Atmos. Chem. Phys. Atmospheric Chemistry and Physics, vol. 10 (2010) pp. 383-396
Although solar radiation initially is unpolarized when entering the Earth's atmosphere, it is polarized by scat-tering processes with molecules, water droplets, ice crys-tals, and aerosols. Hence, measurements of the polariza-tion state of radiation can be used to improve remote sens-ing of aerosols and clouds. The analysis of polarized ra-diance measurements requires an accurate radiative trans-fer model. To this end, a new efficient and flexible three-dimensional Monte Carlo code to compute polarized radi-ances has been developed and implemented into MYSTIC (Monte Carlo code for the phYSically correct Tracing of pho-tons In Cloudy atmospheres). The code has been extensively validated against published benchmark results. The polarized downwelling radiation field is calculated for various aerosol types showing the high sensitivity of polarized ultraviolet radiances to the particle microphysics. Model simulations are compared to ground based measurements and found to be qualitatively in good agreement. Quantitative differences can be attributed to the assumed aerosol models based on the OPAC aerosol database, which does not include exactly the types of aerosols that have been observed. This comparison to the measurements shows that there is a high potential to retrieve information about the aerosol type from polarized radiance measurements.
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