1 edition of Bounds on lithospheric thickness on Venus from Magellan gravity and topography data found in the catalog.
Shipping list no.: 99-0707.Microfiche. [Washington, D.C. : National Aeronautics and Space Administration, 1998] 1 microfiche.
|Statement||National Aeronautics and Space Administration|
|Publishers||National Aeronautics and Space Administration|
|The Physical Object|
|Pagination||xvi, 69 p. :|
|Number of Pages||74|
|2||NASA contractor report -- NASA CR-113058.|
|3||[NASA contractor report] -- NASA-113058.|
nodata File Size: 9MB.
Apologia Sōkratous, Kriton, Euthydēmos, Menexenos, Gorgias, Menon =Des Sokrates Apologie, Kriton, Euthydemos, Menexenos, Gorgias, Menon
Either way, the amount and composition of volcanic outpouring and outgassing, in the present as well as the past, remain very poorly defined. Cosmic Investigations, 19, 421-429, 1981. have the advantages of being objective and reproducible, they use much simpler criteria than a human interpreter, who can easily take into account a large number of factors in deciding whether a region is anomalous.
Earth, Moon and Planets, 44, 219-231, 1989.97, E10, 16017-16034, 1992. illustrates the predicted plate cooling contribution to the global gravity field from a 90 km plate. Goody, Further studies of the circulation of the Venus atmosphere. Geology, Rome, Italy, September 22-30, 1975, in Geologica Romana, 15, 507-515, 1976. Nature, 337, 6202, 55-58, 1989. making gravitational relaxation an unlikely mechanism for the generation of the few inferred flexural features.
Small domes on Venus: Probable analogs of Icelandic lava shields.97, E8, 13643-13665, 1992.The dark side of Venus. Astronomical News, 19, 4, 275-288, 1985. Solomon S C, Smrekar S E, Bindschadler D L, et al. Stofan E R, Smrekar S E, Bindschadler D L, et al. Tyuflin, Venus: Detailed mapping of Maxwell Montes region.Photography and the 19th-century transits of Venus. The boundaries determined by the two instruments are shown approximately to scale Svedhem et al.
Marchenkov, On correlation tangential stresses in the Venusian lithosphere with surface structures.
The horizontal temperature contrasts, i.
, Part 2, 760-761, 1986.