Physics
Scientific paper
Feb 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004esasp.544..109d&link_type=abstract
In: Proceedings of the International Workshop Planetary Probe Atmospheric Entry and Descent Trajectory Analysis and Science, 6-9
Physics
1
Titan Atmosphere, Entry Probes, Huygens
Scientific paper
A Doppler Wind Experiment (DWE) will be performed during the Titan atmospheric descent of the ESA Huygens Probe. The direction and strength of Titan's zonal winds will be determined from the start of mission at an altitude of ~160 km down to the surface. 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. We present an error analysis with the purpose of determining the largest error sources and some simulation results.
Bird Michael K.
Dutta-Roy Robindro
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