Solar protons present a major problem to space systems because of the
ionisation and displacement effects which arise from their interaction
with matter. This is likely to become a greater problem in the future
due to the use of more sensitive electronic components and the propos
ed expansion of manned activities in space. An outline is provided of
the physical processes associated with individual solar events, the so
lar activity cycle and the transport of solar particles between the Su
n and the Earth. The problems of predicting solar event fluences, both
over short- and long-term periods, are discussed. The currently avail
able solar proton event models used for long-term forecasting are brie
fly reviewed, and the advantages and deficiencies of each model are in
vestigated. Predictions using the models are compared to measurements
made by the GOES-7 satellite during the rising phase of the current so
lar cycle. These measurements are also used to illustrate the sensitiv
ity of the models to the choice of confidence level and to the spectra
l form used for extrapolation over the solar proton energy range.