Detection and Spectrometry of Faint Light

Author:   J. Meaburn
Publisher:   Springer
Edition:   1976 ed.
Volume:   56
ISBN:  

9789027711984


Pages:   273
Publication Date:   31 October 1980
Format:   Paperback
Availability:   In Print   Availability explained
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Detection and Spectrometry of Faint Light


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Author:   J. Meaburn
Publisher:   Springer
Imprint:   Kluwer Academic Publishers
Edition:   1976 ed.
Volume:   56
Dimensions:   Width: 15.50cm , Height: 1.50cm , Length: 23.50cm
Weight:   0.900kg
ISBN:  

9789027711984


ISBN 10:   9027711984
Pages:   273
Publication Date:   31 October 1980
Audience:   Professional and scholarly ,  Professional & Vocational
Format:   Paperback
Publisher's Status:   Active
Availability:   In Print   Availability explained
This item will be ordered in for you from one of our suppliers. Upon receipt, we will promptly dispatch it out to you. For in store availability, please contact us.

Table of Contents

1. The Principles of Spectrometry.- 1.1 Introduction.- 1.2. Parameters which Define a Spectrometer.- 1.3. Instrumental Profile.- 1.4. Free Spectral Range.- 1.5. Maximum Wavelength Resolution.- 1.6. Brightness of a Source.- 1.7. Luminosity of a Spectrometer.- 1.8. Flux.- 1.9. Luminosity Resolution Product.- 1.10. Spectral Simultaneity Gain.- 1.11. Spatial Simultaneity Gain.- 1.12. Responsive Quantum Efficiency.- 1.13. A Factor of Merit for a Spectrometer.- 1.14. Combining a Spectrometer with a Telescope.- 2. The Quantum Detectors.- 2.1. Introduction.- 2.2. Performance.- 2.3. Responsive Quantum Efficiency and its Variations.- 2.4. Receiver Noise.- 2.5. Detective Quantum Efficiency.- 2.6. Multiplicity.- 2.7. Event Capacity.- 2.8. Linearity of Response.- 2.9. Dynamic Range.- 2.10. Linear Resolution.- 2.11. Operation.- 2.12. The Photographic Emulsion.- 2.13. The Photocathode.- 2.14. The Photomultiplier.- 2.15. The Electronic Image Tubes.- 2.16. Phosphor Output Tubes.- 2.17. Electronographic Tubes.- 2.18. Digital Image Tubes.- 3. The Prism Spectrometers.- 3.1. Introduction.- 3.2. Comparisons.- 3.3. Objective Prism Spectrographs.- 3.4. The Single-Slit, Single-Detector Prism Monochromator.- 4. Useful Diffraction Gratings.- 4.1. Introduction.- 4.2. Principles.- 4.3. Maxima.- 4.4. Blazing.- 4.5. Practical Plane Reflection Gratings.- 4.6. Ebert Configuration.- 4.7. Littrow Configuration.- 4.8. Practical Plane Transmission Gratings.- 4.9. Gratings in Series or with Multiple Dispersions.- 4.10. Classically Combining a Dispersive Grating Spectrometer with an Astronomical Telescope.- 5. Dispersive Spectrometers Employing Gratings.- 5.1. The Single-Entrance Slit Blazed-Grating Spectographs.- 5.2. The Slitless Blazed-Grating Spectrograph.- 5.3. The Multi-Entrance Slit Blazed Grating Spectrograph.- 5.4. The Single-Entrance Slit, Multi-Exit Slit, Blazed-Grating Monochromator.- 5.5. The Single-Entrance and Exit Slit, Blazed-Grating Monochromators.- 5.6. The Single-Entrance Slit, Many-Photomultiplier, Blazed-Grating Polychromator.- 5.7. The Multi-Band, Blazed-Grating Spectrograph.- 5.8. The Multi-Entrance and Exit-Slit, Single-Photomultiplier Blazed-Grating Monochromator.- 5.9. Objective and Non-Objective Blazed-Grating Spectrographs.- 5.10. The Blazed-Grating Monochromators with Grilles.- 5.11. The Coded-Mask, Multiplex, Grating Spectrometers.- 6. Useful High-Order Plane Fabry-Pérot Etalons.- 6.1. Introduction.- 6.2. Theory.- 6.3. All-Dielectric Multilayer Reflection Coatings.- 6.4. Cavity Losses.- 6.5. Acceptance Solid Angle.- 6.6. Defects.- 6.7. The Effective Finesse.- 6.8. Luminosity-Resolution Product.- 6.9. Scanning and Tuning Fabry-Pérots.- 6.10. Practical Fabry-Pérots — Optically-Contacted Etalons.- 6.11. Exact Fractions for a Pressure Tuned Fabry-Pérot.- 6.12. Practical Fabry-Pérots — Piezo-Mounted Etalons.- 6.13. Practical Fabry-Pérots — Solid High-Order Etalons.- 6.14. The Spherical Fabry-Pérot.- 7. Interference Filters and Their Cameras.- 7.1. Introduction.- 7.2. Luminosity Resolution Product.- 7.3. Variation of the Pass-Band Maximum across the Diameter.- 7.4. Position of the Passband Maximum On-Axis.- 7.5. Variations of the Passband Maximum with Temperature.- 7.6. Variations of the Passband Maximum with Time.- 7.7. Cameras Exploiting Interference Filters.- 7.8. Direct and Quasi-Telecentric Filter Cameras.- 7.9. Telecentric Filter Cameras.- 7.10. Classically Combining a Filter Camera.- 7.11. Wide Field Cameras.- 8. The High-Order Fabry-Pérot Spectrometers.- 8.1. Introduction.- 8.2. The Classical Fabry-Pérot Spectrograph.- 8.3.The High-Order, Gas-Spaced, Fabry-Pérot as a Variable, Narrow Filter.- 8.4. The Non-Classical Fabry-Pérot Spectrograph.- 8.5. The Insect-Eye Fabry-Pérot Spectrograph.- 8.6. The Classical, Single-Fringe, Gas-Spaced Fabry-Pérot Monochromator.- 8.7. The Non-Classical (Telecentric) Single-Fringe, Gas-Spaced, Fabry-Pérot Monochromator.- 8.8. The Classical Multi-Fringe, Gas-Spaced Fabry-Pérot Monochromator.- 8.9. The Multi-Etalon, Single-Fringe, Fabry-Pérot, Monochromators (PEPSIOS).- 9. The Fourier Transform Spectrometers.- 9.1. Introduction.- 9.2. Two-Beam Interferometric Fourier Transform Spectrometers.- 9.3. Lamellar Grating Fourier Transform Spectrometers.- 10. Some Crossed Spectrometers.- 10.1. Grating × Fabry-Pérot Monochromators and Polychromators.- 10.2. The SISAM Monochromator.- 10.3. The SISAM × Fabry-Pérot Monochromator.- 11. Signal to Noise Ratios—The Principal Criteria of Merit.- 11.1. Introduction.- 11.2. Types of Noise.- 11.3. Problem 1.- 11.4. Problem 2.- 11.5. Problem 3.- 11.6. General Comment.

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