The morphology of the ridge belts on Venus

Details The morphology of the ridge belts on Venus The morphology of the ridge belts on Venus

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990avest..24...83k&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 24, Apr.-June 1990, p. 83-95. In Russian.

Astronomy and Astrophysics

Astronomy

Bridges (Landforms), Radar Imagery, Venera Satellites, Venus Surface, Morphology, Northern Hemisphere, Radar Photography, Satellite-Borne Photography, Spatial Distribution

Scientific paper

The length and spacing of linear features were measured for ridge and groove belts, for the outer mountain zones of the Lakshmi planum, and for the outer ridge zones of coronal structures. The distributions of these parameters show small but significant differences in most of the cases. The ridges are assumed to result from deformations. Deformed-layer thickness were estimated for various types of linear subdivisions.

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