1. Angelats i Coll, M., Forget, F., Lopez Valverde, M.A., Lewis, S.R., Read, P.L., 2004. The upper atmosphere of Mars up to 120 km: 2. Mars global surveyor accelerometer data analysis with the LMD general circulation model. J. Geophys. Res. Vol. 109, E01011. doi: 10.1029/2003JE002163.2004.
2. Methods of Celestial Mechanics;Brouwer,1961
3. Capderou, M., 2003. Satellites—Orbits and missions. Springer, Berlin, Paris (Chapter 10 : Satellite of Mars) (in French) 504 pp. [English version, Springer, in 2004].
4. Diurnal Kelvin wave in the atmosphere of Mars: toward and understanding of “Stationary” density structures observed by the MGS accelerometer;Forbes;Geophys. Res. Lett.,2000
5. Improved general circulation models of the Martian atmosphere from the surface to above 80km;Forget;J. Geophys. Res.,1999