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1 . Introduction
The existence of balance is fundamental to the
dynamics and predictability of the atmosphere. Atmospheric motion is dominated
not by rapid fluctuations associated with sound and gravity waves, but rather
by the more slowly changing weather systems. Over much of the globe these
are close to the familiar state of geostrophic balance in which winds blow
parallel to contours of constant geopotential height on an isobaric surface
(Fig. 1 ).
Figure 1 . The operational ECMWF
analysis of height and wind at 500hPa for 12 UTC 13 April 1997.
Faster wave motions are, however, excited if the atmosphere
is suddenly disturbed. The massive volcanic eruption of Krakatau (between
Java and Sumatra) in1883 excited a wave whose propagation could be traced
in the surface pressure field around to the antipodal point and back to
the source (Fig. 2 ). The signal took about 35 hours
to complete its outward and return trip, moving at about 320 ms-1,
around the speed of sound. This was what has come to be known as a Lamb
wave, or in numerical weather prediction as an external gravity wave. More
commonly, and on a much smaller scale, propagating internal gravity waves
may be excited by intense convective systems. Fig. 3 presents observations of wave structure
in mid-tropospheric temperature and wind fields over Japan apparently associated
with the occurrence of exceptionally heavy rainfall.
Figure 2 . Position at two-hourly
intervals of the surface-pressure wave excited by the volcanic eruption
of Krakatau, from Taylor(1929).
Figure 3 . Fine-scale structure
in temperature at 500hPa (left) and wind at 550hPa (right) over Japan at
12UTC on 1 July 1971, from Ninomiya (1983)
Numerical weather prediction models mostly assume hydrostatic
balance, and thus do not support the existence of sound waves. They are
generally based, however, on the primitive equations of motion, and Lamb
and internal gravity waves can be excited in these models. In particular,
they will be excited in data assimilation if the system uses observations
in such a way as to produce analyses in which the balance present in the
background state is disturbed. The waves in this case contaminate the short-range
forecast that provides the background state for the next analysis, adding
to the difficulty of extracting useful information from the observations.
The primary control of gravity waves in a modern data assimilation
system is through the multivariate formulation of the analysis. In such
a system, an observation of surface pressure or temperature that differs
from the background will generally result in an analysis which differs from
the background not only in surface pressure and temperature, but also in
wind, thus preventing an unrealistic deviation from geostrophic balance.
This aspect of the control of gravity waves is not the main concern of these
lecture notes, although we shall return to the topic briefly later. Rather,
we shall be concerned mostly with what is known as the process of initialization.
The term initialization is usually used to refer to the
adjustment of analysed initial model conditions to prevent excessive gravity-wave
activity in the subsequent forecast. This dynamical initialization
is needed if the multivariate formulation of the analysis is unable to provide
an adequate balance throughout the model domain. This is the type of initialization
that will be discussed here. More widely, initialization may be defined
as an adjustment of the initial conditions either to maintain dynamical
or physical balance or to satisfy some physical constraint. Thus it could
include the adjustment of fields to ensure that relative humidities lie
in the range from 0 to 100%, or the adjustment of fields to ensure that
initial rainfall rates match estimates from observations. This is referred
to as physical initialization.
Although the principal use of dynamical initialization
is to remove imbalance introduced during the analysis step in data assimilation,
it has additional applications in numerical weather prediction. It is often
used to remove imbalance in an initial state in which the model resolution
or orography has been changed, for example in:
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• Incremental variational
data assimilation (as discussed later); |
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• Creating initial conditions
for ensemble prediction based on a model with resolution lower than
that of the model used in the data assimilation; |
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• Testing of a new higher
resolution version of a model or new specification of orography. |
Initialization may also be used to remove imbalance when
running forecasts from analyses produced by other forecasting centres. This
is done occasionally to investigate forecasting failures and is under investigation
in the context of ensemble prediction.
Some further characteristics of atmospheric motion must
be taken into account in considering the topic of initialization. A rich
structure of largely stationary gravity-wave motion may be excited by flow
over orography. Fig. 4 shows a classical example. These waves
can have an important direct effect on the tropospheric circulation, and
together with the convectively-excited waves play a critical role in aspects
of the circulation of the stratosphere and mesosphere. Their effects are
in general parametrized in large-scale models, but they are coming increasingly
to be resolved directly in limited-area and finer-resolution global models,
and are a target for short-range mesoscale prediction. They should not be
unduly suppressed by initialization.
Figure 4 . Section of potential
temperature crossing the Rocky Mountains in Colorado, for 17 February 1970,
from Lilly and Kennedy (1973).
Tidal motion in the atmosphere is a form of forced gravity-wave
motion which also should not be suppressed by initialization. The strong
semi-diurnal component at the surface is forced by the daily variation in
solar heating of the stratosphere, dominating the more strongly-forced diurnal
component due to differences in downward propagation. It is seen in quite
pronounced oscillations in surface pressure in the tropics and subtropics
(Fig. 5 and Fig. 17 ) and needs to be handled well if
other signals in the observations are to be interpreted effectively. Moreover,
the quasi-steady tropical circulation systems (as illustrated schematically
in Fig. 6 ) characteristically involve a balance
between diabatic heating (or cooling) and the adiabatic cooling (or heating)
associated with vertical motion. Care is needed to ensure that initialization
does not produce analyses in which these circulations are weakened.
Figure 5 . The semi-diurnal tide.
The upper plot shows surface pressure (hPa) and the lower plot the tendency
of pressure (hPa/hour) at the lowest model level. The quantity plotted is
where denotes the mean ECMWF analysis at UTC for January 1997, truncated spectrally at T10 to remove local
orographic and station-specific features. Solid contours denote positive
values and dashed contours negative values. The nature of atmospheric tides
is described in Chapman and Lindzen (1970).
Figure 6 . Schematic view of the
mean tropospheric circulation in the equatorial plane, from
Webster(1983).
The method of non-linear normal-mode initialization that
has been used extensively at ECMWF to initialize its global models is described
in the following section. The way gravity waves are controlled in the Centre's
variational data assimilation system is described and illustrated in section
3. An alternative approach to initialization, that of digital filtering,
has been developed in recent years, particularly for application in limited-area
models. An introduction to this method is given in section 4.
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