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Performance prediction of the AXAF Technology Mirror Assembly using measured mirror surface errors
Applied Optics
|June 10, 2010
Summary
A new math model accurately predicts Technology Mirror Assembly (TMA) performance using scattering properties. This model accounts for various surface features and contamination, guiding future improvements.
Area of Science:
- Optical engineering
- Materials science
Background:
- Technology Mirror Assemblies (TMAs) are critical optical components.
- Accurate performance prediction is essential for TMA design and validation.
- Existing models may not cover the full range of surface features and environmental factors.
Purpose of the Study:
- To develop a comprehensive mathematical model for TMA performance prediction.
- To validate the model using new TMA data and X-ray test results.
- To identify factors influencing TMA performance, including surface characteristics and contamination.
Main Methods:
- Development of a scalar scattering model applicable to both large and small amplitude features.
- Incorporation of power spectral densities and autocovariance functions across spatial bandwidths.
- Analysis of TMA data from ~0.1-1000 mm(-1) spatial frequency range.
- Consideration of assembly, alignment, and particulate contamination effects.
Main Results:
- The developed model accurately relates measured TMA parameters to final performance.
- The model's predictions align with experimental X-ray test data.
- The study quantifies the impact of microroughness and broader spatial frequencies on performance.
Conclusions:
- The scalar scattering model provides a robust tool for TMA performance prediction.
- Understanding scattering properties and contamination is key to optimizing TMA performance.
- Repolishing is expected to significantly enhance TMA performance based on model insights.

