Using Spatial Density to Characterize Volcanic Fields on Mars

Details Using Spatial Density to Characterize Volcanic Fields on Mars Using Spatial Density to Characterize Volcanic Fields on Mars

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2314r&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2314

Physics

Scientific paper

Kernel density estimation is presented as a new, non-parametric method
for quantifying the spatial arrangement of volcanic fields. It is
applied to two vent fields in Tharsis Province, Mars, to produce
insightful spatial density functions.

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