In this study the behavior of a linear, intermediate model of ENSO is exami
ned under stochastic forcing. The model was developed in a companion paper
(Part I) and is derived from the Zebiak-Cane ENSO model. Four variants of t
he model are used whose stabilities range from slightly damped to moderatel
y damped. Each model is run as a simulation while being perturbed by noise
that is uncorrelated (white) in space and time. The statistics of the model
output show the moderately damped models to be more realistic than the sli
ghtly damped models. The moderately damped models have power spectra that a
re quantitatively quite similar to observations, and a seasonal pattern of
variance that is qualitatively similar to observations. All models produce
ENSOs that are phase locked to the annual cycle, and all display the "sprin
g barrier'' characteristic in their autocorrelation patterns, though in the
models this "barrier'' occurs during the summer and is less intense than i
n the observations (inclusion of nonlinear effects is shown to partially re
medy this deficiency). The more realistic models also show a decadal variab
ility in the lagged autocorrelation pattern that is qualitatively similar t
o observations.
Analysis of the models shows that the greatest part of the variability come
s from perturbations that project onto the first singular vector, which the
n grow rapidly into the ENSO mode. Essentially, the model output represents
many instances of the ENSO mode, with random phase and amplitude, stimulat
ed by the noise through the optimal transient growth of the singular vector
s.
The limit of predictability for each model is calculated and it is shown th
at the more realistic (moderately damped) models have worse potential predi
ctability (9-15 months) than the deterministic chaotic models that have bee
n studied widely in the literature. The predictability limits are strongly
correlated with the stability of the models' ENSO mode-the more highly damp
ed models having much shorter limits of predictability. A comparison of the
two most realistic models shows that even though these models have similar
statistics, they have very different predictability limits. The models hav
e a strong seasonal dependence to their predictability limits.
The results of this study (with the companion paper) suggest that the linea
r, stable dynamical model of ENSO is indeed a plausible hypothesis for the
observed ENSO. With very reasonable levels of stochastic forcing, the model
produces realistic levels of variance, has a realistic spectrum, and quali
tatively reproduces the observed seasonal pattern of variance, the autocorr
elation pattern, and the ENSO-like decadal variability.