Which Way Does the Wind Blow? Titan's Zonal Circulation

Details Which Way Does the Wind Blow? Titan's Zonal Circulation Which Way Does the Wind Blow? Titan's Zonal Circulation

Jul 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997dps....29.3306k&link_type=abstract

American Astronomical Society, DPS meeting #29, #33.06; Bulletin of the American Astronomical Society, Vol. 29, p.1038

Astronomy and Astrophysics

Astronomy

Scientific paper

Knowledge of the direction and magnitude of Titan's circulation is important for the Cassini Huygens Probe mission and for constraining dynamical models of slowly rotating bodies. Ethane emission lines from Titan's stratosphere were measured with a spectral resolving power of ~ 10(7) using the Goddard Infrared Heterodyne Spectrometer at the NASA Infrared Telescope Facility on Mauna Kea, Hawaii in August 1993, October 1995 and September 1996. A comparison of the retrieved line center frequencies of the resolved lineshapes from the east and west hemispheres of Titan provides a measure of the direction and a mean magnitude of the speed of the circulation in the 7--0.1 mbar pressure altitude regions (120--350 km). The relative Doppler shift of the lines from the two hemispheres yields a prograde wind direction and an average limb-to-limb magnitude of ~ 140 m/sec ( ~ 70 m/sec horizontal). The instrumental stability permits absolute measurements to <= 10 m/s, while the signal-to-noise on the data limits the limb-to-limb uncertainty to ~ 100 m/sec. Recent improved analyses and interpretation will be discussed.

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