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3D Measurement Simulation and Relative Pointing Error Verification of the Telescope Mount Assembly Subsystem for the
Unai Mutilba1, Gorka Kortaberria2, Fernando Egaña3
1Department of Mechanical Engineering, IK4-Tekniker, 20600 Eibar, Spain. unai.mutilba@tekniker.es.
This study introduces a new laser tracker method for verifying large optical telescope pointing accuracy. The validated technique ensures precise alignment, even with environmental changes, offering a reliable metrology tool.
Area of Science:
- Optical Engineering
- Astronomy Instrumentation
- Metrology
Background:
- Large optical telescopes require precise engineering validation at the subsystem level.
- Relative pointing error verification is crucial for the absolute pointing performance of synoptic survey telescopes.
Purpose of the Study:
- To present a novel verification method for assessing the relative pointing error of telescope mount assemblies.
- To ensure the accuracy of large optical telescopes through advanced metrology.
Main Methods:
- Utilizing laser tracker technology and fixed floor fiducial points for relative pointing error assessment.
- Employing Monte Carlo-based simulations to validate the methodology under varying conditions.
- Investigating the potential for permanent laser tracker integration for active alignment and post-maintenance verification.
Main Results:
- The proposed methodology is robust and suitable for purpose, accommodating floor movement caused by temperature variations.
- Simulation results indicate measurement uncertainties better than 1 arcsecond with two on-board laser tracker systems and eight measurement targets.
- Demonstrated the feasibility of a reliable built-in metrology tool for large telescopes.
Conclusions:
- The novel laser tracker-based method effectively verifies relative pointing errors in large optical telescopes.
- Permanent integration of laser tracker technology offers potential for active alignment and enhanced operational accuracy.
- The developed technique provides a reliable metrology solution for large telescope structures, achieving sub-arcsecond accuracy.
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