Lunar dielectric constants from aperture synthesis polarimetry at 6 CM

Details Lunar dielectric constants from aperture synthesis polarimetry at 6 CM Lunar dielectric constants from aperture synthesis polarimetry at 6 CM

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..871m&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 871.

Computer Science

Lunar Environment, Dielectrics, Polarimetry, Radio Emission, Very Large Array (Vla), Radar Maps

Scientific paper

The Very Large Array's most compact configuration was used to measure the moon's polarized thermal emission at 6 cm. Deconvolved images of the Stokes parameters were used to compute the degree of linear polarization of the lunar thermal emission, which in turn provides estimates of the dielectric constant; the inversion method used relies on differences between the transmission coefficients parallel and perpendicular to the plane of emission at the regolith-vacuum interface.

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