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Adaptive optics and wavefront sensing

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Scope of this subject

This cluster of papers focuses on the development, principles, and applications of adaptive optics in astronomy and space telescopes. It covers topics such as wavefront sensing, high angular resolution imaging, laser guide star systems, atmospheric turbulence, deformable mirrors, and the performance of adaptive optics systems in various observatories.

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Research vocabulary

adaptive optics; atmospheric turbulence; wavefront sensing; deformable mirror; Shack-Hartmann wavefront sensor; seeing; high-contrast imaging; wavefront correction; Extremely Large Telescope; exoplanet direct imaging; Strehl ratio; laser guide stars; wavefront reconstruction; wavefront sensor; Zernike polynomials; wavefront aberrations; coronagraphy; multi-conjugate adaptive optics; laser beam propagation; coronagraph; direct imaging; wavefront control; active optics; diffraction-limited imaging; segmented mirror

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Local answer status

No owner-reviewed answer has been published for this exact subject page. This is a gap in this collection; it does not establish that the answer is unavailable elsewhere.

Numeric address and provenance

Morton address: 36253099677624951 · morton4x16-v1

Coordinates: (3, 31, 3107, 11484). The address interleaves categorical identifier bits. Nearby addresses are not guaranteed to describe semantically similar subjects.

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