RUBIDIUM ULTRA-STABLE OSCILLATORS AT TITAN: THE HUYGENS DOPPLER WIND EXPERIMENT

The Doppler Wind Experiment (DWE) is one of six investigations to be per- formed during the Titan atmospheric descent of the ESA Huygens Probe. The primary scientific objective is to measure the direction and strength of Titan's zonal winds with an accuracy better than 1 m s ' 1 . The Probe's wind-induced horizontal motion will be derived from the residual Doppler shift of its S-band radio link to the Cassini Orbiter, corrected for all known orbit and propagation effects, from the beginning of the mission (altitude: w160 km) down to impact on the surface. The DWE Instrumentation consists of Rbbased Ultra-Stable Oscillators used to (a) generate the transmitted signal from the Probe and (b) extract the frequency of the received signal on the Orbiter. The capabilities of these USOS under the rugged experimental conditions on Titan and some results from the DWE pre-launch test program are described.