Which consequence results when iterative deconvolution functions are corrupted in astronomical adaptive optics?

💡 Explanation

Reduced Strehl ratio happens when wavefront correction is inaccurate; Distorted deconvolution corrupts phase conjugate formation via Zernike polynomials, because ADAPTIVE OPTICS relies on accurate point spread function modeling. Therefore resultant images sharpness decreases rather than chromatic issues developing or telescope instability.

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