Titlebook: Optics of Cosmic Dust; Gorden Videen,Miroslav Kocifaj Book 2002 Springer Science+Business Media Dordrecht 2002 Aerosol.Solar System.digita

細(xì)菌等

Monte Carlo Modeling of Cometary Atmospheres Including Polarizationres. The observed single scattering linear polarization phase curves of comets are found to be fairly well represented by a mixture of Mg-rich olivine particles and small carbonaceous particles. The input matrix of the code is thus given by the phase matrix for olivine as obtained in the laboratory

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Atmospheric Extinction Derived from Cometary Observationst observational nights. Average extinction coefficients are derived in the paper and some conclusions of common validity (in central European conditions) are formulated. The results of IHW/IAU extinction study have been compared with the results of . extinction coefficients gained mostly as a by-pro

采納

Experimental Modeling of Opposition Effect and Negative Polarization of Regolith-Like Surfacestion for dielectric surfaces depends on the surface tilt; even at small phase angles the polarization degree for tilted surfaces can be nonzero. The negative polarization depends strongly on micro- and macrostructured optical inhomogeneities of scattering surfaces. Double-minimum branches of negativ

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終端

coalition

搖擺

https://doi.org/10.1007/978-94-010-0628-6Aerosol; Solar System; digital elevation model; infrared spectroscopy; modeling; solar; spectroscopy; remot

Foolproof

978-1-4020-0820-7Springer Science+Business Media Dordrecht 2002

開頭

intellect

Infrared Spectroscopy of Cosmic Dusts in infrared spectroscopy of cosmic dust. The main topics are laboratory measurements on cosmic dust analogues and the spectroscopic characterization of primitive material in meteorites and interplanetary dust grains.