ISPRS 2003 Topographic Profile Diagrams of Mars: Architecture of the Density of Craters Curver Low-Pass Filter

Recently, mathematical approach was proposed providing a way to compute how deep Martian ocean was during each period of the planet history, including the probability that ocean existed once. Important step toward the formal proof of Martian ocean recession, timing and probability is representation of Martian topography and related values, in the form of topography profile diagrams. For this purpose, the architecture of the crater density curve low-pass filter is important.

Mimetype

application/pdf

Filename

Nezic_1_isprs_mar03.pdf

Publisher

ISPRS

Author

gsc

Originator

Z. Nežić, G. Salamunićcar

Group

Astrogeology

Added to Astropedia

14 May 2012

Modified

9 July 2013

General

Geospatial Data Presentation Form

Document

Keywords

System

Mars

Target

Mars

Theme

Craters, Topography

Geospatial Information

Quad Name