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Library of Congress Preassigned Control Number Data Keller, Christoph U. Field guide to astronomical instrumentation / Christoph Keller, Ramon Navarro, Bernhard Brandl. pages cm. – (The field guide series ; FG32) Includes bibliographical references and index. ISBN 978-1-62841-177-5 (alk. paper) 1. Astronomical instruments–Handbooks, manuals, etc. I. Navarro, Ramón II. Brandl, Bernhard R. III. Society of Photo-optical Instrumentation Engineers. IV. Title. QB86.K45 2014 522′.87–dc23 2014009876 Published by SPIE P.O. Box 10 Bellingham, Washington 98227-0010 USA Phone: 360.676.3290 Fax: 360.647.1445 Email: Books@spie.org The content of this book reflects the thought of the author(s). Every effort has been made to publish reliable and accurate information herein, but the publisher is not responsible for the validity of the information or for any outcomes resulting from reliance thereon. Printed in the United States of America. First printing. Introduction to the SeriesWelcome to the SPIE Field Guides—a series of publications written directly for the practicing engineer or scientist. Many textbooks and professional reference books cover optical principles and techniques in depth. The aim of the SPIE Field Guides is to distill this information, providing readers with a handy desk or briefcase reference that provides basic, essential information about optical principles, techniques, or phenomena, including definitions and descriptions, key equations, illustrations, application examples, design considerations, and additional resources. A significant effort will be made to provide a consistent notation and style between volumes in the series. Each SPIE Field Guide addresses a major field of optical science and technology. The concept of these Field Guides is a format-intensive presentation based on figures and equations supplemented by concise explanations. In most cases, this modular approach places a single topic on a page, and provides full coverage of that topic on that page. Highlights, insights, and rules of thumb are displayed in sidebars to the main text. The appendices at the end of each Field Guide provide additional information such as related material outside the main scope of the volume, key mathematical relationships, and alternative methods. While complete in their coverage, the concise presentation may not be appropriate for those new to the field. The SPIE Field Guides are intended to be living documents. The modular page-based presentation format allows them to be updated and expanded. We are interested in your suggestions for new Field Guide topics as well as what material should be added to an individual volume to make these Field Guides more useful to you. Please contact us at fieldguides@SPIE.org. John E. Greivenkamp, Series Editor College of Optical Sciences The University of Arizona The Field Guide SeriesKeep information at your fingertips with the SPIE Field Guides:
Field Guide to Astronomical InstrumentationThis Field Guide to Astronomical Instrumentation is the one book that the three of us would want to carry with us if we had to single-handedly design an astronomical instrument on a remote mountain top. To keep it concise, it focuses on the ultraviolet to infrared wavelength range. The Field Guide is not intended to serve as a textbook, but as a handy desktop reference to be found in the labs and offices of instrument builders. This book contains information on a wide range of topics, from fundamental physics to project management, and from technical concepts to material properties. Only the most important concepts and equations are presented here. In many areas, dedicated SPIE Field Guides discuss particular topics in much more detail. While we tried to maintain consistency with other volumes in this series, we wrote this Field Guide in the language that instrumental astronomers use, which might sometimes look strange to people working in other areas. A Field Guide that strives to cover such a wide variety of topics will naturally overlook some potentially relevant topics. We look forward to suggestions from our readers on how to improve this Field Guide for its next edition. Last but not least, we greatly appreciate the continuous support of our families in this endeavor. Christoph U. Keller Leiden Observatory, Leiden University, The Netherlands Ramon Navarro NOVA Optical & Infrared Instrumentation Division at ASTRON, The Netherlands Bernhard R. Brandl Leiden Observatory, Leiden University, The Netherlands Table of ContentsGlossary of Symbols and Acronyms xi General Optics 1 Refraction, Reflection, and Transmission 1 Polarization 2 Brewster Angle and Total Internal Reflection 3 Images, Pupils, and Beams 4 Aberrations 5 Diffraction 6 Point-Spread Function 7 Modulation Transfer Function 8 Spectral Transfer Function 9 Optical Elements 10 Windows 10 Lenses 11 Mirrors 12 Filters 13 Colored Glass Filters 14 Interference Filters 15 Coatings 16 Astronomical Bandpass Filters 17 Prisms 18 Gratings 19 Polarizers 20 Crystal Polarizers 21 Waveplates 22 Optical Fibers 23 Detectors 24 Detector Overview 24 Intrinsic Photoconductors 25 CCD and CMOS Detectors 26 Extrinsic and Stressed Photoconductors 27 BIB Detectors and (Avalanche) Photodiodes 28 Bolometers 29 Coherent (Heterodyne) Detectors 30 CCD and CMOS Readouts 31 Infrared Array Readouts 32 Detector Noise and Artifacts 33 Detector Radiation Effects in Space 34 Detector Flat Fielding 35 Telescopes and Imagers 36 Telescopes 36 Correctors and Wide-Field Imagers 37 Focal Reducers 38 Reimaging Optics 39 High-Resolution Imagers 40 Spectrographs 41 Spectrograph Overview 41 Single-Slit Spectrometer 42 Echelle Spectrometers 43 Slitless Spectrometers 44 Fabry–Pérot Interferometer 45 Fourier Transform Spectrometer 46 Integral Field Spectrometer 47 Multi-object Spectrometer 48 OH-Suppression Spectrographs 49 Spectral Data Analysis 50 Polarimeters 51 Rotating Waveplate Polarimeters 51 Liquid Crystal Polarimeters 52 Spectral Modulation Polarimeters 53 Interferometers 54 Interferometer Principle and Angular Resolution 54 Delay Lines 55 Beam Combiners 56 Fringe Visibility 57 Fringe Tracking and Closure Phase 58 Aperture Synthesis and (u, v) Plane 59 Field of View and Sensitivity 60 Image Processing 61 Coronagraphs 62 Focal-Plane Coronagraphs 62 Pupil-Plane Coronagraphs 63 Space Coronagraphs 64 Adaptive Optics 65 Adaptive Optics 65 Atmospheric Turbulence: Seeing 66 Wavefront Sensors 67 Deformable Mirrors 68 Adaptive Optics Control 69 Laser Guide Stars 70 Operation Modes 71 Optical Design 72 Optical Design Principles 72 Design Approach 73 Ray Tracing 74 Optimization 75 Tolerance Analysis 76 Stray Light Control and Baffles 77 Optomechanics 78 Packaging 78 Optics Mounts 79 Mechanisms 80 Actuators and Motors 81 Sensors 82 Mechanical Engineering for Space 83 Vacuum and Cryogenics 84 Dewars 84 Cooling Methods 85 Thermal Models 86 Thermal Effects in Space 87 Software and Electronics 88 Control 88 Instrument Control System 89 Data Handling 90 Data Transfer from Space 91 Data Analysis Overview 92 Electronics: Cabling 93 Shielding 94 Systems Engineering 95 Systems Engineering: Requirements Definition 95 Block Diagrams 96 Interface Control 97 Error Budgets 98 Noise and its Distribution 99 Signal-to-Noise Ratio 100 Instrument Sensitivity and Integration Time 101 Signal Sampling 102 Project Management 103 Technology Development 104 Risk Management 105 Quality Management 106 Manufacturing, Assembly, Integration, and Testing 107 Optics Manufacturing 107 Optics Testing 108 Alignment 109 Instrument Commissioning 110 Operations and Maintenance 111 Appendices 112 Optical Material Properties 112 Mirror Substrate Material Properties 113 Mechanical Material Properties 114 Material Selection 115 ISO 10110 Optical Drawing Standard 116 ECSS 117 Equation Summary 118 Bibliography 125 Index 127 Glossary of Symbols and Acronyms1D, 2D, 3D One-, two-, or three-dimensional system 4QPM Four-quadrant phase mask
Absorption
Surface area
Telescope aperture
Amplitude of aperture function AC Alternating current ADC Analog-to-digital converter ADC Atmospheric dispersion corrector AG Aplanatic Gregorian AIT Assembly, integration, and testing AIV Assembly, integration, and verification AO Adaptive optics APD Apodizing phase plate APP Avalanche photodiode AR Anti-reflection
Baseline of an interferometer
Bias frame BIB Blocked-impurity-band (detectors) BLIP Background-limited performance BS Beamsplitter CC Closed cycle cooler CCD Charge-coupled device CMOS Complementary metal-oxide semiconductor CNC Computer numerical control CP Closure phase CTE Charge transfer efficiency CTE Coefficient of thermal expansion CWL Center wavelength
Actuator spacing
Dark frame
Diameter
Diameter
Distance
Grating groove spacing
Lens thickness
Telescope diameter DC Direct current DHS Data handling system DQE Detective quantum efficiency DSN Deep space network
Electrical field
Energy
Error signal
Jones vector ECSS European Cooperation for Space Standardization
Bandgap energy ELT Extremely Large Telescope EMC Electromagnetic compatibility EMI Electromagnetic interference ESA European Space Agency ESO European Southern Observatory ETC Exposure time calculator
Finesse
Flat-field frame
Flux
Focal length
Focal ratio, f-number
Frequency
Fresnel number
View factor FDR Final design review FEM Finite element model FFBD Functional Flow Block Diagram
Greenwood frequency FLC Ferro-electric liquid crystals FSR Free spectral range FTS Fourier transform spectrometer FWHM Full width at half maximum
Gain
Strehl ratio gain
Derivative gain in a PID controller
Integral gain in a PID controller
Proportional gain in a PID controller GLAO Ground-layer adaptive optics
Proportional gain in a PID controller GR Generation-recombination
Height of turbulence layer H Near-IR atmospheric band HEB Hot electron bolometer HGA High-gain antenna
Image
Intensity IBF Ion beam figuring ICD Interface control document ICS Instrument control system
Dirty image IFS Integral field spectrometer IFU Integral field unit IR Infrared IRR Integration readiness review J Jones matrix J Near-IR atmospheric band
Zeroth-order Bessel function
First-order Bessel function JWST James Webb Space Telescope
Angular frequency
Conic constant K Near-IR atmospheric band K Temperature in Kelvin
Wave number
Normalized angular frequency
Grating width
Maximum path length difference L2 Second Lagrangian point LCVR Liquid crystal variable retarders LGS Laser guide star LHe Liquid helium
Liquid nitrogen LO Local oscillator LSST Large Synoptic Survey Telescope LVDT Linear variable differential transformer
Grating order, order of diffraction
Mueller matrix mbar Millibar pressure MCAO Multi-conjugate adaptive optics MEMS Micro-electro-mechanical system MKID Microwave kinetic inductance detector MLI Multi-layer isolation MOAO Multi-object adaptive optics MOS Multi-object spectrometer MTF Modulation transfer function
Index of refraction
Noise
Number of actuators
Number of illuminated grooves
Number of photons
Number of telescopes NA Numerical aperture NASA National Aeronautics and Space Administration
Effective index of refraction NGS Natural guide star
Index of refraction of medium
number of photons per
Index of refraction of substrate
Object OCS Observatory control system OPD Optical path difference OTCCD Orthogonal-transfer CCD OTF Optical transfer function
Degree of polarization
Point spread function
Poke matrix
Pressure
Instrumental profile
Probability for value around a mean PDR Preliminary design review PEM Piezo-elastic modulator PIAA Phase-induced amplitude apodization PID Proportional-integral-derivative
Degree of linear polarization PS Point source (diffraction limited) PSF Point spread function Pt100, Pt1000 Platinum temperature sensor PTF Phase transfer function PVA Polyvinyl alcohol
Heat transfer
Stokes Q QA Quality assurance QC Quality control QMS Quality management system
Radial distance
Radius of curvature
Reconstructor
Reflectivity
Spectral resolution R&D Research and development
Fried’s parameter RAM Risk assessment matrix RAMS Risk assessment and method statement RC Ritchey–Chrétien (telescope) RFI Radio frequency interference RMS Root mean square ROI Region of interest
Reflection amplitude for p-polarization
Reflection amplitude for s-polarization RVDT Rotary variable differential transformer
Rotation around coordinates
Science frame
Sensor data
Signal
Stokes vector SH Shack–Hartmann wavefront sensor Si Silicon SIS Superconductor–insulator–superconductor SL Seeing limited SNR Signal-to-noise ratio STEP Standard for exchange of product data STF Spectral transfer function SUR Sample-up-the-ramp
Temperature
Thickness
Time
Transmission T1, T2 Telescopes TCS Telescope control system
Dark frame exposure time TDRSS Tracking and data relay satellite system TES Transition edge sensor
Flat-field frame exposure time TIR Total internal reflection TIS Total integrated scatter TLR Top-level requirements TMA Three-mirror anastigmat
Transmission amplitude for -polarization TRL Technology readiness level
Science frame exposure time
Transmission amplitude for s-polarization
Translation in coordinates
Control signal
Coordinates in Fourier space
Stokes U UV Ultraviolet
Fringe visibility
Stokes V
Wind speed VPH Volume phase hologram W Watt WBS Work breakdown structure WFS Wavefront sensor
Weighting coefficient
Path-length difference
coordinates
Actuator position
Distance from field center
Yield strength
Surface zag
Zenith angle
Linear polarization orientation
Absorption coefficient
Prism apex angle
Incident angle on grating
Reflected angle on grating
Groove center to edge phase difference
Phase change on total internal reflection
Retardation in birefringent material
Dispersion angle
Angle of linear polarization
OPD in an interferometer
Filter transmission profile FWHM
Spectral resolution element
Emissivity
Relative grating efficiency
Throughput
Half-angle
Position or rotation angle
Angular resolution in radians
Brewster angle
Blaze angle
Angle of incidence
Refracted angle of incidence
Isoplanatic angle
Angle of dispersed beam
Angle of reflected beam
Angle of transmitted beam
Wavelength
Blaze wavelength
Center wavelength
Cutoff wavelength
Free spectral range m micrometer
Frequency
Stefan Boltzmann constant
Standard deviation
Control system lag induced variance
Fitting error induced variance
Anisoplanatism wavefront variance
Total wavefront variance
Wavefront sensor induced variance
Internal transmission
Frequency in Nyquist sampling
Internal transmission
Servo lag time
Atmospheric coherence time
Intrinsic phase
Observed phase
Phase shifted by atmospheric effects
Angular slit width
Phase of aperture function
Wedge angle
Angular frequency |
CITATIONS
Adaptive optics
Astronomical imaging
Atmospheric optics
Geometrical optics
CCD image sensors
Infrared sensors
Sensors