The STOP analysis demonstrates that temperature-induced optical perturbations remain well below allowable limits for all observing conditions, with in-orbit temperature variations under 300 mK producing detectable but manageable effects on PSF stability.
In our analysis, we removed VIS frames that were affected by strong solar flares using a merit function derived frome 1,e 2, andR 2 covariances
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Euclid Structural-Thermal-Optical Performance
The STOP analysis demonstrates that temperature-induced optical perturbations remain well below allowable limits for all observing conditions, with in-orbit temperature variations under 300 mK producing detectable but manageable effects on PSF stability.