A principal component based accurate fast vector radiative transfer model with very high resolution in the UV (200 nm) to NIR (2500 nm) has been developed. This model greatly reduces the number of necessary radiative transfer calculations, and no time-consume convolution process is needed to get the final radiance spectrum. The error in the obtained Stokes component is usually smaller than 0.1% and is much smaller than the uncertainty in the measured solar irradiance.
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