Constraining the Origin of Pitted Cones in Chryse and Acidalia Planitiae, Mars, Based on Their Statistical Distributions and Marginal Relationships

Details Constraining the Origin of Pitted Cones in Chryse and Acidalia Planitiae, Mars, Based on Their Statistical Distributions and Marginal Relationships Constraining the Origin of Pitted Cones in Chryse and Acidalia Planitiae, Mars, Based on Their Statistical Distributions and Marginal Relationships

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2905s&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2905

Physics

Scientific paper

Despite the fact that pitted cones are common landforms in the martian
northern plains, there is still ambiguity regarding their origin. This
study addresses these ambiguities by assessing their spatial variations
and marginal relationships.

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