Loss Tangent Map of the Martian Surface: A Frequency Dependent Model for the Near Equatorial Regions | INSTITUT DE PHYSIQUE DU GLOBE DE PARIS

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  Loss Tangent Map of the Martian Surface: A Frequency Dependent Model for the Near Equatorial Regions

Type de publication:

Conference Proceedings

Auteurs:

Heggy, E.

Source:

36th Annual Lunar and Planetary Science Conference, Volume 36, p.2109 (2005)

URL:

http://adsabs.harvard.edu/abs/2005LPI....36.2109H

Mots-clés:

Etudes spatiales et planétaires, UMR 7154

Résumé:

Using laboratory dielectric characterization of basaltic Mars-like soils and soil density distribution extracted from TES data, we suggest a frequency dependent loss tangent and complex dielectric map of the Martian surface in the frequency range from 1 MHz to 3 GHz.