Lava, Debris, and Pyroclastic Flow Deposits: Analysis and Identification Using Curvature Spectra

Details Lava, Debris, and Pyroclastic Flow Deposits: Analysis and Identification Using Curvature Spectra Lava, Debris, and Pyroclastic Flow Deposits: Analysis and Identification Using Curvature Spectra

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996lpi....27..877m&link_type=abstract

Lunar and Planetary Science, volume 27, page 877

Physics

Curvature Spectra, Flows: Debris, Flows: Lava, Flows: Pyroclastic, Lahars

Scientific paper

Evidence of rhyolite, andesite, basalt, debris or pyroclastic flow deposits on planets such as Mars and Venus can give important clues to the nature of volcanic processes, crustal evolution and volatile abundance and history. The positive identification of lahars or debris flows on Mars is evidence for the presence of water. Despite this importance, it is often difficult to recognize flow deposit type with confidence from remote observation.

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