Polarimetric measurements of simulated lunar surfaces.
Polarimetric properties of simulated lunar surface, showing polarization effect on particle size
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Polarimetric properties of simulated lunar surface, showing polarization effect on particle size
Optical polarimetric observations of quasi-stellar objects
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The potentially measureable effects of Faraday rotation on linearly polarized interferometric or polarimetric SAR measurements from space are addressed.
In this paper, lessons learned through the calibration of SIR-C data will be reviewed in the context of upcoming spaceborne, polarimetric SAR missions planned for launch later in this decade.
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The design and testing results for the Radio Frequency (RF) portion of a breadboard polarimetric scatterometer operating at 13.402 GHz are presented.
Studies of polarized radiation from molecular clouds and the environments of protostars are providing information about the orientations and strengths of magnetic fields and the sizes andcompositions of dust grains in these environments.
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We show that the geometry of the polarization can be understood in terms of multiple scattering within an optically thick disk, yielding the observed polarization parallel to the long axis of the observed edge-on disk.
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The sensitivities of wind direction signals in passive microwave brightness temperatures of sea surfaces to wind speed, incidence angle, polarization and frequency are presented in this paper.
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The US Space Shuttle is a useful platform from which to evaluate remote sensing instrumentation.
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It is necessary to calibrate SAR data in order to use the data for science applications. When both polarimetric and interferometric data are collected simultaneously, these SAR data can be used for cross-calibration and verification.