Optics In Astronomy
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Author | : Daniel J. Schroeder |
Publisher | : Elsevier |
Total Pages | : 367 |
Release | : 2012-12-02 |
Genre | : Science |
ISBN | : 032313856X |
Written by a recognized expert in the field, this clearly presented, well-illustrated book provides both advanced level students and professionals with an authoritative, thorough presentation of the characteristics, including advantages and limitations, of telescopes and spectrographic instruments used by astronomers of today. - Written by a recognized expert in the field - Provides both advanced level students and professionals with an authoritative, thorough presentation of the characteristics, including advantages and limitations, of telescopes and spectrographic instruments used by astronomers of today
Author | : François Roddier |
Publisher | : Cambridge University Press |
Total Pages | : 421 |
Release | : 1999-06-17 |
Genre | : Science |
ISBN | : 052155375X |
Adaptive optics is set to revolutionise the future of astronomy; this is the first book on the subject and is set to become the standard reference.
Author | : John W. Hardy |
Publisher | : Oxford Optical and Imaging Sci |
Total Pages | : 452 |
Release | : 1998 |
Genre | : Science |
ISBN | : 9780195090192 |
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.
Author | : N. Ageorges |
Publisher | : Springer Science & Business Media |
Total Pages | : 362 |
Release | : 2013-04-17 |
Genre | : Science |
ISBN | : 9401596247 |
Adaptive optics allows the theoretical limit of angular resolution to be achieved from a large telescope, despite the presence of turbulence. Thus an eight meter class telescope, such as one of the four in the Very Large Telescope operated by ESO in Chile, will in future be routinely capable of an angular resolution of almost 0.01 arcsec, compared tot he present resolution of about 0.5 arcsec for conventional imaging in good condition. All the world's major telescopes either have adaptive optics or are in the process of building AO systems. It turns out that a reasonable fraction of the sky can be observed using adaptive optics, with moderately good imaging quality, provided imaging in done in the near IR. To move out of the near IR, with its relatively poor angular resolution, astronomers need a laser guide star. There is a layer of Na atoms at approximately 90 km altitude that can be excited by a laser to produce such a source, or Rayleigh scattering can be employed lower in the atmosphere. But the production and use of laser guide stars is not trivial, and the key issues determining their successful implementation are discussed here, including the physics of the Na atom, the cone effect, tilt determination, sky coverage, and numerous potential astronomical applications.
Author | : Stefano Minardi |
Publisher | : VCH |
Total Pages | : 350 |
Release | : 2012-04-04 |
Genre | : |
ISBN | : 9783527411108 |
Written by well-known scientists in the field with vast experience in teaching astrophotonics, this is the first book to bridge astronomy and photonics for the benefit of developing new astronomical instrumentation. The textbook is clearly structured and covers four main methods relevant to observational astronomy: adaptive optics, photometry, interferometry and spectroscopy. It follows a progressive didactical path in photonics, starting from fundamentals of wave- and micro-optics and developing step-by-step the formalisms required for the treatment of optical multilayers, fiber optics and diffraction/holographic gratings. This approach allows students with a physics/engineering background to learn about the problematic of observational astronomy, while, conversely, students of astronomy are exposed to topics in modern photonics. Each chapter is divided into three main sections devoted to the discussion of astronomical concepts required to size an instrument designed for the particular method, the photonic concepts that most suit that instrument, and an analysis of existing, related photonic instruments. A set of exercises and a bibliography complete each chapter. Appendices include a short review of fundamentals of wave optics and photon detectors, plus an overview of project design and management using a real-life example of an astronomical instrumentation project. With its review of the latest instrumentation and techniques, this is invaluable for graduate and post-graduate students in astronomy, physics and optical engineering.
Author | : Gérard René Lemaitre |
Publisher | : Springer Science & Business Media |
Total Pages | : 575 |
Release | : 2008-12-04 |
Genre | : Science |
ISBN | : 3540689052 |
Astronomical Optics and Elasticity Theory provides a very thorough and comprehensive account of what is known in this field. After an extensive introduction to optics and elasticity, the book discusses variable curvature and multimode deformable mirrors, as well as, in depth, active optics, its theory and applications. Further, optical design utilizing the Schmidt concept and various types of Schmidt correctors, as well as the elasticity theory of thin plates and shells are elaborated upon. Several active optics methods are developed for obtaining aberration corrected diffraction gratings. Further, a weakly conical shell theory of elasticity is elaborated for the aspherization of grazing incidence telescope mirrors. The very didactic and fairly easy-to-read presentation of the topic will enable PhD students and young researchers to actively participate in challenging astronomical optics and instrumentation projects.
Author | : Harrie G. J. Rutten |
Publisher | : |
Total Pages | : 392 |
Release | : 1988 |
Genre | : Science |
ISBN | : |
Author | : Lawrence Mertz |
Publisher | : Springer Science & Business Media |
Total Pages | : 170 |
Release | : 1996-06-20 |
Genre | : Science |
ISBN | : 9780387946641 |
These "excursions" into astronomical optics discuss innovative, often radical, suggestions for the design of optical instruments. Providing a storehouse of ideas and approaches not available elsewhere, Mertz suggests opportunities for further exploration and development rather than proven solutions. Covering a wide array of topics, from x-ray telescopes to gravitational lenses and from microscope objectives to Fourier transform spectroscopy, the excursions share a common thread of optical science related to astronomy. The book should thus interest researchers and graduate students in astronomy, optics, and optical engineering. Appendices provide Fortran code for some of the design techniques discussed in the book and for Monte Carlo image synthesis
Author | : Jim Bernard Breckinridge |
Publisher | : SPIE-International Society for Optical Engineering |
Total Pages | : 0 |
Release | : 2012 |
Genre | : Astronomical instruments |
ISBN | : 9780819483669 |
This text was written to provide students of astronomy and engineers an understanding of optical science - the study of the generation, propagation, control, and measurement of optical radiation - as it applies to telescopes and instruments for astronomical research in the areas of astrophysics, astrometry, exoplanet characterization, and planetary science. The book provides an overview of the elements of optical design and physical optics within the framework of the needs of the astronomical community.
Author | : Raymond N. Wilson |
Publisher | : Springer Science & Business Media |
Total Pages | : 551 |
Release | : 2013-03-09 |
Genre | : Science |
ISBN | : 3662032279 |
This is the first volume of a monumental work that will provide a complete treatment of all theoretical aspects of reflecting telescope optics. It addresses all specialists in the field, both within the astronomical community and in industry, and, consequently, particular emphasis is placed on subjects such as practical alignment, test techniques, and maintenance aspects. Whereas the second volume will concentrate on technical aspects and modern developments, this one is devoted to the theory of reflecting telescope optics and, together with the historical development, it will also prove to be useful to students. This book has real classic potential.