Author:
Benešová Nina,Čížková Hana
Publisher
Springer Science and Business Media LLC
Subject
Geochemistry and Petrology,Geophysics
Reference40 articles.
1. Arkani-Hamed J., 1996. Analysis and interpretation of the surface topography and gravitational potential of Venus. J. Geophys. Res., 101, 4711–4724.
2. Armann M. and Tackley P.J., 2010. 3-D spherical modelling of the thermo-chemical evolution of Venus’ mantle and crust. Geophys. Res. Abs., 12, EGU2010–10507, 2010.
3. Barnett D.N., Nimmo F. and McKenzie D., 2002. Flexure of Venusian lithosphere measured from residual topography and gravity. J. Geophys. Res., 107, 5007, DOI: 10.1029/2000JE001398.
4. Běhounková M. and Choblet G., 2009. Onset of convection in a basally heated spherical shell, application to planets. Phys. Earth Planet. Inter., 176, 157–173.
5. Choblet G. and Sotin C., 2000. 3D thermal convection models of uids with variable viscosity: comparison between secular cooling and volumetric heating. Phys. Earth Planet. Inter., 119, 321–336.
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