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.


    Zugriff

    Zugriff über TIB

    Verfügbarkeit in meiner Bibliothek prüfen


    Exportieren, teilen und zitieren



    Titel :

    Tides in Titan


    Beteiligte:

    Erscheinungsdatum :

    21.04.1997


    Medientyp :

    Preprint


    Format :

    Keine Angabe


    Sprache :

    Englisch




    Numerical Ocean Tides on Titan: Spherical Case

    Sears, W. D. / Lunar and Planetary Institute| National Aeronautics and Space Administration| Universities Space Research Association | British Library Conference Proceedings | 1994


    Numerical Ocean Tides on Titan: Spherical Case

    Sears, W. D. / Lunar and Planetary Institute / National Aeronautics and Space Administration et al. | British Library Conference Proceedings | 1994


    Tides

    Manolis, N. | Engineering Index Backfile | 1935


    Tides

    Online Contents | 2003


    Weather & Tides

    Online Contents | 2004