Microwave thermal emission mapping of the Stealth region on Mars

Details Microwave thermal emission mapping of the Stealth region on Mars Microwave thermal emission mapping of the Stealth region on Mars

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..629i&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 629.

Physics

Microwave Emission, Thermal Emission, Mapping, Mars Surface, Very Large Array (Vla), Image Processing, Interferometers

Scientific paper

The Very Large Array has been used to interferometrically observe Mars in order to study the Stealth feature, west of the Tharsis ridge, from which no measurable echo can be detected. Stealth is interpreted as a medium free of rocks and clamps of cm size and larger that would act as subsurface scatterers; it is suggested that Stealth had its origin in the activity of Tharsis volcanoes during the Late Amazonian period.

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