The signals from the Cassini spacecraft that will be used for radio science
experiments will be affected by delay fluctuations in the Earth's atmosphe
re. These fluctuations are dominated by water vapor in the troposphere, and
in the case of the gravitational wave experiment (GWE), they are likely to
be a limiting error source. A passive remote sensing system, centered arou
nd a water vapor radiometer (WVR), has been developed to provide calibratio
ns of water vapor fluctuations during radio science experiments. During the
past two years, most of the technical challenges involved in the design of
this instrument have been overcome and we are ready to begin implementatio
n. We will discuss the performance that has been demonstrated with the curr
ent generation of WVR instrumentation and the general design of the package
that will be installed at the Goldstone tracking site. In addition, recent
results obtained for a comparison of co-located WVRs and global positionin
g system (GPS) receivers will be presented. The possibility of using these
results to estimate gradients and/or fluctuations in the dry atmosphere wil
l be discussed. (C) 1998 Elsevier Science Ltd. All rights reserved.