Evolution of the Dichotomy Boundary Zone, Arabia Terra, Mars

Details Evolution of the Dichotomy Boundary Zone, Arabia Terra, Mars Evolution of the Dichotomy Boundary Zone, Arabia Terra, Mars

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1148m&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1148

Physics

Scientific paper

Mapping of 4 1:500K quadrangles (30-45N332) transecting the martian
dichotomy boundary indicates that fretted channels and debris flows
formed over finite intervals but at different times; thus the flow lobes
do not necessarily imply that the channels formed by mass wasting.

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