The use of image stabilization has grown to the point that it is now a common component of modern optical systems for imaging, communications, and remote-sensing applications. The benefits of image stabilization to astronomical research alone are so rich that it is common for astronomical telescopes, built over the last century, to be retrofitted with fast steering mirrors and tip-tilt sensors to extend their useful lifetimes.
This text provides the basics of image stabilization starting with a consid
This volume of the SPIE Tutorial Text explores the fundamental aspects of image
stabilization in optical systems used for astronomy and optical communication systems.
The material is presented with few assumptions about the reader?s previous experience in
the field and should be accessible to most interested readers. Chapter 1 serves as an
introduction to wavefronts, optical systems, and the challenges surrounding image
stabilization. Chapter 2 provides an overview of the effects of atmospheric turbulence on
a wavefront and Chapters 3 and 4 discuss how to sense and minimize these effects,
respectively. In Chapter 5, the devices introduced in the previous two chapters are
combined into an image-stabilization system, with Chapter 6 discussing key performance
issues of such systems. Chapter 7 provides a brief survey of existing image-stabilization
systems. Chapter 8 describes several alternative approaches to image stabilization that,
while less common, can also be effective. Complete coverage of all possible approaches
and methods available for image stabilization is not possible in an introductory text, so
the authors have focused on the most commonly encountered approaches. Also, many of
the subtleties of advanced image-stabilization systems have been left for the interested
reader to explore on his/her own. Many useful reference texts and articles are provided in
Chapter 9.