P. G. Weber
Los Alamos National Laboratory
The instruments of the Cloud and Earth Radiant Energy System (CERES) are intended to provide the Earth Observing System (EOS) with continued long-term measurement
of the Earth's radiation budget. The CERES instruments are a pair of broadband, scanning radiometers based on the Earth Radiation Budget Experiment (ERBE)
scanners (EOS 1990, Stowe et al. 1990). There are three spectral channels in each radiometer: total radiance (0.2 to > 100 mm), shortwave (0.2 to 3.5
m) and
longwave (6.5 to 25
m), defined using filters. The detectors are thermistor bolometers, which are to operate at a constant 375C. The operating principle is
that of an active cavity radiometer; namely, the heat required to main-tain the temperature of the active cavity relative to a reference cavity determines
the thermal flux collected. The instrument view angle is to be 82
(half angle) about nadir, while the instantaneous field-of-view (IFOV) will be about a 35
pixel centered at the optical axis corresponding to a 25 x 35-km footprint at nadir from a polar platform.