LEADER 05391nam 2200649Ia 450 001 9910877147603321 005 20200520144314.0 010 $a1-282-01055-7 010 $a9786612010552 010 $a3-527-61784-1 010 $a3-527-61785-X 035 $a(CKB)1000000000377348 035 $a(EBL)481361 035 $a(SSID)ssj0000180895 035 $a(PQKBManifestationID)11172203 035 $a(PQKBTitleCode)TC0000180895 035 $a(PQKBWorkID)10158140 035 $a(PQKB)10641493 035 $a(MiAaPQ)EBC481361 035 $a(OCoLC)212140206 035 $a(EXLCZ)991000000000377348 100 $a20000405d2001 uy 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 10$aInterferometry and synthesis in radio astronomy /$fA. Richard Thompson, James M. Moran, George W. Swenson, Jr 205 $a2nd ed. 210 $aNew York $cWiley$dc2001 215 $a1 online resource (720 p.) 300 $a"A Wiley-Interscience publication." 311 $a3-527-41452-5 311 $a0-471-25492-4 320 $aIncludes bibliographical references and indexes. 327 $aINTERFEROMETRY AND SYlNTHESIS IN RADIO ASTRONOMY; CONTENT'S; Preface to the Second Edition; Preface to the First Edition; 1 Introduction and Historical Review; 1.1 Applications of Radio Interferometry; 1.2 Basic Tenns and Definitions; Cosmic Signals; Source Positions and Nomenclature; Receptiorl of Cosmic Signals; 1.3 Development of Radio Interferometry; Evolution of Synthesis Techniques; Michelson Interferometer; Early Two-Element Radio Interferometers; Sea Interferometer; Phase-Switching Interferometer; Optical Identifications and Calibration Sources; Early Measurements of Angular Width 327 $aSurvey Interferometers and the Mills CrossCentimeter-Wavelength Solar Mapping; Measurements of Intensity Profiles; Spectral Line Interferometry; Earth-Rolation Synthesis Mapping; Development of Synthesis Arrays; Very-Long-Baseline Interferometry; VLBI Using Orbiting Antennas; 1.4 Quantum Effect; 2 Introductory Theory of Interferometry and Synthesis Imaging; 2.1 Planar Analysis; 2.2 Effect of Bandwidth; 2.3 One-Dimensional Source Synthesis; Interferometer Response as a Convolution; Convolution Theorem and Spatial Frequency; Example of One-Dimensional Synthesis; 2.4 Two-Dimensional Synthesis 327 $aProjection-Slice Theorem3 Analysis of the Interferometer Response; 3.1 Fourier Transform Relationship between Intensity and Visibility; 3.2 Cross-Correlation and the Wiener-Khinchin Relation; 3.3 Basic Response of the Receiving System; Antennas; Filters; Correlator; Response to the Incident Radiation; Appendix 3.1 Mathematical Representation of Noise-Like Signals; Analytic Signal; Truncated Function; 4 Geometric Relationships and Polarimetry; 4.1 Antenna Spacing Coordinates and (u, v) Loci; 4.2 (u', v') Plane; 4.3 Fringe Frequency; 4.4 Visibility Frequencies; 4.5 Calibration of the Baseline 327 $a4.6 Antenna Mounts4.7 Beamwidth and Beam-Shape Effects; 4.8 Polarimetry; Parameters Defining Polarization; Antenna Polarization Ellipse; Stokes Visibilities; Instrumental Polarization; Matrix Formulation; Calibration of Instrumental Polarization; Appendix 4.1 Conversion Between Hour Angle-Declination and Azimuth-Elevation Coordinates; Appendix 4.2 Leakage Parameters in Terms of the Polarization Ellipse; Linear Polarization; Circular Polarization; 5 Antennas and Arrays; 5. I Antennas; 5.2 Sampling the Visibility Function; Sampling Theorem; Discrete Two-Dimensional Fourier Transform 327 $a5.3 Introductory Discussion of ArraysPhased Arrays and Correlator Arrays; Spatial Sensitivity and the Spatial Transfer Function; Meter-Wavelength Cross and T Arrays; 5.4 Spatial Transfer Function of a Tracking Array; Desirable Characteristics of the Spatial Transfer Function; Holes in the Spatial Frequency Coverage; 5.5 Linear Tracking Arrays; 5.6 Two-Dimensional Tracking Arrays; Open-Ended Configurations; Closed Configurations; VLBI Configurations; Orbiting VLBI Antennas; Planar Arrays; 5.7 Conclusions on Antenna Configurations; 5.8 Other Considerations; Sensitivity; Long Wavelengths 327 $aMillimeter Wavelengths 330 $aComprehensive, authoritative coverage of interferometric techniques for radio astronomyIn this Second Edition of Interferometry and Synthesis in Radio Astronomy, three leading figures in the development of large imaging arrays, including very-long-baseline interferometry (VLBI), describe and explain the technology that provides images of the universe with an angular resolution as fine as 1/20,000 of an arcsecond.This comprehensive volume begins with a historical review followed by detailed coverage of the theory of interferometry and synthesis imaging, analysis of interferomete 606 $aRadio interferometers 606 $aRadio astronomy 615 0$aRadio interferometers. 615 0$aRadio astronomy. 676 $a522.682 700 $aThompson$b A. R$g(Anthony Richard),$f1931-$01757120 701 $aMoran$b James M$0822951 701 $aSwenson$b George W$g(George Warner),$f1922-$0822952 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910877147603321 996 $aInterferometry and synthesis in radio astronomy$94194793 997 $aUNINA