by Israel Program for Scientific Translations; [available from the U.S. Dept. of Commerce, Clearinghouse for Federal Scientific and Technical Information, Springfield, Va.] in Jerusalem .
Written in English
|Statement||Edited by V.G. Fesenkov. Translated from Russian [and edited by IPST staff].|
|Contributions||Fesenkov, V. G. 1889- ed., United States. Dept. of Commerce., National Science Foundation (U.S.)|
|LC Classifications||QC975 .V7613|
|The Physical Object|
|Pagination||iv, 227 p.|
|Number of Pages||227|
|LC Control Number||he 65000059|
Scattering and polarization of light in the atmosphere (Rasseyanie i polyarizatsiya sveta v zemnoi atmosfere); proceedings. Author: V G Fesenkov ; United States. Polarization of light in the atmosphere and ocean. Abstract. In this chapter, we will present a brief history of polarization, a short description of the Stokes parameter–Mueller matrix representation of polarized light, and techniques for using polarization for remote sensing of both the atmosphere and the by: 4. Polarization and Intensity of Light in the Atmosphere. azimuth Babinet beam Brewster cause clear cloud color complete components computations Coulson crystals curves decrease degree of polarization dependence determined developed diagram direction discussed distance distribution drop Polarization and Intensity of Light in the Atmosphere. The work is aimed at the review of hot topics in modern light scattering and radiative transfer. A special attention will be given to the description of the methods of integro-differential radiative t Search within book. Front Matter Front Matter. Pages PDF. Polarization of light in the atmosphere and ocean. George W. Kattawar.
Polarization of light in the atmosphere and ocean. there is a significant place for methods of light-scattering optics that are fast and noninvasive. This is the first study to investigate. Simulation of atmospheric scattering and polarization of sunlight using slide projector and aquarium containing milky water. What it shows: Unpolarized light passing through a fluid is scattered; the scattered light being partially or completely plane polarized. For scattering by particles of comparable size to the wavelength of the light, this process is called Rayleigh scattering. Light scattering off atoms and molecules in the atmosphere is unpolarized if the light keeps traveling in the same direction, is linearly polarized if at scatters in a direction perpendicular to the way it was traveling, and somewhere between linearly polarized and unpolarized if it scatters of at another angle. Request PDF | On Jan 1, , G.W. Kattawar and others published Polarization of light in the atmosphere and ocean | Find, read and cite all the research you need on ResearchGate.
Rotational Raman scattering of polarized light in the Earth atmosphere: a vector radiative transfer model using the radiative transfer perturbation theory approach The approach contains an exact solution for singly scattering light. To ease the correction. so the light appears partially polarized. Thus, the process of scattering explains the polarization of skylight. Scattering of light by the Earth's atmosphere depends on A. For particles much smaller than the wavelength of light (such as molecules of air), the parti cles will be less of an obstruction to long wavelengths than to short ones. TheFile Size: 5MB. With our polarized RT model and the Mie code combined, the Stokes parameters as well as the degree of polarization for each scattering order are simulated and presented; meanwhile, the polarization (depolarization) properties of multiply scattering are preliminary analyzed and compared with different air quality (clear and pollution).Cited by: 2. vi Scattering, Absorption, and Emission of Light by Small Particles Phase matrix 49 Extinction matrix 54 Extinction, scattering, and absorption cross sections 56 Radiation pressure and radiation torque 60 Thermal emission 63 Translations of the origin 66 Further reading