We use Mars Orbiter Laser Altimeter (MOLA) data to measure small volcanoes in the Tempe Terra and Ceraunius Fossae regions of Mars. We find that previous geometry estimates based on imagery alone are inaccurate, but MOLA data support image-based interpretations of eruptive style. Additional information is contained in the original extended abstract.
T. C. Duxbury, David E. Smith, M. T. Zuber, H. V. Frey, James Jim Brian Garvin, J. W. Head, D. O. Muhleman, G. H. Pettengill, R. J. Phillips, Sean C. Solomon
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