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This article will give an overview of all effects that determine the spectral features amplitude (SFA). The origin of
spectral features is explained and methods are indicated that can be used to minimize the SFA. Spectral features are
observed in the ratio between two spectra of sun calibration measurements. Mechanisms helping to reduce spectral
features are spectral averaging, angular averaging, and temporal averaging. It will be shown what optical design choices
can be made in order to benefit from these SFA reducing mechanisms. In the final chapter some insight in the modeling
is given where four types of diffusers are compared.
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Hedser van Brug, "Spectral features: an overview," Proc. SPIE 8148, Solar Physics and Space Weather Instrumentation IV, 81480R (6 October 2011); https://doi.org/10.1117/12.890314