Morphometric properties of Martian volcanoes

January 1, 2004

Mars Orbiter Laser Altimeter (MOLA) data have been used to construct Digital Elevation Models (DEM) of the Martian volcanoes in order to determine height, flank slope, caldera depth, and volumes. Summit elevations range from 21.1 km to −0.5 km, and relief varies from 1.0 km to almost 22 km. Average flank slopes are in the range of

Publication Year	2004
Title	Morphometric properties of Martian volcanoes
DOI	10.1029/2002JE002031
Authors	J. B. Plescia
Publication Type	Article
Publication Subtype	Journal Article
Series Title	Journal of Geophysical Research E: Planets
Index ID	70026910
Record Source	USGS Publications Warehouse
USGS Organization	Astrogeology Science Center

Morphometric properties of Martian volcanoes

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