Saturn Probe Doppler Wind Experiment

Details Saturn Probe Doppler Wind Experiment Saturn Probe Doppler Wind Experiment

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1399a&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1399

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A Saturn probe Doppler Wind Experiment will be comparable to the Galileo Jupiter Doppler wind methodology. Measurement of the Saturn zonal wind structure will depend on a mission design that includes a rapidly varying probe/carrier (receiver) geometry, preferably including probe meridian crossing by the carrier. The only hardware requirements are ultrastable oscillators on both the probe (transmitter) and carrier (receiver) sides of the radio link, a significantly smaller cost than most instruments comprising the probe science payload. The relatively low cost, and small impact on the mass EPSC Abstracts Vol. 6, EPSC-DPS2011-1399-1, 2011 EPSC-DPS Joint Meeting 2011 c Author(s) 2011 and power budget required to perform the Saturn probe Doppler wind measurement provides a very high science return and makes the Saturn probe Doppler Wind Experiment an attractive option for enhancing total mission science return with minimal impact on mission resources (mass and cost) and mission design.

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