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About Principles of Adaptive Optics and New Challenges For Extremely Large Astronomical Telescopes
This document discusses the principles of adaptive optics and challenges for extremely large telescopes. It begins by outlining the history of ground-based astronomy from Galileo's small telescopes to modern very large telescopes and upcoming extremely large telescopes with diameters over 40 meters. It then discusses how atmospheric turbulence limits resolution and how adaptive optics aims to correct for this to achieve near-diffraction limited imaging. Key components of adaptive optics including deformable mirrors, wavefront sensors, reconstruction and control are introduced. Modal representations of the turbulent phase such as Zernike polynomials and Karhunen-Loeve modes are discussed. The transition from current very large telescopes to future extremely large telescopes and the new challenges this brings are also summarized
Detailed Information
| Author: | ['bhansalianiket96'] |
|---|---|
| Publication Year: | 2013 |
| Pages: | 45 |
| Language: | English |
| Format: | |
| Price: | FREE |
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