Dynamic of the liquid masses on Titan

Details Dynamic of the liquid masses on Titan Dynamic of the liquid masses on Titan

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28.1047o&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 047.

Physics

Fluid Dynamics

Titan, Water, Fluid Dynamics, Satellite Surfaces, Sediments, Reynolds Number

Scientific paper

If liquid is available at the surface of Titan, the hydrodynamic behavior of its masses can be modeled, as in the present case, to understand the influence of the tidal forces on the ocean. The hydrodynamic characteristics are modeled using the Lunine (1993) composition for the bodies of standing liquid, and for the fluvial-like liquid the composition used ranges from that of the Lunine ocean to that of pure methane.

Affiliated with

Also associated with

No associations

Rating

Dynamic of the liquid masses on Titan does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Dynamic of the liquid masses on Titan, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamic of the liquid masses on Titan will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-873720