Subresolution clinometry with Magellan radar images - Height of lava flow edges on Venus

Details Subresolution clinometry with Magellan radar images - Height of lava flow edges on Venus Subresolution clinometry with Magellan radar images - Height of lava flow edges on Venus

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..759k&link_type=abstract

Conference Paper,

Physics

Radar Imagery, Satellite Imagery, Magellan Spacecraft (Nasa), Lava, Venus Surface, Radio Altimeters, Backscattering

Scientific paper

A new method for estimations of heights and slopes of small-scale
topographical features on Venus with Magellan radar images is proposed.
The method is used for estimation of height of a step associated with
some edges of digitate lava flows. The upper limit of such height is
estimated for sheet flows.

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