Citation: P. Vacher et al., COMPUTATION OF SEISMIC PROFILES FROM MINERAL PHYSICS - THE IMPORTANCEOF THE NON-OLIVINE COMPONENTS FOR EXPLAINING THE 660 KM DEPTH DISCONTINUITY, Physics of the earth and planetary interiors, 106(3-4), 1998, pp. 275-298
Citation: P. Vacher et al., COMPARISON BETWEEN TOMOGRAPHIC STRUCTURES AND MODELS OF CONVECTION INTHE UPPER-MANTLE, Geophysical journal international, 124(1), 1996, pp. 45-56
Citation: A. Mocquet et al., THEORETICAL SEISMIC MODELS OF MARS - THE IMPORTANCE OF THE IRON CONTENT OF THE MANTLE, Planetary and space science, 44(11), 1996, pp. 1251-1268
Citation: O. Grasset et al., INVESTIGATION OF THE NH3-H2O PHASE-DIAGRAM IN THE RANGE 100MPA-1.5GPAUSING IN-SITU RAMAN-SPECTROSCOPY - APPLICATION TO TITANS DYNAMICS, Comptes rendus de l'Academie des sciences. Serie II. Mecanique, physique, chimie, astronomie, 320(4), 1995, pp. 249-256
Citation: L. Dupeyrat et C. Sotin, THE EFFECT OF THE TRANSFORMATION OF BASALT TO ECLOGITE ON THE INTERNAL DYNAMICS OF VENUS, Planetary and space science, 43(7), 1995, pp. 909-921
Authors:
BUSSE FH
CHRISTENSEN U
CLEVER R
CSEREPES L
GABLE C
GIANNANDREA E
GUILLOU L
HOUSEMAN G
NATAF HC
OGAWA M
PARMENTIER M
SOTIN C
TRAVIS B
Citation: Fh. Busse et al., 3D CONVECTION AT INFINITE PRANDTL NUMBER IN CARTESIAN GEOMETRY - A BENCHMARK COMPARISON, Geophysical and astrophysical fluid dynamics, 75(1), 1994, pp. 39-59