A surface layer adaptive optical system error analysis method

By employing analytical methods based on error structure functions and mode covariance matrices, the problems of high computational resource consumption and difficulty in tracing errors in surface adaptive optics systems are solved. This enables rapid and efficient error analysis and image quality prediction, supporting the adaptive optics design of modern large astronomical telescopes.

CN122113458BActive Publication Date: 2026-07-03CHENGDU TECH UNIV

Patent Information

Authority / Receiving Office
CN · China
Patent Type
Patents(China)
Current Assignee / Owner
CHENGDU TECH UNIV
Filing Date
2026-04-28
Publication Date
2026-07-03

AI Technical Summary

Technical Problem

The simulation computation of existing surface adaptive optics systems is resource-intensive and the errors are difficult to trace independently. Traditional methods cannot provide accurate guidance for error allocation.

Method used

A systematic error analytical method based on error structure function and mode covariance matrix is ​​adopted. By calculating the residual wavefront structure function of uncompensated atmospheric turbulence error and instrument error, and linearly superimposing them, the overall performance structure function is obtained, and then the long exposure optical transfer function and point spread function are calculated.

Benefits of technology

It greatly improves the generation speed of long exposure point spread function for large-aperture, wide-field-of-view systems, reducing it from several hours to seconds, and achieves "white-box" decoupling of various physical errors, providing accurate image quality prediction and error allocation scheme guidance.

✦ Generated by Eureka AI based on patent content.

Smart Images

  • Figure CN122113458B_ABST
    Figure CN122113458B_ABST
Patent Text Reader

Abstract

This invention discloses an error analysis method for a surface-level adaptive optics system, relating to the field of adaptive optics technology for astronomical telescopes. The key technical points are: calculating the first structure function of the residual wavefront generated by uncompensated atmospheric turbulence errors; calculating the second structure function of the residual wavefront generated by instrument errors in the surface-level adaptive optics system; linearly superimposing the first and second structure functions to obtain the overall performance structure function of the surface-level adaptive optics system; calculating the long-exposure optical transfer function based on the overall performance structure function, and performing a Fourier transform on the long-exposure optical transfer function to obtain the point spread function of the surface-level adaptive optics system; wherein, the point spread function is used to analyze the errors and performance of the surface-level adaptive optics system.
Need to check novelty before this filing date? Find Prior Art