Astrophysical Techniques. C R Kitchin
|
|
- Ashlynn Amberly Walsh
- 8 years ago
- Views:
Transcription
1 Astrophysical Techniques C R Kitchin University of Hertfordshire Observatory Third Edition SUB Gottingen A 8843 Institute of Physics Publishing Bristol and Philadelphia
2 Contents Preface Standard symbols xiii xv 1 Detectors OPTICAL AND INFRARED DETECTION 1 Introduction 1 Detectors 1 Detector types 1 The eye 2 Photomultipliers 7 A detector breviary 18 Charge-coupled devices (CCD) 20 Other types of detectors 30 Photovoltaic cells 30 Photoelectromagnetic detectors 33 Thermocouples 33 Pyroelectric detectors 34 Bolometers 34 Photoconductive cells 35 Phototransistors 36 Charge injection devices (CID) 36 Photographic emulsion 37 Gas cells 37 Television tubes 37 Image intensifiers 37 Golay cell 37 Ultraviolet detectors 37 Future possibilities 38 Noise. 39 Intrinsic noise 39 Signal noise 40 Digitisation 41 vii
3 viii CONTENTS Telescopes 42 Optical theory 42 Telescope designs 62 Exercises ' RADIO AND MICROWAVE DETECTION 91 Introduction 91 Detectors and receivers 92 Radio telescopes 97 Construction 105 Exercises X-RAY AND GAMMA-RAY DETECTION 107 Introduction 107 Detectors 109 Geiger counters 109 Proportional counters 110 Scintillation detectors 111 Gas scintillation proportional counters 112 Charge coupled devices 112 Compton interaction detectors 113 Spark detectors 113 Cerenkov detectors 113 Solid state detectors 113 MicroChannel plates 114 Nuclear emulsions 115 Shielding 116 Imaging 116 Collimation 117 Coincidence detectors 120 Occultation 120 Reflecting telescopes 120 Resolution and image identification 125 Spectroscopy 126 Grating spectrometers 126 Bragg spectrometers 127 Polarimetry 129 Observing platforms COSMIC RAY DETECTORS 131 Background 131 Detectors 131 Real-time methods 132 Residual track detectors 138 Indirect detectors 143 Arrays 144
4 CONTENTS ix Correction factors 145 Atmospheric effects. 145 Solar effects Terrestrial magnetic field ' 146 Exercises NEUTRINO DETECTORS 149 Background 149 Chlorine 37 detectors 151 Water-based detectors 153 Gallium-based detectors 155 Other types of detectors 155 Direct interaction type detectors 155 Indirect interaction type detectors 156 Geological detectors 156 Scattering detectors 157 Exercises GRAVITATIONAL RADIATION 158 Introduction 158 Detectors 160 Direct resonant detectors 160 Direct, non-resonant detectors 161 Indirect detectors 163 Exercises Imaging THE INVERSE PROBLEM 165 Deconvolution PHOTOGRAPHY 170 Introduction 170 Structure of the photographic emulsion 171 The photographic image 174 Processing 182 Hypersensitisation 185 Temperature effects 186 Liquid bathing effects 186 Gas immersion effects 186 Pre-exposure 187 Post-exposure techniques 187 Faint image contrast enhancement 188 Autoradiographic image retrieval 188 Film types '. 188 Techniques of astronomical photography 189 Analysis of photographic images 190 Special applications 191
5 CONTENTS 2.3 ELECTRONIC IMAGING Introduction Arrays Television and related systems Image intensifies Magnetically focused image intensifies Electrostatically focused image intensifies Proximity focused image intensifies Cascades Recording Photon counting imaging systems Electronographic cameras 2.4 SCANNING 2.5 INTERFEROMETRY Introduction Michelson radio interferometer Michelson stellar interferometer Intensity interferometer Reflection interferometers Exercises 2.6 SPECKLE INTERFEROMETRY 2.7 OCCULTATIONS Background Techniques Analysis 2.8 RADAR Introduction Theoretical principles Equipment Data analysis Meteors Exercise 2.9 ELECTRONIC IMAGES Image formats Image compression Image processing Grey scaling Image combination Spatial filtering Photometry 3.1 PHOTOMETRY Background Magnitudes
6 CONTENTS xi Filter systems 262 Stellar parameters 266 Exercises PHOTOMETERS 281 Instruments 281 Visual photometers 282 Photographic photometry 282 Photoelectric photometers 286 Observing techniques 294 Data reduction and analysis 297 Exercise 300 Spectroscopy SPECTROSCOPY 301 Optics 301 Prisms 301 Diffraction gratings 312 Interferometers 320 Fabry-Perot interferometer 320 Michelson interferometer 327 Holography 333 Exercises SPECTROSCOPES 334 Basic design considerations 334 Prism-based spectroscopes 341 Grating spectroscopes 345 Techniques of spectroscopy 348 Future developments 355 Exercises 355 Other Techniques ASTROMETRY 356 Background 356 Coordinate systems 356 Position angle and separation 358 Micrometers 359 Photography 364 Electronic images 366 Measurement and reduction 366 Exercises POLARIMETRY 368 Background 368 Stokes' parameters 369
7 xii CONTENTS Optical components for polarimetry 372 Birefringence 372 Polarisers ^ 375 Converters 379 Depolarises 383 Polarimeters 383 Photographic polarimeters 384 Photoelectric polarimeters 385 Data reduction and analysis 388 Exercises SOLAR STUDIES 390 Introduction 390 Solar telescopes 391 Spectrohelioscope 394 Narrow band filters 395 Coronagraph 401 Solar oscillations 403 Other solar observing methods 404 Exercise MAGNETOMETRY 405 Background 405 Zeemah effect 405 Magnetometers 412 Data reduction and analysis 416 Appendices 417 I Magnitudes and spectral types of bright stars 417 II North polar sequence 420 III Standard stars for the UBV photometric system 423 IV Standard stars for the uvby photometric system 426 V Standard stars for MK spectral types 435 VI Standard stars for polarimetry 443 VII Julian date 445 VIII Catalogues 447 IX Answers to the exercises 449 Bibliography 451 Index 458
Optical Metrology. Third Edition. Kjell J. Gasvik Spectra Vision AS, Trondheim, Norway JOHN WILEY & SONS, LTD
2008 AGI-Information Management Consultants May be used for personal purporses only or by libraries associated to dandelon.com network. Optical Metrology Third Edition Kjell J. Gasvik Spectra Vision AS,
More informationIntroduction to Optics
Second Edition Introduction to Optics FRANK L. PEDROTTI, S.J. Marquette University Milwaukee, Wisconsin Vatican Radio, Rome LENO S. PEDROTTI Center for Occupational Research and Development Waco, Texas
More informationSolar Ast ro p h y s ics
Peter V. Foukal Solar Ast ro p h y s ics Second, Revised Edition WI LEY- VCH WILEY-VCH Verlag Co. KCaA Contents Preface 1 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.9 2 2.1 2.1.1 2.1.2 2.2 2.2.1 2.2.2 2.2.3 2.3
More informationModern Classical Optics
Modern Classical Optics GEOFFREY BROOKER Department of Physics University of Oxford OXPORD UNIVERSITY PRESS Contents 1 Electromagnetism and basic optics 1 1.1 Introduction 1 1.2 The Maxwell equations 1
More informationIntroduction to CCDs and CCD Data Calibration
Introduction to CCDs and CCD Data Calibration Dr. William Welsh San Diego State University CCD: charge coupled devices integrated circuit silicon chips that can record optical (and X-ray) light pixel =
More informationfor Communication Systems Protection EMI CD-ROM INCLUDED
Krešimir Malarić EMI Protection for Communication Systems CD-ROM INCLUDED Contents Preface xiii CHAPTER 1 Communications Systems 1 1.1 Components of Communications Systems 1 1.2 Transmitter Systems 2 1.2.1
More informationSpectroscopy and Regions of the Spectrum
Basics 9 Spectroscopy and Regions of the Spectrum Different regions of the spectrum probe different types of energy levels of an atomic or molecular system. It is not uncommon to refer to a spectroscopic
More informationUse the following image to answer the next question. 1. Which of the following rows identifies the electrical charge on A and B shown above?
Old Science 30 Physics Practice Test A on Fields and EMR Test Solutions on the Portal Site Use the following image to answer the next question 1. Which of the following rows identifies the electrical charge
More informationPhysics 30 Worksheet # 14: Michelson Experiment
Physics 30 Worksheet # 14: Michelson Experiment 1. The speed of light found by a Michelson experiment was found to be 2.90 x 10 8 m/s. If the two hills were 20.0 km apart, what was the frequency of the
More information5. The Nature of Light. Does Light Travel Infinitely Fast? EMR Travels At Finite Speed. EMR: Electric & Magnetic Waves
5. The Nature of Light Light travels in vacuum at 3.0. 10 8 m/s Light is one form of electromagnetic radiation Continuous radiation: Based on temperature Wien s Law & the Stefan-Boltzmann Law Light has
More informationHow Does One Obtain Spectral +Imaging Data
How Does One Obtain Spectral +Imaging Data What we observe depends on the instruments that one observes with! In x and γ-ray spectroscopy we have a wide variety of instruments with different properties
More informationSynthetic Sensing: Proximity / Distance Sensors
Synthetic Sensing: Proximity / Distance Sensors MediaRobotics Lab, February 2010 Proximity detection is dependent on the object of interest. One size does not fit all For non-contact distance measurement,
More informationHTRA Instrumentation I
HTRA Instrumentation I Phil Charles (Univ. of Southampton) Lecture 1: 1. Introduction, basic concepts of HTRA 2. History (~60yrs) of HTRA 3. Space science developments multi-wavelength 4. Fast timing in
More informationCalifornia Standards Grades 9 12 Boardworks 2009 Science Contents Standards Mapping
California Standards Grades 912 Boardworks 2009 Science Contents Standards Mapping Earth Sciences Earth s Place in the Universe 1. Astronomy and planetary exploration reveal the solar system s structure,
More informationChapter 6 Telescopes: Portals of Discovery. How does your eye form an image? Refraction. Example: Refraction at Sunset.
Chapter 6 Telescopes: Portals of Discovery 6.1 Eyes and Cameras: Everyday Light Sensors Our goals for learning:! How does your eye form an image?! How do we record images? How does your eye form an image?
More informationTutorial 4.6 Gamma Spectrum Analysis
Tutorial 4.6 Gamma Spectrum Analysis Slide 1. Gamma Spectrum Analysis In this module, we will apply the concepts that were discussed in Tutorial 4.1, Interactions of Radiation with Matter. Slide 2. Learning
More informationSchneps, Leila; Colmez, Coralie. Math on Trial : How Numbers Get Used and Abused in the Courtroom. New York, NY, USA: Basic Books, 2013. p i.
New York, NY, USA: Basic Books, 2013. p i. http://site.ebrary.com/lib/mcgill/doc?id=10665296&ppg=2 New York, NY, USA: Basic Books, 2013. p ii. http://site.ebrary.com/lib/mcgill/doc?id=10665296&ppg=3 New
More informationRESULTS FROM A SIMPLE INFRARED CLOUD DETECTOR
RESULTS FROM A SIMPLE INFRARED CLOUD DETECTOR A. Maghrabi 1 and R. Clay 2 1 Institute of Astronomical and Geophysical Research, King Abdulaziz City For Science and Technology, P.O. Box 6086 Riyadh 11442,
More informationDetecting and measuring faint point sources with a CCD
Detecting and measuring faint point sources with a CCD Herbert Raab a,b a Astronomical ociety of Linz, ternwarteweg 5, A-400 Linz, Austria b Herbert Raab, chönbergstr. 3/1, A-400 Linz, Austria; herbert.raab@utanet.at
More informationPHOTOELECTRIC EFFECT AND DUAL NATURE OF MATTER AND RADIATIONS
PHOTOELECTRIC EFFECT AND DUAL NATURE OF MATTER AND RADIATIONS 1. Photons 2. Photoelectric Effect 3. Experimental Set-up to study Photoelectric Effect 4. Effect of Intensity, Frequency, Potential on P.E.
More informationRaman Spectroscopy Basics
Raman Spectroscopy Basics Introduction Raman spectroscopy is a spectroscopic technique based on inelastic scattering of monochromatic light, usually from a laser source. Inelastic scattering means that
More informationComponents for Infrared Spectroscopy. Dispersive IR Spectroscopy
Components for Infrared Spectroscopy Mid-IR light: 00-000 cm - (5.5 m wavelength) Sources: Blackbody emitters Globar metal oxides Nernst Glower: Silicon Carbide Detectors: Not enough energy for photoelectric
More informationLight Telescopes. Grade Level: 5. 2-3 class periods (more if in-depth research occurs)
Light Telescopes Grade Level: 5 Time Required: Suggested TEKS: Science - 5.4 Suggested SCANS Information. Acquires and evaluates information. National Science and Math Standards Science as Inquiry, Earth
More informationAtomic and Nuclear Physics Laboratory (Physics 4780)
Gamma Ray Spectroscopy Week of September 27, 2010 Atomic and Nuclear Physics Laboratory (Physics 4780) The University of Toledo Instructor: Randy Ellingson Gamma Ray Production: Co 60 60 60 27Co28Ni *
More informationPreview of Period 3: Electromagnetic Waves Radiant Energy II
Preview of Period 3: Electromagnetic Waves Radiant Energy II 3.1 Radiant Energy from the Sun How is light reflected and transmitted? What is polarized light? 3.2 Energy Transfer with Radiant Energy How
More informationThe CCD Photometric Calibration
The CCD Photometric Calibration Cookbook Next: Abstract The CCD Photometric Calibration Cookbook Starlink Cookbook 6.2 J. Palmer & A.C. Davenhall 29th January 1998 CCLRC / Rutherford Appleton Laboratory
More informationLecture 14. Introduction to the Sun
Lecture 14 Introduction to the Sun ALMA discovers planets forming in a protoplanetary disc. Open Q: what physics do we learn about the Sun? 1. Energy - nuclear energy - magnetic energy 2. Radiation - continuum
More informationAn Introduction to the MTG-IRS Mission
An Introduction to the MTG-IRS Mission Stefano Gigli, EUMETSAT IRS-NWC Workshop, Eumetsat HQ, 25-0713 Summary 1. Products and Performance 2. Design Overview 3. L1 Data Organisation 2 Part 1 1. Products
More informationSpherical Beam Volume Holograms Recorded in Reflection Geometry for Diffuse Source Spectroscopy
Spherical Beam Volume Holograms Recorded in Reflection Geometry for Diffuse Source Spectroscopy Sundeep Jolly A Proposal Presented to the Academic Faculty in Partial Fulfillment of the Requirements for
More informationJorge E. Fernández Laboratory of Montecuccolino (DIENCA), Alma Mater Studiorum University of Bologna, via dei Colli, 16, 40136 Bologna, Italy
Information technology (IT) for teaching X- and gamma-ray transport: the computer codes MUPLOT and SHAPE, and the web site dedicated to photon transport Jorge E. Fernández Laboratory of Montecuccolino
More informationProblem Set 6 UV-Vis Absorption Spectroscopy. 13-1. Express the following absorbances in terms of percent transmittance:
Problem Set 6 UV-Vis Absorption Spectroscopy 13-1. Express the following absorbances in terms of percent transmittance: a 0.051 b 0.918 c 0.379 d 0.261 e 0.485 f 0.072 A = log P o /P = log1/t = - log T
More informationSpectroscopy. Biogeochemical Methods OCN 633. Rebecca Briggs
Spectroscopy Biogeochemical Methods OCN 633 Rebecca Briggs Definitions of Spectrometry Defined by the method used to prepare the sample 1. Optical spectrometry Elements are converted to gaseous atoms or
More informationTime out states and transitions
Time out states and transitions Spectroscopy transitions between energy states of a molecule excited by absorption or emission of a photon hn = DE = E i - E f Energy levels due to interactions between
More informationHigh Resolution Imaging in the Visible from the Ground without Adaptive Optics: New Techniques and Results
High Resolution Imaging in the Visible from the Ground without Adaptive Optics: New Techniques and Results Craig Mackay *a, John Baldwin b, Nicholas Law a and Peter Warner b a Institute of Astronomy and
More informationPreface Light Microscopy X-ray Diffraction Methods
Preface xi 1 Light Microscopy 1 1.1 Optical Principles 1 1.1.1 Image Formation 1 1.1.2 Resolution 3 1.1.3 Depth of Field 5 1.1.4 Aberrations 6 1.2 Instrumentation 8 1.2.1 Illumination System 9 1.2.2 Objective
More informationExperiment #5: Qualitative Absorption Spectroscopy
Experiment #5: Qualitative Absorption Spectroscopy One of the most important areas in the field of analytical chemistry is that of spectroscopy. In general terms, spectroscopy deals with the interactions
More informationSolar Activity and Earth's Climate
Rasmus E. Benestad Solar Activity and Earth's Climate Second Edition Published in association with Springer Praxis ids Publishing Publisl PRAXI Chichester, UK Contents Preface to the second edition Preface
More informationPHYSICS PAPER 1 (THEORY)
PHYSICS PAPER 1 (THEORY) (Three hours) (Candidates are allowed additional 15 minutes for only reading the paper. They must NOT start writing during this time.) ---------------------------------------------------------------------------------------------------------------------
More informationScience Standard 4 Earth in Space Grade Level Expectations
Science Standard 4 Earth in Space Grade Level Expectations Science Standard 4 Earth in Space Our Solar System is a collection of gravitationally interacting bodies that include Earth and the Moon. Universal
More informationPolarization Dependence in X-ray Spectroscopy and Scattering. S P Collins et al Diamond Light Source UK
Polarization Dependence in X-ray Spectroscopy and Scattering S P Collins et al Diamond Light Source UK Overview of talk 1. Experimental techniques at Diamond: why we care about x-ray polarization 2. How
More information(3) Interaction of high energy photons with matter
(3) Interaction of high energy photons with matter Photoelectric Absorption (Inverse) Compton Scattering Electron-positron pair production Application in Detectors 1 Photoelectric Absorption Similar to
More informationGünter Seeber. Satellite Geodesy 2nd completely revised and extended edition
Günter Seeber Satellite Geodesy 2nd completely revised and extended edition Walter de Gruyter Berlin New York 2003 Contents Preface Abbreviations vii xvii 1 Introduction 1 1.1 Subject of Satellite Geodesy...
More informationCSSAR Space Science Cooperation
CSSAR Space Science Cooperation WANG Shuzhi Center for Space Science and Applied Research Chinese Academy of Science(CSSAR) Table of Contents Brief History of CSSAR International Cooperation CAS Strategic
More informationCosmic Journey: Teacher Packet
Cosmic Journey: Teacher Packet Compiled by: Morehead State University Star Theatre with help from Bethany DeMoss Table of Contents Table of Contents 1 Corresponding Standards 2 Vocabulary 4 Sizing up the
More informationIntroduction. Stefano Ferrari. Università degli Studi di Milano stefano.ferrari@unimi.it. Elaborazione delle immagini (Image processing I)
Introduction Stefano Ferrari Università degli Studi di Milano stefano.ferrari@unimi.it Elaborazione delle immagini (Image processing I) academic year 2011 2012 Image processing Computer science concerns
More informationPowder diffraction and synchrotron radiation
Powder diffraction and synchrotron radiation Gilberto Artioli Dip. Geoscienze UNIPD CIRCe Center for Cement Materials single xl diffraction powder diffraction Ideal powder Powder averaging Textured sample
More informationMaster Degree Program
SAINT PETERSBURG STATE ELECTROTECHNICAL UNIVERSITY LETI Laser Measurement and Navigation Systems department Master Degree Program ETU LETI TRADITIONS AND INNOVATIONS ETU LETI is the oldest Electrotechnical
More informationScience and the Taiwan Airborne Telescope
Cosmic Variability Study in Taiwan Wen-Ping Chen Institute of Astronomy National Central University, Taiwan 2010 November 16@Jena/YETI Advantages in Taiwan: - Many high mountains - Western Pacific longitude
More informationCHAPTER 3: DIGITAL IMAGING IN DIAGNOSTIC RADIOLOGY. 3.1 Basic Concepts of Digital Imaging
Physics of Medical X-Ray Imaging (1) Chapter 3 CHAPTER 3: DIGITAL IMAGING IN DIAGNOSTIC RADIOLOGY 3.1 Basic Concepts of Digital Imaging Unlike conventional radiography that generates images on film through
More informationSpecifying Plasma Deposited Hard Coated Optical Thin Film Filters. Alluxa Engineering Staff
Specifying Plasma Deposited Hard Coated Optical Thin Film Filters. Alluxa Engineering Staff December 2012 Specifying Advanced Plasma Deposited Hard Coated Optical Bandpass and Dichroic Filters. Introduction
More informationD.S. Boyd School of Earth Sciences and Geography, Kingston University, U.K.
PHYSICAL BASIS OF REMOTE SENSING D.S. Boyd School of Earth Sciences and Geography, Kingston University, U.K. Keywords: Remote sensing, electromagnetic radiation, wavelengths, target, atmosphere, sensor,
More informationOptics and Spectroscopy at Surfaces and Interfaces
Vladimir G. Bordo and Horst-Gunter Rubahn Optics and Spectroscopy at Surfaces and Interfaces WILEY- VCH WILEY-VCH Verlag GmbH & Co. KGaA Contents Preface IX 1 Introduction 1 2 Surfaces and Interfaces 5
More informationOptical System Design
Optical System Design Robert E. Fischer CEO, OPTICS 1, Incorporated Biljana Tadic-Galeb Panavision Paul R. Yoder Consultant With contributions by Ranko Galeb Bernard C.Kress, Ph.D. Stephen C. McClain,
More information16 th IOCCG Committee annual meeting. Plymouth, UK 15 17 February 2011. mission: Present status and near future
16 th IOCCG Committee annual meeting Plymouth, UK 15 17 February 2011 The Meteor 3M Mt satellite mission: Present status and near future plans MISSION AIMS Satellites of the series METEOR M M are purposed
More informationNASA s Future Missions in X-ray Astronomy
NASA s Future Missions in X-ray Astronomy Nicholas E. White NASA s Goddard Space Flight Center Laboratory for High Energy Astrophysics Greenbelt, MD 20771 USA nwhite@lheapop.gsfc.nasa.gov Abstract The
More informationLight as a Wave. The Nature of Light. EM Radiation Spectrum. EM Radiation Spectrum. Electromagnetic Radiation
The Nature of Light Light and other forms of radiation carry information to us from distance astronomical objects Visible light is a subset of a huge spectrum of electromagnetic radiation Maxwell pioneered
More informationSolar Energy. Outline. Solar radiation. What is light?-- Electromagnetic Radiation. Light - Electromagnetic wave spectrum. Electromagnetic Radiation
Outline MAE 493R/593V- Renewable Energy Devices Solar Energy Electromagnetic wave Solar spectrum Solar global radiation Solar thermal energy Solar thermal collectors Solar thermal power plants Photovoltaics
More informationSTAAR Science Tutorial 30 TEK 8.8C: Electromagnetic Waves
Name: Teacher: Pd. Date: STAAR Science Tutorial 30 TEK 8.8C: Electromagnetic Waves TEK 8.8C: Explore how different wavelengths of the electromagnetic spectrum such as light and radio waves are used to
More informationALMA Newsletter. ALMA In-depth. How Will ALMA Make Images? April 2010
How Will ALMA Make Images? Credit: ALMA (ESO / NAOJ / NRAO), Cynthia Collao (ALMA). The invention of the optical telescope by Galileo 400 years ago marked the beginning of modern astronomy. Galileo used
More informationSpectral Measurement Solutions for Industry and Research
Spectral Measurement Solutions for Industry and Research Hamamatsu Photonics offers a comprehensive range of products for spectroscopic applications, covering the, Visible and Infrared regions for Industrial,
More informationStatus of the FERMI@Elettra Free Electron Laser
Status of the FERMI@Elettra Free Electron Laser E. Allaria on behalf of the FERMI team Work partially supported by the Italian Ministry of University and Research under grants FIRB-RBAP045JF2 and FIRB-RBAP06AWK3
More informationSmithsonian Astrophysical Observatory Contracts, 1961-1966
Smithsonian Astrophysical Observatory Contracts, 1961-1966 by Smithsonian Institution Archives Smithsonian Institution Archives Washington, D.C. Contact us at osiaref@si.edu http://siarchives.si.edu Table
More information07 - Cherenkov and transition radiation detectors
07 - Cherenkov and transition radiation detectors Jaroslav Adam Czech Technical University in Prague Version 1.0 Jaroslav Adam (CTU, Prague) DPD_07, Cherenkov and transition radiation Version 1.0 1 / 30
More informationIt has long been a goal to achieve higher spatial resolution in optical imaging and
Nano-optical Imaging using Scattering Scanning Near-field Optical Microscopy Fehmi Yasin, Advisor: Dr. Markus Raschke, Post-doc: Dr. Gregory Andreev, Graduate Student: Benjamin Pollard Department of Physics,
More informationSection 2.2. Contents of the Tycho Catalogue
Section 2.2 Contents of the Tycho Catalogue 141 2.2. Contents of the Tycho Catalogue Overview of the Tycho Catalogue: The Tycho Catalogue provides astrometry (positions, parallaxes and proper motions)
More informationEl programa de ciencias del espacio de la ESA
El programa de ciencias del espacio de la ESA Fabio Favata European Space Agency Astronomy and Fundamental Physics Missions Coordinator A broad mission portfolio A long-term commitment to the excellence
More informationEfficiency, Dispersion and Straylight Performance Tests of Immersed Gratings for High Resolution Spectroscopy in the Near Infra-red
Changing the economics of space Efficiency, Dispersion and Straylight Performance Tests of Immersed Gratings for High Resolution Spectroscopy in the Near Infra-red J. Fernandez-Saldivar 1, F. Culfaz 1,
More informationGREEN NANOTECHNOLOGY. Geoffrey. Energy in the Built Environment. Solutions for Sustainability and. B. Smith Claes G. Granqvist.
GREEN NANOTECHNOLOGY Solutions for Sustainability and Energy in the Built Environment Geoffrey B. Smith Claes G. Granqvist CRC Press Taylor & Francis Group Boca Raton London NewYork CRC Press is an imprint
More informationChapter 2: Forms of Energy
Chapter 2: Forms of Energy Goals of Period 2 Section 2.1: To describe the forms of energy Section 2.2: To illustrate conversions from one form of energy to another Section 2.3: To define the efficiency
More informationAre We Alone?! Exoplanet Characterization and Direct Imaging!
From Cosmic Birth to Living Earths A Vision for Space Astronomy in the 2020s and Beyond Are We Alone?! Exoplanet Characterization and Direct Imaging! A Study Commissioned by the Associated Universities
More informationSoftware challenges in the implementation of large surveys: the case of J-PAS
Software challenges in the implementation of large surveys: the case of J-PAS 1/21 Paulo Penteado - IAG/USP pp.penteado@gmail.com http://www.ppenteado.net/ast/pp_lsst_201204.pdf (K. Taylor) (A. Fernández-Soto)
More informationChapter 3 SYSTEM SCANNING HARDWARE OVERVIEW
Qiang Lu Chapter 3. System Scanning Hardware Overview 79 Chapter 3 SYSTEM SCANNING HARDWARE OVERVIEW Since all the image data need in this research were collected from the highly modified AS&E 101ZZ system,
More informationDevelopment of the Extreme Ultraviolet Spectrometer: EXCEED
Development of the Extreme Ultraviolet Spectrometer: EXCEED Go Murakami*, Kazuo Yoshioka, Atsushi Yamazaki, Tomoki Kimura Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency
More informationA down-under undergraduate optics and photonics laboratory
A down-under undergraduate optics and photonics laboratory Barry Perczuk and Michael Gal School of Physics, The University of New South Wales, Sydney, NSW 2052, Australia ABSTRACT Our senior undergraduate
More informationThe Future of Astronomy
The Future of Astronomy by Jesse Greenstein Jesse Greenstein, Lee A. DuBridge Professor of Astrophysics and staff member of the Hale Observatories and Owens Valley Radio Observatory, was chairman of the
More informationEarth Sciences -- Grades 9, 10, 11, and 12. California State Science Content Standards. Mobile Climate Science Labs
Earth Sciences -- Grades 9, 10, 11, and 12 California State Science Content Standards Covered in: Hands-on science labs, demonstrations, & activities. Investigation and Experimentation. Lesson Plans. Presented
More informationPhysical Therapy 602-523-4092
320 Physics and Astronomy PHI 351 Philosophy in Literature (3). Philosophical issues as expressed in the novel, drama, and poetry. Fall or Spring. PHI 352 Philosophy of Religion (3). Problems concerning
More informationSSO Transmission Grating Spectrograph (TGS) User s Guide
SSO Transmission Grating Spectrograph (TGS) User s Guide The Rigel TGS User s Guide available online explains how a transmission grating spectrograph (TGS) works and how efficient they are. Please refer
More informationAssessments of LEDs IESNA LM-79, LM-80 & LM-82
Assessments of LEDs IESNA LM-79, LM-80 & LM-82 by Rolf S. Bergman Consultant 4/30/2012 1 ALA M Outline of Presentation Background Information EPA Energy Star specifications NVLAP Accreditation IESNA Technical
More informationThe Sino-French Gamma-Ray Burst Mission SVOM (Space-based multi-band astronomical Variable Objects Monitor)
The Sino-French Gamma-Ray Burst Mission SVOM (Space-based multi-band astronomical Variable Objects Monitor) Didier BARRET on behalf of the SVOM collaboration didier.barret@cesr.fr Outline SVOM background
More informationSchlieren and Shadowgraph Techniques
G. S. Settles Schlieren and Shadowgraph Techniques Visualizing Phenomena in Transparent Media With 208 Figures and 48 Color Plates Springer Table of Contents List of Nomenclature, XV 1 Historical Background
More informationvii TABLE OF CONTENTS CHAPTER TITLE PAGE DECLARATION DEDICATION ACKNOWLEDGEMENT ABSTRACT ABSTRAK
vii TABLE OF CONTENTS CHAPTER TITLE PAGE DECLARATION DEDICATION ACKNOWLEDGEMENT ABSTRACT ABSTRAK TABLE OF CONTENTS LIST OF TABLES LIST OF FIGURES LIST OF SYMBOLS / ABBREVIATIONS LIST OF APPENDICES ii iii
More informationThe Bamberg photographic plate archive
The Bamberg photographic plate archive The digitizing project H. Edelmann, N. Jansen, U. Heber, H. Drechsel, J. Wilms, I. Kreykenbohm Dr. Karl Remeis-Observatory & ECAP Astronomical Institute Friedrich-Alexander-University
More informationOptical Modeling of the RIT-Yale Tip-Tilt Speckle Imager Plus
SIMG-503 Senior Research Optical Modeling of the RIT-Yale Tip-Tilt Speckle Imager Plus Thesis Kevin R. Beaulieu Advisor: Dr. Elliott Horch Chester F. Carlson Center for Imaging Science Rochester Institute
More informationScience Drivers for Big Data Joseph Lazio SKA Program Development Office & Jet Propulsion Laboratory, California Institute of Technology
Science Drivers for Big Data Joseph Lazio SKA Program Development Office & Jet Propulsion Laboratory, California Institute of Technology 2010 California Institute of Technology. Government sponsorship
More informationCopyright 1999 2010 by Mark Brandt, Ph.D. 12
Introduction to Absorbance Spectroscopy A single beam spectrophotometer is comprised of a light source, a monochromator, a sample holder, and a detector. An ideal instrument has a light source that emits
More informationBoardworks AS Physics
Boardworks AS Physics Vectors 24 slides 11 Flash activities Prefixes, scalars and vectors Guide to the SI unit prefixes of orders of magnitude Matching powers of ten to their SI unit prefixes Guide to
More informationGraduate Programs in Physics and Astronomy
Graduate Programs in Physics and Astronomy Western s award winning faculty members, cutting edge research and interdisciplinary environment give you the tools to engage your imagination. The University
More informationA PHOTOGRAMMETRIC APPRAOCH FOR AUTOMATIC TRAFFIC ASSESSMENT USING CONVENTIONAL CCTV CAMERA
A PHOTOGRAMMETRIC APPRAOCH FOR AUTOMATIC TRAFFIC ASSESSMENT USING CONVENTIONAL CCTV CAMERA N. Zarrinpanjeh a, F. Dadrassjavan b, H. Fattahi c * a Islamic Azad University of Qazvin - nzarrin@qiau.ac.ir
More informationFig.1. The DAWN spacecraft
Introduction Optical calibration of the DAWN framing cameras G. Abraham,G. Kovacs, B. Nagy Department of Mechatronics, Optics and Engineering Informatics Budapest University of Technology and Economics
More informationRAY TRACING UNIFIED FIELD TRACING
RAY TRACING Start to investigate the performance of your optical system using 3D ray distributions, dot diagrams of ray positions and directions, and optical path length. GEOMETRIC FIELD TRACING Switch
More informationAugust, 2000 LIGO-G000313-00-D. http://www.ligo.caltech.edu/~smarka/sn/
LIGO-G000313-00-D Proposal to the LSC for Entry of LIGO into the Supernova Nova Early Warning System (SNEWS) and Prototype Development of Real-Time LIGO Supernova Alert 1 Barry Barish, Kenneth Ganezer(CSUDH),
More informationCosmological Analysis of South Pole Telescope-detected Galaxy Clusters
Cosmological Analysis of South Pole Telescope-detected Galaxy Clusters March 24th Tijmen de Haan (McGill) - Moriond 2014 Photo credit: Keith Vanderlinde Outline The galaxy cluster sample Calibrating the
More informationA high accuracy, small field of view star guider with application to SNAP.
A high accuracy, small field of view star guider with application to SNAP. Aurélia Secroun and Michael Lampton Space Sciences Laboratory, U.C. Berkeley Michael Levi Lawrence Berkeley National Laboratory,
More informationR&D on CdTe pixel detectors J. Alvarez, J.L. Galvez, M. Hernanz, J. Isern
R&D on CdTe pixel detectors J. Alvarez, J.L. Galvez, M. Hernanz, J. Isern on behalf of a large collaboration with IMB(CNM-CSIC) and IFAE LOFT Large Observatory For x-ray Timing M. Hernanz, J. Alvarez,
More informationEdited by. C'unter. and David S. Moore. Gauglitz. Handbook of Spectroscopy. Second, Enlarged Edition. Volume 4. WlLEY-VCH. VerlagCmbH & Co.
Edited by C'unter Gauglitz and David S. Moore Handbook of Spectroscopy Second, Enlarged Edition Volume 4 WlLEY-VCH VerlagCmbH & Co. KGaA IX Volume 4 Section XII Applications 6: Spectroscopy at Surfaces
More informationA Preliminary Summary of The VLA Sky Survey
A Preliminary Summary of The VLA Sky Survey Eric J. Murphy and Stefi Baum (On behalf of the entire Science Survey Group) 1 Executive Summary After months of critical deliberation, the Survey Science Group
More informationHigh resolution images obtained with Solar Optical Telescope on Hinode. SOLAR-B Project Office National Astronomical Observatory of Japan (NAOJ)
High resolution images obtained with Solar Optical Telescope on Hinode SOLAR-B Project Office National Astronomical Observatory of Japan (NAOJ) Temperature stratification of solar atmosphere G-band Ca
More informationStudy of the Human Eye Working Principle: An impressive high angular resolution system with simple array detectors
Study of the Human Eye Working Principle: An impressive high angular resolution system with simple array detectors Diego Betancourt and Carlos del Río Antenna Group, Public University of Navarra, Campus
More informationThe Milky Way Galaxy is Heading for a Major Cosmic Collision
The Milky Way Galaxy is Heading for a Major Cosmic Collision Roeland van der Marel (STScI) [based on work with a team of collaborators reported in the Astrophysical Journal July 2012] Hubble Science Briefing
More information