Image-based wavefront correction for space telescopes
Telescope image: ray, wavefront and diffraction
Active compensation for optimal RMS wavefront error in perturbed off-axis optical telescopes using nodal aberration theory
Active Control of Large Telescopes: Adaptive Optics | SpringerLink
A Shack-Hartmann Wavefront Sensor measures the wavefront by computing... | Download Scientific Diagram
Photonics | Free Full-Text | Wide-Field Telescope Alignment Using the Model-Based Method Combined with the Stochastic Parallel Gradient Descent Algorithm | HTML