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• W2051191505 abstract "Radio Doppler shifts between a lander on Mars' surface and an orbiter are modeled through a linearized analytical formulation. This simplified formulation allows us to understand the signature and interplay of the different geophysical parameters (nutations, polar motion, and rotation rate variations) on the lander‐orbiter observable. The frequency band of the investigated periodic phenomena goes from some months to about one Martian year in their respective frames. Long‐term effects like precession are taken into account but are not investigated. The satellite orbit is modeled as a precessing orbit because of the oblateness of Mars. We show that we are able to see the signature of a possible liquid core after less than 50 weeks of observation for a given precision of 0.1 mm/s for the Doppler tracking. We are also able to monitor the rotation rate variation and polar motion at a level of 5 mas over the same period. This study was done in the frame of the preparation of the Netlander Ionosphere and Geodesy Experiment (NEIGE)." @default.
• W2051191505 created "2016-06-24" @default.
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• W2051191505 date "2003-07-01" @default.
• W2051191505 modified "2023-10-15" @default.
• W2051191505 title "Analytical modeling of the Doppler tracking between a lander and a Mars orbiter in terms of rotational dynamics" @default.
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• W2051191505 doi "https://doi.org/10.1029/2003je002045" @default.
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