In this paper, we consider two types of
prediction. Following Lorenz
(1975), we refer to initial value problems as 'predictions of the first
kind'. By contrast, forecasts which are not dependent on initial conditions,
for example predicting changes in the statistics of climate as a result
of some prescribed imposed perturbation, would constitute a 'prediction
of the second kind'. A weather forecast is clearly a prediction of the first
kind; so is a forecast of El Niño, referred to as a climate prediction
of the first kind. By contrast, estimating the effects on climate of a prescribed
volcanic emission, prescribed variations in Earth's orbit (thought to cause
ice ages) or prescribed anthropogenic changes in atmospheric composition,
would constitute a climate prediction of the second kind.
In Section
2, we consider how to forecast uncertainty in a prediction of the first
kind, assuming a perfect deterministic forecast model. The evolution equation
for the probability density function (pdf) of the climate state vector is
the Liouville equation; an example of its solution is given for illustration.
However, application to the real climate system is severely hampered by
two fundamental problems. The first is directly associated with the dimensionality
of the climate equations; as mentioned above, current numerical weather
prediction models comprise O(107) individual scalar variables.
The second problem (not unrelated to the first) is that, in practice, the
initial pdf is not itself well known.
To amplify on this last remark, a description
of current (variational) meteorological data assimilation schemes is described
in Section 3. These schemes
are used to determine initial conditions for weather and climate forecasts,
given a set of atmospheric and oceanic observations whose density is heterogeneous
in both space and time. Such data assimilation schemes are based on minimising
a cost function which combines these observations with a background estimate
of the initial state provided by a short-range model forecast from an earlier
set of initial conditions. In principle, given Gaussian error statistics,
the Hessian or second derivative of the cost function determines the initial
pdf. In practice, there are significant shortcomings in our ability to estimate
this pdf.
A theoretical framework for describing error
growth is developed in Section
5. Two common measures of perturbation amplification used in different
branches of physics and mathematics are normal mode growth and Lyapunov
exponent growth. Neither is well suited to describing error growth in the
climate system. Firstly, because of the advective nonlinearity in the governing
equations of motion, the linearised dynamical operators are not normal;
as such, over finite times, perturbation growth need not be bounded by the
fastest eigenmode growth. Also, dominant Lyapunov or eigenmode growth in
a comprehensive multi-scale model may refer to fast instabilities (such
as convective instabilities) whose spatial scales are much smaller than
those describing weather or climate phenomena. To address these problems,
we discuss in Section 5
a general formulation of perturbation growth in the linearised approximation,
in terms of a singular value decomposition of the linearised dynamics (building
on the developments in Section
3). Examples of singular vectors for weather and climate prediction
problems are shown, and their fundamental non-modality is discussed. Because
of the nonlinearity of the underlying dynamics, the appropriate singular
values vary on the attractor; this variation describes why forecast error
can fluctuate for fixed initial error. The variation of singular values
on the attractor is also relevant for understanding the amplification of
model error by flow dependent instabilities. The relationship between singular
values, eigevalues and Lyapunov exponents is discussed.
Section
6 discusses some applications of the singular vector analysis. In one
application ('chaotic control of the observing system') singular vectors
are used to determine locations where additional 'targeted' observations
might significantly improve a forecast's initial state.
Section
7 describes the basis behind attempts to predict uncertainty in daily,
seasonal and climate change forecasts using ensembles of atmosphere or coupled
ocean-atmosphere model integrations. In practice such ensembles are interpreted
in probabilistic form. If the ensemble of forecast phase-space trajectories
evolve though a relatively stable part of the climate attractor, then resulting
probability forecasts will be relatively sharp. Conversely, if the ensemble
passes through a particularly unstable part of the attractor, then the corresponding
forecast probability may be little different from a long-term climatological
frequency.
The question of how to validate probability
forecasts is discussed in Section
8. Two particular techniques are described. The first is based on a
root mean square distance between the probability forecast of a dichotomous
event and the corresponding verification. This measure allows one to formulate
the notion of reliability of probability forecasts. The second quantity
measures the so-called hit and false alarm rate of the forecast of a dichotomous
event, assuming that the event is forecast if the predicted probability
exceeds some prescribed probability threshold.