we consider the problem of continuous dynamic berth allocation to containerships in a tidal seaport. in some container ports, low water depth in coastal area causes many restrictions on providing vessel's services. therefore, berth allocation planning for relatively large vessels with high draft is subject to tidal conditions when the vessels are in the access channel as from anchorage are...

We compare several recent Martian interior models and evaluate how these are impacted by the tidal constraints provided Love number k2 secular acceleration in longitude s of its main moon, Phobos. The expression latter is developed up to harmonic degree 5 match accuracy current observations. a structure measurements parameters derive estimations possible core radius, temperature profile, attenu...

Magnetic induction measurements and astrometry provide constraints on the internal structure of Io, a volcanically active moon of Jupiter. We model the tidal response of a partially molten Io using an Andrade rheology which is supported by silicate deformation experiments. This model uses material properties similar to the Earth’s mantle and includes feedbacks between partial melting, tidal hea...

We use the tidal deformations of Moon induced by Earth and Sun as a tool for studying inner structure our satellite. Based on measurements degree-two Love numbers k2 h2 dissipation coefficients from GRAIL mission, Lunar Laser Ranging Altimetry board LRO spacecraft, we perform Monte Carlo samplings 120,000 possible combinations thicknesses viscosities two classes lunar models. The first one incl...

Abstract Tidal dissipation in binary systems is the primary source for synchronization and circularization of objects system. The efficiency tidal energy inside stars or planets results significant changes observed properties system often studied empirically using a parameter, commonly known as modified quality factor (${Q_{\star }^{\prime }}$). Though assumed constant, general that parameter w...

In this paper, the effect on tidal response of low-viscosity zone in deep interior Moon is investigated based hypothetical temperature profiles. The parameters are computed numerically to demonstrate their dependence and frequency. One calculated quality factor, which energy dissipation inversely proportional. other Love numbers, normalized magnitudes displacement potential perturbation deforma...