论文信息 - Evidence for convection in planetary interiors from first-order topography - 字舞流文

Evidence for convection in planetary interiors from first-order topography

G. Schubert | R. Lingenfelter

[1] G. Hills. The formation of the continents by convection , 1947 .

[2] W. S. Cameron,et al. EVIDENCE FROM THE MOON'S SURFACE FEATURES FOR THE PRODUCTION OF LUNAR GRANITES , 1962 .

[3] G. Hills. The Granitic and Basaltic Areas of the Earth's Surface , 1934, Geological Magazine.

[4] Mariner 9 Celestial Mechanics Experiment: Gravity Field and Pole Direction of Mars , 1972, Science.

[5] A E Rogers,et al. Martian Craters and a Scarp as Seen by Radar , 1971, Science.

[6] J. Pratt. I. On the attraction of the Himalaya Mountains, and of the elevated regions beyond them, upon the plumb-line in India , 1855, Philosophical Transactions of the Royal Society of London.

[7] R. P. Ingalls,et al. Surface‐Height Variations on Venus and Mercury , 1970 .

[8] K. Jung. Figur der Erde , 1956 .

[9] W. Sjogren,et al. Mascons: Lunar Mass Concentrations , 1968, Science.

[10] M E Davies,et al. Mariner 9 Television Reconnaissance of Mars and Its Satellites: Preliminary Results , 1972, Science.

[11] On the Computation of the Effect of the Attraction of Mountain Masses as disturbing the Apparent Astronomical Latitude of Stations in Geodetic Surveys , 1855 .