The current standard models of tile radiation-belt environment have ma
ny shortcomings, not the least of which is their extreme age, Most of
the data used for them were acquired in the 1960's and early 1970's, P
roblems with the present models, and the ways in which data from more
recent missions are being or can be used to create new models with imp
roved functionality, are described. The phenomenology of the radiation
belts, the effects on space systems, and geomagnetic coordinates and
modeling are discussed, Errors found in present models, their function
al limitations, and problems with their implementation and use are det
ailed, New modeling must address problems at low altitudes with the so
uth Atlantic anomaly, east-west asymmetries and solar cycle variations
, and at high altitudes with the highly dynamic electron environment,
The important issues in space environment modeling from the point of v
iew of usability and relationship with effects evaluation are presente
d, New sources of data are discussed, Future requirements in the data,
models, and analysis tools areas are presented.