Structural history of Maxwell Montes, Venus: Implications for Venusian mountain belt formation
@article{Keep1994StructuralHO, title={Structural history of Maxwell Montes, Venus: Implications for Venusian mountain belt formation}, author={M. Keep and V. Hansen}, journal={Journal of Geophysical Research}, year={1994}, volume={99}, pages={26015-26028} }
Models for Venusian mountain belt formation are important for understanding planetary geodynamic mechanisms. A range of data sets at various scales must be considered in geodynamic modelling. Long wavelength data, such as gravity and geoid to topography ratios, need constraints from smaller-scale observations of the surface. Pre-Magellan images of the Venusian surface were not of high enough resolution to observe details of surface deformation. High-resolution Magellan images of Maxwell Montes… CONTINUE READING
19 Citations
Structural and Kinematic Analysis of Eastern Ovda Regio, Venus: Implications for Crustal Plateau Formation
- Geology
- 1999
- 64
- PDF
Surface processes in the Venus highlands: Results from analysis of Magellan and Arecibo data
- Geology
- 1999
- 26
Morphology and deformational history of Tellus Regio, Venus: Evidence for assembly and collision
- Geology
- 2018
- 12
- Highly Influenced
- PDF
References
SHOWING 1-10 OF 48 REFERENCES