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In both mirror models the slope depends on the energy.
The structure of the PSFs is very similar, emphasizing how good both mirror models are.
The 'table-top mirror' models of this proposed circuit have been shown here.
As a case study, we apply these test methods to secondary segmented mirror models of the Giant Magellan Telescope.
Different from the existing event-driven control approaches for systems with completely unknown nonlinearities, the main contribution of this paper is to design a simple event-based tracking scheme with preassigned performance, without the use of adaptive function approximators and adaptive mirror models.
Those features are obtained by exploiting the peculiarities of wavelet transforms, which can perform mirror models of spatial decompositions occurring in the V1 area of the primary visual cortex.
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SAOTrace, the offical Chandra mirror model simulator used by ChaRT uses the quaternion values.
The pure marx simulations have much larger deviations due to marx's simplified mirror model.
Both the marx and the SAOTrace mirror model also have energy dependent exponents.
Using SAOTrace as a mirror model, gives better results but they still differ significantly from the observed distribution.
The SAOTrace mirror model produces a smoother distribution that is more similar to the observed data tan marx.
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