Cross-Sectional Profile of Baltis Vallis Channel on Venus: Reconstruction from Magellan SAR Brightness Data

Details Cross-Sectional Profile of Baltis Vallis Channel on Venus: Reconstruction from Magellan SAR Brightness Data Cross-Sectional Profile of Baltis Vallis Channel on Venus: Reconstruction from Magellan SAR Brightness Data

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1555o&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1555

Physics

1

Scientific paper

We develop a new method to reconstruct small scale topography from
brightness of SAR images, and reconstruct cross-sectional profiles of
Baltis Vallis. The results indicate that Baltis Vallis have been formed
by mechanical erosion in general.

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