Tessera terrain on Venus: A survey of the global distribution, characteristics, and relation to surrounding units from Magellan data

Journal of Geophysical Research: Planets

Volumn 101, Issue E6, 1996, Pages 14861-14908

  Ivanov, Mikhail A ^a,b   Head, James W ^b  

^a VERNADSKY INSTITUTE OF GEOCHEMISTRY AND ANALYTICAL CHEMISTRY   (Russian Federation)

^b BROWN UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

MAGELLAN DATA; PLANETARY TOPOGRAPHY; TESSERA;

VENUS;

EID: 0030453880     PISSN: 01480227     EISSN: None     Source Type: Journal    
DOI: 10.1029/96JE01245     Document Type: Article

References (4)

1. Arkani-Hamed, J., On the tectonics of Venus, Phys. Earth Planet. Inter., 76, 75-96, 1993.
2. Arkani-Hamed, J., and M. N. Toksoz, Thermal evolution of Venus, Phys. Earth Planet. Inter., 34, 232-250, 1984.
3. Aricani-Hamed, J., G. G. Schaber, and R. G. Strom, Constraints on the thermal evolution of Venus inferred from Magellan data, J. Geophys. Res. 98 (E3), 5309-5315, 1993.
4. Barsukov, V. L., et al., The geology and geomorphology of the Venus surface as revealed by the radar images obtained by Veneras 15 and 16, Proc. Lunar Planet. Sci Conf. 16th, Part 2, J. Geophys. Res., 91, suppl., D378-D398, 1986.