Tides raised in Titan by Saturn give rise to a static and a periodic deformation; both will be measured with Doppler tracking during the CASSINI Tour of the Saturnian System. The latter deformation is due to the significant eccentricity of Titan's orbit and has a frequency equal to the orbital angular velocity of Titan.
Tides in Titan
1997-04-21
Preprint
No indication
English
Numerical Ocean Tides on Titan: Spherical Case
British Library Conference Proceedings | 1994
|Numerical Ocean Tides on Titan: Spherical Case
British Library Conference Proceedings | 1994
|Engineering Index Backfile | 1935
|Online Contents | 2003
Online Contents | 2004