An adaptive optical system performance analysis tool for astronomical observation design
AdaptiveLens
What is it about?
An adaptive optical system performance analysis tool for astronomical observation design. Through accurate physical model calculation, astronomers and telescope operators can be helped to optimize observation parameters and evaluate the correction effect of adaptive optical system. Core functions: Real-time performance analysis: according to the atmospheric conditions, observation wavelength, control system parameters and other factors, the performance index of adaptive optical system is calculated in real time. Multi-parameter adjustment: support the adjustment of key parameters such as atmospheric visibility, observation wavelength, loop frequency, brightness of guiding star and telescope aperture. Professional calculation model: Based on classical optical theories such as Fried parameter and Maréchal approximation, some important indexes such as residual wavefront error and Strehl ratio are calculated. Visual results display: Display the image quality rating by color coding, from excellent to poor at a glance. History management: automatically save calculation records, which is convenient for comparing the performance of different parameter combinations.
App Store Description
An adaptive optical system performance analysis tool for astronomical observation design. Through accurate physical model calculation, astronomers and telescope operators can be helped to optimize observation parameters and evaluate the correction effect of adaptive optical system. Core functions: Real-time performance analysis: according to the atmospheric conditions, observation wavelength, control system parameters and other factors, the performance index of adaptive optical system is calculated in real time. Multi-parameter adjustment: support the adjustment of key parameters such as atmospheric visibility, observation wavelength, loop frequency, brightness of guiding star and telescope aperture. Professional calculation model: Based on classical optical theories such as Fried parameter and Maréchal approximation, some important indexes such as residual wavefront error and Strehl ratio are calculated. Visual results display: Display the image quality rating by color coding, from excellent to poor at a glance. History management: automatically save calculation records, which is convenient for comparing the performance of different parameter combinations.
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