New ASPIICS observations confirm the qualitative properties of a diffraction model for coronagraph straylight and achieve 30-50% quantitative agreement after fine-tuning, with diffracted light two orders of magnitude below the coronal signal.
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Diffraction in the ASPIICS coronagraph: observations and modeling
New ASPIICS observations confirm the qualitative properties of a diffraction model for coronagraph straylight and achieve 30-50% quantitative agreement after fine-tuning, with diffracted light two orders of magnitude below the coronal signal.