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Optical properties of aerosols in Titan's atmosphere
Authors:YuV Skorov  HU Keller
Institution:a Max-Planck Institute for Solar System Research, 37191 Katlenburg-Lindau, Germany
b Space Research Institute, Russian Academy of Sciences, 117997, 84/32 Profsoyuznaya Street, Moscow, Russian Federation
c Moscow Institute of Physics and Technology, 141700, Institutsky Dr 9, Dolgoprudny, Moscow Region, Russian Federation
Abstract:In the frame of fractal modeling of tholin aggregates we made a systematic analysis of their optical properties. Ballistic particle-cluster aggregation (BPCA) and diffusion-limited aggregation (DLA) of spherical primary particles (monomers) identical in material composition were considered. Aggregates composed of identical particles (monodisperse cluster), as well as of size-distributed particles (polydisperse cluster), were simulated. To calculate the light-scattering models, the code based on the superposition T-matrix method is used. Orientationally averaged properties of light scattering by model particles were extracted, and the normalized phase function and the degree of linear polarization were calculated as functions of scattering angle. We concluded that: (a) aggregation mechanism as well as specific internal structure of the clusters play only a minor role, and for the future it is not necessary to investigate aggregates of different types; (b) the intensity is very sensitive both to the size parameter of forming particles x and to the size parameter of the aggregates X; (c) characterization of the aggregates by the number of monomers is insufficient to retrieve physical properties of aggregates from optical measurement; and (d) it is very desirable to include into the analysis polarization data calculated for the different clusters.
Keywords:Titan  Huygens  Photometry  Polarimetry
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