ISBN: 9789027711984
The aim of this book is to bridge the gap between the pure instrumental physicist and the user of detectors and spectrometers. The essential parameters describing the performance of these… Meer...
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1980, ISBN: 9789027711984
The aim of this book is to bridge the gap between the pure instrumental physicist and the user of detectors and spectrometers. The essential parameters describing the performance of these… Meer...
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ISBN: 9789027711984
The aim of this book is to bridge the gap between the pure instrumental physicist and the user of detectors and spectrometers. The essential parameters describing the performance of these… Meer...
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ISBN: 9789027711984
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ISBN: 9789027711984
The aim of this book is to bridge the gap between the pure instrumental physicist and the user of detectors and spectrometers. The essential parameters describing the performance of these… Meer...
bij Orellfuessli.ch
1980, ISBN: 9789027711984
The aim of this book is to bridge the gap between the pure instrumental physicist and the user of detectors and spectrometers. The essential parameters describing the performance of these… Meer...
ISBN: 9789027711984
The aim of this book is to bridge the gap between the pure instrumental physicist and the user of detectors and spectrometers. The essential parameters describing the performance of these… Meer...
ISBN: 9789027711984
Detection and Spectrometry of Faint Light ab 176.49 € als Taschenbuch: Auflage 1976. Aus dem Bereich: Bücher, Wissenschaft, Physik, Medien > Bücher nein Buch (kartoniert) Hardcover;Naturw… Meer...
1980, ISBN: 9789027711984
Buch, Softcover, 1976 ed. [PU: Kluwer Academic Publishers], Kluwer Academic Publishers, 1980
Bibliografische gegevens van het best passende boek
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Gedetalleerde informatie over het boek. - Detection and Spectrometry of Faint Light
EAN (ISBN-13): 9789027711984
ISBN (ISBN-10): 9027711984
pocket book
Verschijningsjaar: 1980
Uitgever: Springer Netherlands
288 Bladzijden
Gewicht: 0,435 kg
Taal: eng/Englisch
Boek bevindt zich in het datenbestand sinds 2007-07-03T20:36:44+02:00 (Amsterdam)
Boek voor het laatst gevonden op 2024-01-04T15:59:20+01:00 (Amsterdam)
ISBN/EAN: 9027711984
ISBN - alternatieve schrijfwijzen:
90-277-1198-4, 978-90-277-1198-4
alternatieve schrijfwijzen en verwante zoekwoorden:
Auteur van het boek: meaburn
Titel van het boek: detectio, detection and spectrometry faint light, let there light, all the light cannot see
Gegevens van de uitgever
Auteur: J. Meaburn
Titel: Astrophysics and Space Science Library; Detection and Spectrometry of Faint Light
Uitgeverij: Springer; Springer Netherland
273 Bladzijden
Verschijningsjaar: 1980-10-31
Dordrecht; NL
Taal: Engels
160,49 € (DE)
164,99 € (AT)
177,00 CHF (CH)
Available
IX, 273 p.
BC; Hardcover, Softcover / Physik, Astronomie/Astronomie; Astronomische Beobachtung: Observatorien, Ausrüstungen und Methoden; Verstehen; spectrometry; Astronomy, Observations and Techniques; BB
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.Andere boeken die eventueel grote overeenkomsten met dit boek kunnen hebben:
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