A first tentative trial to produce a forecast using the laws of physics was made by Felix Exner
(1908), working in Vienna. His efforts yielded a realistic forecast for the particular case that
he chose. Despite the restricted applicability of his technique, his work was a first attempt at
systematic, scientific weather forecasting. However, it involved some drastic simplifications
and was far from providing anything of use for practical forecasting.
Weather Prediction by Numerical Process
Lewis Fry Richardson first learned of Bjerknes’ plan for rational forecasting in 1913, when
he took up employment with the Meteorological Office. Richardson’s forecasting scheme
amounts to a precise and detailed implementation of the prognostic component of Bjerknes’
programme. It is a highly intricate procedure: as Richardson observed, “the scheme is
complicated because the atmosphere is complicated.” It also involved an enormous volume
of numerical computation and was quite impractical in the pre-computer era. But Richardson
was undaunted, expressing his dream that “some day in the dim future it will be possible to
advance the computations faster than the weather advances.”
Earlier, Richardson had applied an approximate numerical method to the solution of par-
tial differential equations to investigate the stresses in masonry dams. He realized that this
method had potential for use in a wide range of problems. The idea of numerical weather
prediction appears to have germinated in his mind for several years. Around 1911, Richard-
son had begun to think about the application of his approach to the problem of forecasting
the weather. He stated in the Preface of WPNP that the idea “grew out of a study of finite
differences and first took shape in 1911 as a fantasy.” The fantasy was that of a forecast
factory, which we will discuss below.
Upon joining the Met Office, Richardson was appointed Superintendent of Eskdalemuir
Observatory in the Southern Uplands of Scotland and began serious work on numerical
forecasting. In May 1916 he resigned from the Met Office in order to work with the Friends
Ambulance Unit in France. By this time, he had completed the formulation of his scheme
and had set down the details in the first draft of his book. But he was not concerned merely
with theoretical rigour and wished to include a fully worked example to demonstrate how
the method could be put to use.
Richardson assumed that the state of the atmosphere at any point could be specified by seven
numbers: pressure, temperature, density, water content and velocity components eastward,
northward and upward. He formulated a description of atmospheric phenomena in terms of
seven partial differential equations. To solve them, he divided the atmosphere into discrete
columns of extent 3 degrees east-west and 200 km north-south, giving 120×100 = 12,000
columns to cover the globe. Each of these columns was divided vertically into five cells. The
values of the variables were given at the centre of each cell, and the differential equations
were approximated by expressing them in finite difference form. The rates of change of the
variables could then be calculated by arithmetical means. These rates enabled Richardson
to calculate the variables at a later time.
Richardson calculated the initial changes over a six hour period in two columns over central
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