Computer Science
Scientific paper
Apr 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.338..321s&link_type=abstract
In ESA, Symposium on Titan p 321-323 (SEE N92-32348 23-91)
Computer Science
2
Ethane, Methane, Ocean Surface, Surface Waves, Titan, Wave Generation, Wind Velocity, Cassini Mission, Ground Wind, Oceans, Satellite Atmospheres, Space Probes
Scientific paper
A preliminary look at the possibility of surface waves existing on Titan, assuming it possesses an ethane/methane ocean, is taken. The properties of the waves are deduced using well understood theory and compared with the properties of waves on the Earth's oceans. Our calculations show that the lack of knowledge of surface wind speed on Titan produces the greatest uncertainty in the expected wave properties.
Challenor Peter G.
Green Simon F.
Srokosz Meric A.
Zarnecki John C.
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