02814nam 2200589Ia 450 991080941350332120230721025415.01-281-12193-29786611121938981-270-888-X(CKB)1000000000334106(EBL)312398(OCoLC)476100201(SSID)ssj0000138940(PQKBManifestationID)11158583(PQKBTitleCode)TC0000138940(PQKBWorkID)10107990(PQKB)10670077(MiAaPQ)EBC312398(WSP)00006492(Au-PeEL)EBL312398(CaPaEBR)ebr10188746(CaONFJC)MIL112193(OCoLC)935264104(EXLCZ)99100000000033410620070720d2007 uy 0engur|n|---|||||txtccrDiffraction-limited imaging with large and moderate telescopes[electronic resource] /Swapan K. SahaSingapore ;Hackensack, NJ World Scientificc20071 online resource (633 p.)Description based upon print version of record.981-270-777-8 Includes bibliography (p. 579-594) and index.Preface; Principal symbols; List of acronyms; Contents; 1. Introduction to electromagnetic theory; 2. Wave optics and polarization; 3. Interference and diffraction; 4. Image formation; 5. Theory of atmospheric turbulence; 6. Speckle imaging; 7. Adaptive optics; 8. High resolution detectors; 9. Image processing; 10. Astronomy fundamentals; 11. Astronomical applications; Appendix A Typical tables; Appendix B Basic mathematics for Fourier optics; Appendix C Bispectrum and phase values using triplecorrelation algorithm; Bibliography; IndexThis book deals with the fundamentals of wave optics, polarization, interference, diffraction, imaging, and the origin, properties, and optical effects of turbulence in the Earth's atmosphere. Techniques developed during the last few decades to overcome atmospheric image degradation (including passive methods, speckle interferometry in particular, and active methods such as adaptive optics), are highlighted. Also discussed are high resolution sensors, image processing, and the astronomical results obtained with these techniques.Imaging systems in astronomyTelescopesImaging systems in astronomy.Telescopes.522/.2Saha Swapan K1156379MiAaPQMiAaPQMiAaPQBOOK9910809413503321Diffraction-limited imaging with large and moderate telescopes4127171UNINA