The Cosmic Radiation Environment Dosimetry experiment is providing data on
particle fluxes and linear energy transfer spectra for inner belt protons,
cosmic rays and solar particles in order to correlate with device behaviour
in the MPTB experiments and to provide tests of environment models. Partic
le fluxes are related to geomagnetic co-ordinates in order to explain the o
bserved time variations around the orbit and the differences between odd an
d even orbits. Cosmic-ray fluxes are slowly decreasing as solar maximum is
approached. Outer-belt electrons show large variations and are particularly
enhanced during late August to November 1998. Several solar particle event
s have been observed. Integral linear energy transfer (LET) spectra for the
se show both lower intensities and a lack of enhancement at high values of
LET when compared with the October 1989 event which is commonly used as a w
orst case.