Simplified Telescope Test Bench Using Autocollimation Mirror
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Solution Overview
Problem
The high cost and complexity of measuring the Modulation Transfer Function (MTF) of large telescopes using conventional optical control benches, which require expensive equipment and are impractical for field use, necessitate a more economical and portable solution for monitoring optical performance.
Innovation Solution
An optical control bench utilizing a smaller autocollimation mirror to perform partial characterization of the telescope's optical quality, focusing a light source's image on a photo-detection unit, and employing a wavefront analyzer to estimate the Wave-Front Error (WFE), allowing for the detection of optical quality drift without the need for large, expensive optical components.
Engineering Contradictions & Design Principles
Engineering Contradiction Analysis
1Measurement precision
If a classic optical control bench with large optical components and vacuum chamber is used to measure MTF, then measurement precision is improved, but device complexity and cost increase significantly
Solution Approach 1:
The patent segments the measurement process into two parts: (1) measuring geometric characteristics of optical components using simple distance measurements and videogrammetry, and (2) calculating MTF from these geometric parameters through computational methods. This eliminates the need for a complete classic optical control bench while maintaining measurement capability.
Solution Approach 2:
The patent replaces the mechanical-optical measurement system (requiring large optical components, vacuum chambers, and stabilized environments) with a computational approach based on geometric measurements. MTF is calculated from geometric parameters rather than measured directly through complex optical benches.
2Measurement precision
If a classic optical control bench is used for MTF measurement, then measurement precision is improved, but cost increases to several million euros
Solution Approach 1:
The measurement system is segmented into low-cost geometric measurement components (distance sensors, cameras) and computational processing, replacing the expensive integrated optical bench. This allows MTF measurement capability to be achieved through software calculation rather than expensive hardware.
Solution Approach 2:
The patent uses inexpensive, readily available components (standard cameras, laser distance meters, videogrammetry systems) instead of expensive, specialized optical components. These conventional components can be replaced or upgraded more easily and at lower cost.
3Measurement precision
If a classic optical control bench is used, then measurement accuracy is improved, but portability and field use capability deteriorate
Solution Approach 1:
The measurement system is divided into portable geometric measurement devices that can be transported to the telescope location, rather than requiring the test object to be brought to a fixed, complex control bench. This enables field measurements at the actual telescope site.
Solution Approach 2:
The patent replaces the requirement for a fixed, environment-controlled measurement facility with a computational method that can operate in field conditions. Geometric measurements taken in-situ are processed computationally to determine MTF, eliminating the need for portable vacuum chambers and stabilized optical benches.
Applied Scientific Principles
This section explains which scientific principles are used to turn an abstract innovation direction into a practical engineering solution.
Function Achieved in This Case
Enables cost-effective, portable monitoring of optical performance, suitable for field use and endurance tests, by focusing on the evolution of optical quality rather than absolute performance, with the ratio of the mirror diameters between 30% and 80%, effectively capturing low-frequency WFE changes indicative of mirror movements during thermal or mechanical tests.
Implementation Method 1
an optical objective (110), a photo-detection unit (120) arranged at the focus of said optical objective
Implementation Method 2
the bench comprises a single plane mirror (130) and means for arranging this plane mirror so that the image of the light source given by the optical objective and reflected by said plane mirror is focused on the photo-detection unit
Data Source
Figure 1~2
Figure 3
AI summary
The bench has a plane mirror (130) having a first diameter smaller than a second diameter of an optical pupil of an optical object (110). A positioning unit arranges the plane mirror in a manner such that an image of a light source (121) provided by the optical object and reflected by the plane mirror is focused on a photo-detection housing (120). An analyzing unit analyzes the received image so as to determine optical quality of a spatial telescope (100), where the light source comprises an optical fiber whose one end is arranged adjacent to a photosensitive surface of the housing. An independent claim is also included for an optical telescope.