Adaptive Optics for Astronomical Telescopes
Adaptive Optics for Astronomical Telescopes
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DOI：
10.1063/1.883053
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发表时间：
1998-07
期刊：
影响因子：
3.5
通讯作者：
J. Hardy;L. Thompson
中科院分区：
文献类型：
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作者：
J. Hardy;L. Thompson
这本书由自适应光学领域的一位领导者撰写，涵盖了基本理论，然后详细描述了如何将这项技术应用于大型地面望远镜，以补偿大气湍流的影响。它包括基本的自适应光学元件和技术的信息，并有专门的章节大气湍流，光学图像结构，激光信标，和整体系统设计。系统设计一章特别详细，包括性能估计和优化。结合物理原理的明确讨论与众多现实世界的例子，这本书将是一个宝贵的资源，为所有研究生和研究人员在天文学和光学。
This book by one of the leaders in adaptive optics covers the fundamental theory and then describes in detail how this technology can be applied to large ground-based telescopes to compensate for the effects of atmospheric turbulence. It includes information on basic adaptive optics components and technology, and has chapters devoted to atmospheric turbulence, optical image structure, laser beacons, and overall system design. The chapter on system design is particularly detailed and includes performance estimation and optimization. Combining a clear discussion of physical principles with numerous real-world examples, this book will be a valuable resource for all graduate students and researchers in astronomy and optics.