The Cassini/Huygens Doppler Wind Experiment: Results from the Titan Descent

M K Bird; R Dutta-Roy; M Allison; S W Asmar; D H Atkinson; P Edenhofer; D Plettemeier; G L Tyler

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NASA NTRS · 20050166927

The Cassini/Huygens Doppler Wind Experiment: Results from the Titan Descent

M K Bird·R Dutta-Roy·M Allison·S W Asmar·D H Atkinson·P Edenhofer·D Plettemeier·G L Tyler

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Abstract

The primary objective of the Doppler Wind Experiment (DWE), one of the six scientific investigations comprising the payload of the ESA Huygens Probe, is a determination of the wind velocity in Titan's atmosphere. Measurements of the Doppler shift of the S-band (2040 MHz) carrier signal to the Cassini Orbiter and to Earth were recorded during the Probe descent in order to deduce wind-induced motion of the Probe to an accuracy better than 1 m s-1. An experiment with the same scientific goal was performed with the Galileo Probe at Jupiter. Analogous to the Galileo experience, it was anticipated that the frequency of the Huygens radio signal could be measured on Earth to obtain an additional component of the horizontal winds. Specific secondary science objectives of DWE include measurements of: (a) Doppler fluctuations to determine the turbulence spectrum and possible wave activity in the Titan atmosphere; (b) Doppler and signal level modulation to monitor Probe descent dynamics (e.g., spinrate/spinphase, parachute swing); (c) Probe coordinates and orientation during descent and after impact on Titan.

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M K Bird, R Dutta-Roy, M Allison, S W Asmar, D H Atkinson, P Edenhofer, D Plettemeier, G L Tyler. 2005-01-01. The Cassini/Huygens Doppler Wind Experiment: Results from the Titan Descent. https://ntrs.nasa.gov/citations/20050166927

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