Polarimetric remote sensing of Solar System objects

@article{Mishchenko2010PolarimetricRS,
  title={Polarimetric remote sensing of Solar System objects},
  author={Michael I. Mishchenko and Vera K. Rosenbush and Nikolai Kiselev and Dmitrij F. Lupishko and Victor P. Tishkovets and Vadim G. Kaydash and Irina Belskaya and Yu. S. Efimov and Nikolay M. Shakhovskoy},
  journal={arXiv: Earth and Planetary Astrophysics},
  year={2010}
}
This book outlines the basic physical principles and practical methods of polarimetric remote sensing of Solar System objects and summarizes numerous advanced applications of polarimetry in geophysics and planetary astrophysics. In the first chapter we present a complete and rigorous theory of electromagnetic scattering by disperse media directly based on the Maxwell equations and describe advanced physically based modeling tools. This is followed, in Chapter 2, by a theoretical analysis of… 
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References

SHOWING 1-10 OF 476 REFERENCES
Estimate of the aerosol properties over the ocean with POLDER
The wide field of view imaging spectroradiometer Polarization and Directionality of the Earth's Reflectance (POLDER) developed by Centre National d'Etudes Spatiales and operated aboard the Japanese
Passive Microwave Remote Sensing of the Earth
  • W. Wilson
  • Environmental Science, Mathematics
  • 2004
TLDR
The description of a number of Russian aircraft and space microwave experiments in this field are described, 1980–1990, but provide examples of the pioneering techniques and results achieved by Russian scientists.
Photometric and Polarimetric Opposition Phenomena Exhibited by Solar System Bodies
Ground-based and spacecraft observations of atmosphere less solar system bodies (planets, satellites, planetary rings, and asteroids) and cometary and interplanetary dust particles have provided a
Asteroid Photometric and Polarimetric Phase Effects
We review progress in the photometric and polarimetric observations of asteroids, including theoretical and experimental advances in interpreting scattering and absorption of light by asteroid
Accurate monitoring of terrestrial aerosols and total solar irradiance: Introducing the Glory mission
The NASA Glory mission is intended to facilitate and improve upon long-term monitoring of two key forcings influencing global climate. One of the mission's principal objectives is to determine the
Remote sensing of aerosols with the earth-observing scanning polarimeter
  • L. Travis
  • Environmental Science, Physics
    Optics & Photonics
  • 1992
Tropospheric aerosols have potential climate forcing roles through both the direct effect on solar radiation scattered and absorbed and the indirect effect as condensation nuclei for cloud particles.
Aerosol polarimetry sensor for the Glory Mission
  • R. Peralta, C. Nardell, R. Hooker
  • Environmental Science
    International Symposium on Multispectral Image Processing and Pattern Recognition
  • 2007
This paper describes the Glory Mission Aerosol Polarimetry Sensor (APS) being built by Raytheon under contract to NASA's Goddard Space Flight Center. Scheduled for launch in late 2008, the instrument
Optical polarimetry of asteroids and laboratory samples
Interpretations of astronomical polarization data for more than 100 minor planets are summarized with reference to laboratory data for lunar, meteoritic, and terrestrial samples. All observed
Satellite retrieval of aerosol properties over the ocean using polarization as well as intensity of reflected sunlight
Most current and proposed satellite remote sensing of tropospheric aerosols relies upon radiance measurements that are interpreted using algorithms that determine best fits to precalculated scattered
...
...