal mean components
in determining the interannual variability of seasonal
mean precipitation. Several approaches, for example,
variance methods, have been used to decompose the
interannual variability of the seasonal mean field into
forced components by slowly varying boundary forcing
and other forcing types (e.g., Stern and Miyakoda 1995;
Rowell 1998; Zwiers 1996; Zheng et al. 2000; Zheng and
Frederiksen 2004). In particular, Zheng et al. (2000)
proposed a variance method to estimate the interannual
variability resulting from the weather noise component,
which is distinguishable from the annual variability re-
sulting from slowly varying components, such as the SST-
forced signal. In addition, Zheng and Frederiksen (2004)
reported that this weather noise component can be viewed
as the intraseasonal component of interannual variability
of the seasonal mean, because weather noise contributes
considerably to intraseasonal events. Therefore, we used
the method of Zheng et al. (2000) to decompose the
interannual variability of the seasonal mean into slowly
varying ‘‘forced’’ and ‘‘intraseasonal’’ components.
First, we assumed that the monthly mean of a variable
(x) for a particular season obtained over a number of
years (Y ) can be decomposed in the following linear
regression form,
xy,m
5 my
1 «y,m
(1)
Here, y (51, . . . , Y ) denotes the year, m (51, 2, or 3) is
the month within a given 3-month season, my is a sea-
sonal mean anomaly in year y resulting from slowly
varying external forcing (such as SST forcing) and in-
ternal dynamics (interannual/supraannual), and «y,m is
a residual monthly departure of xy,m from the seasonal
value my resulting from intraseasonal variability. The
residual component, which consists of («y,1, «y,2, «y,3), is
assumed to comprise a three-dimensional stationary
stochastic process and be statistically independent with
respect to year y. As in Zheng et al. (2000), an average
over m, or y, is indicated by replacing the appropriate
subscript with ‘‘o.’’ For example, xy,o represents a sam-
ple seasonal mean and xo,o is an average over all 3
months and Y years. Throughout this paper, we refer
to the components my and «y,o of the seasonal mean xy,o,
as the ‘‘forced’’ and ‘‘intraseasonal’’ components, respec-
tively. Zheng et al. (2000) derived the following estimate
of the interannual variance of the forced component V(my)
and intraseasonal component V(«y,o) at each grid point
V(«y,o
) 5V(«
y,1)[3 1 4C(«
y,1, «
y,2)]
9, (2)
V(my) 5 V(x
y,o)� V(«
y,o). (3)
Here, formulas for the estimation of (2) and (3) are listed
in Table 1. We calculated estimates using time series data
of the ensemble average for 10 members.
FIG. 2. Annual variation of (a) bias and rms error (mm day21)
and (b) anomaly correlation coefficients for summer precipitation.
The EXP-SAS run (closed circles) and EXP-RAS run (open cir-
cles) are denoted.
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Figure 3 shows the interannual variability of the ob-
served precipitation and its two decompositions, as cal-
culated using the methods described above. From Fig. 3,
it is obvious that the interannual variability of summer
precipitation depends to a significant extent on the in-
traseasonal variation as well as the forced component.
Because the slowly varying forced component depends
on tropical SST variability, the main correlation be-
tween the forced component and summer precipitation
variability occurs primarily over the ENSO mode region
over the equatorial eastern to central Pacific Ocean. It
is also apparent that the intraseasonal component af-
fects interannual variability over the western Pacific
area (including the Indian Ocean) more strongly than
does the forced component. The strong forced compo-
nent of variability in the Bay of Bengal appears to be
associated with dynamical forcing resulting from the
land–sea contrast. We realize that using Zheng et al.’s
(2000) method to separate forced and intraseasonal com-
ponents of the precipitation is not as robust as using other
meteorological fields. For example, part of the precipita-
tion over warm SSTs may arise because of enhanced in-
traseasonal activity in that region. Bearing in mind this
uncertainty, we feel that it is still useful to qualitatively
compare the two components of precipitation obtained
from the model experiments and observations.
In both experiments (Figs. 4 and 5), the overall pat-
terns of interannual variability were similar to the cor-
responding observations in Fig. 3. However, it is clear
that both simulations show a much stronger response to
the SST variation over the central Pacific than the actual
observations. In Fig. 4, the EXP-SAS case simulates
strong interannual variability in precipitation over the
eastern Pacific, which is closely related to the SST-
forced component. In contrast, the EXP-SAS run shows
weaker variability in the intraseasonal component over
the warm pool area, including the western Pacific and
Indian Oceans, than does the observation. Although the
EXP-RAS run generated a relatively similar pattern to
a forced component in the EXP-SAS run, the EXP-RAS
run produced a stronger intraseasonal component over
the warm pool area, which is more similar to what was
observed. The tabulated results show that the improve-
ment in the estimate of interannual variability in pre-
cipitation obtained from the EXP-RAS run compared to
the EXP-SAS run can be largely attributed to the more
accurate intraseasonal variability simulated by the EXP-
RAS run (Table 2).
To further evaluate the interannual variation in the
ISO activity, temporal correlation coefficients between
the annual ACCs of summer precipitation and the ob-
servational ENSO and ISO time series from 1979 to 2002
were examined (Table 3). In this study, the absolute value
of the Nino index was used to reflect the intensity of
variability caused only by ENSO. Furthermore, the OLR
time series was taken from the ;20–70-day bandpass-
filtered variance over the Indian Ocean. Table 3 shows
conclusively that the difference in seasonal predictability
of the two simulations is closely related to the difference
in the ISO signal between the two experiments. Corre-
lation coefficients associated with ENSO intensity show
that most of the seasonal predictability results from the
simulation skill of this SST-forced signal, and that this
forced component of interannual variability is well sim-
ulated in both of the experiments. However, the values
related with ISO intensity were significantly different
between the two experiments. The correlation coefficient
for ISO intensity was 20.15 in the EXP-SAS run and 0.16
in the EXP-RAS run.
Although the spatial distribution of the intraseasonal
component of the interannual variability of precipita-
tion was resolved better by the EXP-RAS experiment
than by the EXP-SAS experiment (Table 2), it is not
clear that the EXP-RAS run can simulate the ISO better
than the EXP-SAS run, because the temporal coefficients
associated with the ISO signal are relatively low (Table 3).
The characteristics of the simulated ISO are discussed
further in the following section.
4. Simulated intraseasonal oscillation
a. Analytical techniques
We used several techniques in this study to identify
the characteristics of the ISO simulated by the model.
First, the datasets from the model experiments and the
observational daily means were filtered using a ;20–
70-day Murakami bandpass filter (Murakami 1979) for
an 8-yr extended boreal summertime (MJJAS) to focus
on the ISO signal.
TABLE 1. Formulas for parameter estimates.
Parameter Formula
V(xy,o)1
Y � 1�Y
y51(xy,o � xo,o)2
C(«y,1, «y,2) 5 C(«y,2, «y,3) min 0.1, max 1.5� v1v2
, 0� �h i
C(«y,1, «y,3) 0
V(«y,m
), m 5 1, 2, 3�2v2C(«y,1, «y,2) 1 2v1
3� 4C(«y,1
, «y,2
)
v1
1
2Y�Y
y51�
3
m51x2
y,m � �m 6¼m2
xy,m1
xy,m2
0@
1A
v2
1
2Y�Y
y51(xy,1 � xy,3)2
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FIG. 3. Global distributions of observed summer mean precipitation (mm day21) re-
constructed by the method of Zheng et al. (2000): (a) interannual variability of CMAP,
(b) variability resulting from the forced component, and (c) variability resulting from the
intraseasonal component.
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FIG. 4. As in Fig. 3, but for the EXP-SAS run.
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FIG. 5. As in Fig. 3, but for the EXP-RAS run.
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In addition, a space–time spectral analysis was per-
formed to capture the characteristics of propagating
waves. This technique is useful for analyzing zonally
propagating waves, because it decomposes the time and
longitude-dependent data stream into wavenumber and
frequency components for eastward- and westward-
propagating waves as well as zonal-mean fluctuations
(Hayashi 1982). To prevent aliasing, a spectral analysis
was applied to the seasonal cycle–removed daily anom-
alies. The seasonal cycle for each particular year was
defined as the sum of the first two harmonics at each grid
point. After the seasonal cycles were removed, the mean
and linear trends of each segment were removed in time
by a least squares fit, and then the ends of the series were
tapered to zeros. Further, to reduce noise, the space–time
spectra were generated for 8 yr by applying a 30-day
overlap to successive 92-day data segments, as in Wheeler
and Kiladis (1999).
Although ordinary empirical orthogonal function
(EOF) analysis can determine stationary variability, it is
not appropriate for studying the ISO because EOF is
only applicable to stationary waves. We therefore ap-
plied complex empirical orthogonal function (CEOF)
analysis (Horel 1984; Yih and Kwon 2006) to the ;20–
70-day velocity potential fields to determine the domi-
nant propagating mode embedded in the datasets.
b. Comparison of the simulated ISO
The global distributions of the approximately 20–70-day
precipitation variance from the observations and sim-
ulations are compared in Fig. 6. Overall, the EXP-SAS
and EXP-RAS experiments showed similar patterns in
terms of dominant variance over the Indian Ocean and
the western Pacific region, compared to those from the
GPCP observation. However, the magnitude simulated
by both experimental runs was larger than the obser-
vation over these regions. Further, it is clear that the
EXP-SAS experiment exaggerates the variance along the
ITCZ over the central and eastern Pacific and the South
Pacific convergence zone (SPCZ) over the western Pacific.
The variance from the EXP-RAS run is closer to that
observed along the ITCZ and SPCZ; however, it is ob-
vious that the EXP-RAS run shows exaggerated vari-
ance over a broader region, from the Indian Ocean to
the western Pacific. The distribution of the approximately
20–70-day precipitation variance in Fig. 6 resembles the
seasonal precipitation in Fig. 1, indicating that the ISO
signals analyzed in this section comply with the signals in
the SMIP runs discussed in the previous section. Indeed,
the overall distribution of the 8-yr-averaged JJA pre-
cipitation was found to be close to what was shown in
Fig. 1 (data not shown).
The wave characteristics of the simulated ISO were
compared to those from the GPI observations in Fig. 7,
after applying wavenumber–frequency spectral analysis
to equatorial precipitation. In Fig. 7a, it is clear that the
dominant mode in the observations is the eastward-
propagating wave with a 46-day period and a wavenumber
of 1. This observational feature of ISO is consistent with
the results of many previous analyses that used outgoing
longwave radiation (OLR; e.g., Wheeler and Kiladis
1999) and precipitation (e.g., Zhang and Mu 2005; Lin
et al. 2006). In contrast, the EXP-SAS simulation (Fig. 7b)
generated a mainly stationary wave of zonal wave-
number 0, and its spectral peak occurred after a period
of 46 days. The dominant propagating mode for wave-
number 1 was the eastward-propagating wave with a
nearly 30-day period. In addition, the EXP-SAS run
showed a westward-propagating wave with a spectral
peak of a ;20–30-day period at wavenumber 4, which is
too strong, but may reflect an observed Rossby wave
frequency. The EXP-RAS case (Fig. 7c) generated a
stationary wave with a 46-day period, similar to the EXP-
SAS run, but its spectral power was larger at the peak than
that of the EXP-SAS experiment, with a longer period.
The dominant eastward-propagating mode simulated by
the EXP-RAS experiment was 1–2, with a 46-day period.
Westward-propagating waves were also generated in the
EXP-RAS run, with the wavenumber ranging between
2 and 4 and a period of approximately 20–30 days.
However, Jiang et al. (2004) reported that the
ISO in the boreal summertime has a significant
TABLE 2. Correlation coefficients for variance decomposition of
the simulated precipitation.
Experiments
Interannual
variability
Forced
component
Intraseasonal
component
EXP-SAS 0.77 0.69 0.76
EXP-RAS 0.81 0.70 0.82
TABLE 3. Temporal correlation coefficients between the annual
ACCs of summer precipitation and the observational ENSO and
ISO time series from 1979 to 2002. The coefficients from the two
simulations for the ENSO and ISO intensities are temporal corre-
lations calculated from the annual ACCs and a time series of ab-
solute values of the Nino-3.4 index, and the variance of ;20–70-day
bandpass-filtered OLR averaged over the Indian Ocean (approxi-
mately 58S–58N, approximately 708–808E), respectively. When these
values were different, the temporal correlation was calculated from
the time series of differences in the annual ACCs predicted by the
two experiments. Values with one or two asterisks indicate co-
efficients significant at the 99% or 90% levels, respectively.
Experiment ENSO intensity ISO intensity
EXP-SAS 0.70* 20.15
EXP-RAS 0.71** 0.16
Difference (RAS 2 SAS) 0.06 0.34*
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northward-propagating component. Therefore, the me-
ridional wavenumber–frequency spectra for precipitation
over the western Pacific region were calculated to analyze
propagating waves in the south–north direction; the re-
sults are presented in Figs. 7d–f. It is clear that the ob-
served GPI rainfall has a dominant wave component that
is propagated northward at the peak of 46-day period with
a meridional wavenumber of 1. Note that wavenumber 1
in Figs. 7d–f corresponds to the domain of approximately
108S–37.58N. Furthermore, the southward-propagating
component occurred at wavenumber 1 within the same
period, but with a weaker power than the northward
component. It is clear from Fig. 7e that the EXP-SAS case
is similar to the GPI spectra. However, the two propa-
gating modes in the northward and southward directions
tend to have shorter periods than those in the GPCP GPI
data. In the EXP-RAS simulation (Fig. 7f), it was ap-
parent that the dominant northward-propagating wave
FIG. 6. The 20–70-day precipitation variance (mm2 day22) averaged for 8 yr from 1997 to 2004.
(a) GPI observation, (b) the EXP-SAS run, and (c) the EXP-RAS run.
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FIG. 7. Wavenumber–frequency power spectra of average precipitation for the boreal summers from 1997 to 2004.
(left) Zonal wavenumber spectra averaged over approximately 158S–158N for (a) GPI data, (b) the EXP-SAS run,
and (c) the EXP-RAS run are denoted. (right) Meridional wavenumber spectra averaged over ;1008–1508E for
(d) GPI data, (e) the EXP-SAS run, and (f) the EXP-RAS run are also indicated.
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occurred at the same wavenumber and period, but its
spectral power was exaggerated. The EXP-RAS experi-
ment, however, did not clearly distinguish the southward-
propagating wave with wavenumber 1 from the northward
waves, in contrast to the EXP-SAS run.
To better visualize the ISO-related wave characteris-
tics in large-scale circulation, CEOF analysis was applied
to the 200-hPa velocity potential fields from NCEP/DOE
Reanalysis 2 data and two model simulations (Fig. 8). The
velocity potential field was chosen for the analysis of
MJO signal because it can represent the global distri-
bution of upper-level divergence-associated convective
activities. The first CEOF extracted from the obser-
vation accounted for 50% of the total approximately
20–70-day variance, whereas the first modes from the
EXP-SAS and EXP-RAS experiments accounted for 34%
and 36% of the total approximately 20–70-day variance,
respectively. The first modes were well separated from
the other modes, satisfying the criteria of North et al.
(1982), even though the percentages from the model
simulations were smaller than observation percentages.
Nevertheless, Fig. 8 clearly demonstrates that the first
CEOF mode of the 200-hPa velocity potential from the
EXP-RAS run is closer to the observation at day 46 as
compared to the approximately 20–30 days in the case of
the EXP-SAS run, which is consistent with the precipi-
tation analysis in Fig. 7.
Composite fields taken from the first CEOF mode were
constructed to investigate the spatial features of the ISO.
In Fig. 9, the composite velocity potential anomalies for
each phase from 08 to 2708 are shown; the whole phase
range corresponds to the period of the dominant modes
shown in each case. At a 08 phase angle (top panel), the
positive anomaly of the 200-hPa velocity potential (con-
vergence area) appears over the entire Pacific Ocean,
with its maximum at the western Pacific. Furthermore,
the divergence region (negative anomaly of the 200-hPa
velocity potential) covers a broad area from the Atlantic
to the Indian Oceans. In the next phase (second panel),
the divergence area has moved to the Indian Ocean,
whereas the convergence area has moved to the eastern
Pacific. It is clear that the anomaly fields in phase angle
1808 (third panel) show a pattern opposite to that of phase
angle 08 (top panel); similarly, phase angle 2708 (bottom
panel) is the reverse of phase angle 908 (second panel).
The composite velocity potential anomalies from the
two experiments captures the global propagation of the
ISO as atmospheric responses to convective perturba-
tions well; this global propagation is characterized by a
convectively forced Kelvin–Rossby wave moving east-
ward from the western Indian Ocean to the western Pa-
cific with a slow phase speed of about 5 m s21, and a fast
dry Kelvin wave moving from the central Pacific to the
eastern Pacific with a fast phase speed of about 30 m s21
(e.g., Madden and Julian 1972; Salby and Hendon 1994;
Weickmann et al. 1997; Matthews 2000). However, al-
though both experiments agreed qualitatively with the
observations, the two simulations showed faster move-
ment of the convection core (negative anomalies) from
phase angle 908 to 1808 than what was observed. A close
inspection revealed that results from the EXP-RAS were
more realistic in terms of maximum amplitudes and their
locations at each phase than the EXP-SAS run. For ex-
ample, the amplitude of the negative velocity potential
anomaly from the EXP-RAS run was strongest at phase
angle 908, which is consistent with the observed data, but
this negative velocity potential anomaly appeared only in
the next phase in the EXP-SAS run.
5. Summary and concluding remarks
We examined the simulated boreal summer climate
from 1979 to 2002 using a GCM with two different con-
vective parameterization schemes—the SAS and RAS
algorithms—on a SMIP-type integration test bed. The
characteristics of wave propagation and intensity of the
ISO simulated in extended boreal summers from 1997 to
2004 by the model with two convection schemes were
investigated. The possible link between ISO simulation
and dynamical seasonal prediction was also discussed.
The simulated global precipitation climatology and
interannual variability show that both experiments cap-
ture the global precipitation climatology, and interannual
variability fairly well, but RAS outperforms SAS in terms
of bias, root-mean-square error, and anomaly correlation
coefficients. Decomposition of the interannual variability
of summer precipitation into two components indicated
FIG. 8. Power spectra for time series of the first CEOF mode of
the 200-hPa velocity potential. The NCEP/DOE Reanalysis 2 data
(solid lines), and the EXP-SAS (dotted lines) and the EXP-RAS
(dashed lines) experiments are denoted.
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that the observed interannual variability of the summer
mean precipitation is dominated by the intraseasonal
component over the warm pool area and the SST-forced
signal prevailing over the equatorial Pacific Ocean. The
major difference between the two model simulations is
the interannual variability over the warm pool area,
which is associated with differences in the simulation of
the intraseasonal component. The temporal correlation
coefficients between the annual anomaly correlation co-
efficients of summer precipitation and the observational
ENSO and ISO time series also indicate that most of the
seasonal predictability results from the simulation skill
of the SST-forced signal, and the difference in seasonal
predictability of the two simulations is closely related to
the difference in the ISO signal, although the significance
of this is relatively low.
When we compared the simulated ISO values, we
found that the global distributions of the approximately
20–70-day precipitation variance and the wave character-
istics of the simulated ISO were fairly well reproduced by
the model regardless of the convection scheme. However,
the power spectra for the time series of the first CEOF
FIG. 9. Composite of the 200-hPa velocity potential anomalies (106 m2 s21) taken from (top) the NCEP/DOE Reanalysis 2, (left) the
EXP-SAS run, and (right) EXP-RAS run. Segments are separated by 908, with phase angles increasing from top to bottom.
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mode of the 200-hPa velocity potential were closer to
the observed data on day 46 in the RAS run than the
SAS run. The composite fields of the 200-hPa velocity
potential taken from the first CEOF mode revealed that
the global propagation of the ISO as atmospheric re-
sponses to convective perturbations was well reproduced
by both experiments, but the RAS run outperformed the
SAS run in terms of the amplitude of anomalies.
It is not clear from the model results for seasonal
prediction and ISO simulation that accurate ISO simu-
lation guarantees improved seasonal predictability of
boreal summer precipitation, even though some ana-
lyses imply that better ISO simulation can result in better
seasonal prediction. Nevertheless, it is possible to con-
clude that accurate simulation of the ISO is an important
factor toward an improvement of seasonal predictabil-
ity. Traditionally, the predictability of the dynamical
seasonal prediction model has been assessed based on
evaluation of the seasonal mean climate and interannual
variability in the model simulation. However, we have
shown in this study that the seasonal predictability of the
dynamical climate model is also closely related to its
ability to simulate intraseasonal variability accurately. It
is again important to note that the purpose of this re-
search was not to judge the superiority of one algorithm
over another, but to examine the role of intraseasonal
variability in accurate seasonal prediction. For example,
the seasonal mean tropical precipitation simulated by the
SAS run was closer to the actual observations than the
precipitation simulated by the RAS scheme when the re-
vised vertical diffusion scheme was employed (Byun and
Hong 2004), indicating that further improvements in the
physical parameterizations of GCMs are likely to improve
climate prediction.
Acknowledgments. This research was supported by
project NIMR-2009-B-2 of the National Institute of
Meteorological Research in Korea Meteorological Ad-
ministration, and by the Basic Science Research Program
through the National Research Foundation of Korea
(NRF) funded by the Ministry of Education, Science
and Technology (2010-0000840).
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