On the uniformity of 'volcanic flows' distribution in the northern hemisphere of Venus

Details On the uniformity of 'volcanic flows' distribution in the northern hemisphere of Venus On the uniformity of 'volcanic flows' distribution in the northern hemisphere of Venus

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990avest..24..195l&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 24, July-Sept. 1990, p. 195-202. In Russian.

Astronomy and Astrophysics

Astronomy

Radar Photography, Surface Roughness, Venus Surface, Volcanology, Northern Hemisphere, Spatial Distribution, Venera Satellites

Scientific paper

The distribution of flowlike details ('volcanic flows') on the Venus surface was investigated on the basis of Venera-15, 16 radar data. The areal distribution of these details appears to be nonuniform and to be clustered with a characteristic cluster size of about 1000 km. The alternative hypothesis is that the flowlike details are concentrated in the northern hemisphere in the 210-300-deg longitude region.

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