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The clouds and radiation group is responsible for improving the
representation of solar and infrared (thermal) radiation as well as
prediction of cloud and precipitation in both forecast and climate
models.
The most important issue faced by the team is the representation of
clouds on scales smaller than the model resolution, where unresolved
physical processes and variations in conditions must be taken into
account. This forms a significant amount of the work undertaken by
the group.
Cloud microphysics and radiation parametrizations used at the Met
Office are based firmly on observational evidence and physical theory.
For example, cloud physics parametrizations are developed using aircraft,
satellite, balloon and radar observations in conjunction with the
latest theoretical ideas.
Simplified modelling tools, such as the single column model, are also
used for parametrization development and help determine the numerical
stability of parametrizations. The group works to draw together the
varied information from these data sources to produce robust and simple
representations of the relevant processes.
The important task of evaluation of the model predictions for cloud
and radiation forms a large part of the external collaboration with
non-Met Office groups. A number of novel ways to infer cloud properties
from satellite or radar and lidar data can be used to evaluate the
predicted structure of clouds. Similarly, data from the model may
be used to simulate observations, such as radiances. Evaluation of
the operational model is also conducted via regular consultation with
forecasters.
The representation of radiation in the model is evaluated against
detailed line-by-line radiation codes. The full solution of the three-dimensional
radiative transfer problem, even in the absence of clouds, is computationally
expensive and too slow for an atmospheric model to use. This means
that approximation techniques need to be developed in order to speed
up the scheme. Such techniques include the assumption that radiation
can be modelled as vertical fluxes in model columns, across a number
of frequency bands, rather than individual lines.
Find out more
about the large-scale cloud and precipitation parametrization.
Find out
more about the radiation parametrization.
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