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Tomographic reconstruction for wide-field adaptive optics systems: Fourier domain analysis and fundamental limitations

机译:宽视场自适应光学系统的层析成像重建:傅里叶域分析和基本局限性

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摘要

Several wide-field-of-view adaptive optics (WFAO) concepts such as multi-conjugate AO (MCAO), multi-object AO (MOAO), and ground-layer AO (GLAO) are currently being studied for the next generation of Extremely Large Telescopes (ELTs). All these concepts will use atmospheric tomography to reconstruct the turbulent-phase volume. In this paper, we explore different reconstruction algorithms and their fundamental limitations, conducting this analysis in the Fourier domain. This approach allows us to derive simple analytical formulations for the different configurations and brings a comprehensive view of WFAO limitations. We then investigate model and statistical errors and their effect on the phase reconstruction. Finally, we show some examples of different WFAO systems and their expected performance on a 42 m telescope case.
机译:目前正在研究多种广视场自适应光学(WFAO)概念,例如多共轭AO(MCAO),多对象AO(MOAO)和地层AO(GLAO),用于下一代Extremely大型望远镜(ELT)。所有这些概念都将使用大气层析成像技术来重建湍流相体积。在本文中,我们探索了不同的重建算法及其基本局限性,并在傅立叶域中进行了分析。这种方法使我们可以为不同的配置导出简单的分析公式,并全面了解WFAO的局限性。然后,我们调查模型和统计误差及其对相位重建的影响。最后,我们展示了一些不同WFAO系统及其在42 m望远镜盒上的预期性能的示例。

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