Theory and Applications Laser Speckle Interferometry
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Aperture Mask Interferometry with an Integral Field Spectrograph
Aperture Mask Interferometry with an Integral Field Spectrograph Neil Zimmermana,b, Anand Sivaramakrishnanc,b,d, David Bernate, Ben R. Oppenheimerb, Sasha Hinkleyf,g, James P. Lloyde, Peter Tuthillh, Douglas Brennerb, Ian R. Parryi, Michal Simond, John E. Kristj, Laurent Pueyok,g a Max Planck Institute for Astronomy, K¨onigstuhl 17, 69117 Heidelberg, Germany, b Department of Astrophysics, American Museum of Natural History, 79th Street at CPW, New York, NY 10024, USA c Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA d Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794, USA e 230 Space Sciences Building, Cornell University, Ithaca, NY 14853, USA f California Institute of Technology, Pasadena, CA 91125, USA g Sagan Fellow h School of Physics, University of Sydney, NSW 2006, Australia i Institute of Astronomy, University of Cambridge, Cambridge CB3 OHA, UK j Jet Propulsion Laboratory, Pasadena, CA 91109, USA k Department of Physics & Astronomy, Johns Hopkins University, 366 Bloomberg Center, 3400 N. Charles Street, Baltimore, MD 21212, USA ABSTRACT A non-redundant pupil mask placed in front of a low-resolution integral field spectrograph (IFS) adds a spectral dimension to high angular resolution imaging behind adaptive optics systems. We demonstrate the first appli- cation of this technique, using the spectroscopic binary star system β CrB as our target. The mask and IFS combination enabled us to measure the first low-resolution spectrum of the F3–F5 dwarf secondary component of β CrB, at an angular separation 141 mas from its A5–A7Vp primary star. To record multi-wavelength closure phases, we collected interferograms simultaneously in 23 spectral channels spanning the J and H bands (1.1 µm–1.8 µm), using the Project 1640 IFS behind the 249-channel PalAO adaptive optics system on the Hale telescope at Palomar Observatory. -
Laser Speckle Imaging: a Quantitative Tool for Flow Analysis
LASER SPECKLE IMAGING: A QUANTITATIVE TOOL FOR FLOW ANALYSIS A Thesis presented to the Faculty of California Polytechnic State University, San Luis Obispo In Partial Fulfillment of the Requirements for the Degree Master of Science in Biomedical Engineering by Taylor Andrew Hinsdale June 2014 © 2014 Taylor Andrew Hinsdale ALL RIGHTS RESERVED ii COMMITTEE MEMBERSHIP TITLE: Laser Speckle Imaging: A Quantitative Tool for Flow Analysis AUTHOR: Taylor Andrew Hinsdale DATE SUBMITTED: June 2104 COMMITTEE CHAIR: Lily Laiho, PhD Associate Professor of Biomedical Engineering COMMITTEE MEMBER: David Clague, PhD Associate Professor of Biomedical Engineering COMMITTEE MEMBER: John Sharpe, PhD Professor of Physics iii ABSTRACT Laser Speckle Imaging: A Quantitative Tool for Flow Analysis Taylor Andrew Hinsdale Laser speckle imaging, often referred to as laser speckle contrast analysis (LASCA), has been sought after as a quasi-real-time, full-field, flow visualization method. It has been proven to be a valid and reliable qualitative method, but there has yet to be any definitive consensus on its ability to be used as a quantitative tool. The biggest impediment to the process of quantifying speckle measurements is the introduction of additional non dynamic speckle patterns from the surroundings. The dynamic speckle pattern under investigation is often obscured by noise caused by background static speckle patterns. One proposed solution to this problem is known as dynamic laser speckle imaging (dLSI). dLSI attempts to isolate the dynamic speckle signal from the previously mentioned background and provide a consistent dynamic measurement. This paper will investigate the use of this method over a range of experimental and simulated conditions. -
Industrial Applications of Speckle Techniques
TRITA-IIP-02-03 ISSN-1650-1888 Industrial Applications of Speckle Techniques -Measurement of Deformation and Shape Wei An Doctoral Thesis Chair of Industrial Metrology & Optics Department of Production Engineering Stockholm 2002 Royal Institute of Technology Industrial Applications of Speckle Techniques -Measurement of Deformation and Shape Wei An Doctoral Thesis TRITA-IIP-02-03 ISSN-1650-1888 Royal Institute of Technology Department of Production Engineering Chair of Industrial Metrology & Optics 100 44 Stockholm, Sweden 2002 TRITA-IIP-02-03 ISSN-1650-1888 Copyright © Wei An Department of Production Engineering Royal Institute of Technology S-100 44 Stockholm Sweden ABSTRACT Modern industry needs quick and reliable measurement methods for measuring deformation, position, shape, roughness, etc. This thesis is mainly concerned with industrial applications of speckle metrology. Speckle metrology is an optical non-contact whole field technique that provides the means to measure; deformation and displacement, object shape, surface roughness, vibration, and dynamic events, on rough surfaces and with a sensitivity of the order of a light wavelength. In particular, the electronic speckle metrology technique combined with advanced computers, fast frame grabbers, and image processing makes it very suitable for industrial applications. The thesis consists of four main parts. The first part presents the basic principle of speckle metrology. Some formulas and theoretical analysis are reviewed. The procedure of recording electronic speckle patterns is discussed. The phase shifting and the phase unwrapping techniques are also presented in this part. The second part considers some applications of speckle metrology technique. Four types of measurements have been done during this thesis period. They correspond to deformation measurements of solder joints on electronic device boards, 3D shape measurement with light-in-flight electronic speckle pattern interferometry, continuous deformation measurement, and cutting tool monitoring. -
An Investigation of Six Poorly Described Close Visual Double Stars Using Speckle Interferometry Daniel B
University of North Dakota UND Scholarly Commons Theses and Dissertations Theses, Dissertations, and Senior Projects January 2015 An Investigation Of Six Poorly Described Close Visual Double Stars Using Speckle Interferometry Daniel B. Wallace Follow this and additional works at: https://commons.und.edu/theses Recommended Citation Wallace, Daniel B., "An Investigation Of Six Poorly Described Close Visual Double Stars Using Speckle Interferometry" (2015). Theses and Dissertations. 1849. https://commons.und.edu/theses/1849 This Thesis is brought to you for free and open access by the Theses, Dissertations, and Senior Projects at UND Scholarly Commons. It has been accepted for inclusion in Theses and Dissertations by an authorized administrator of UND Scholarly Commons. For more information, please contact [email protected]. AN INVESTIGATION OF SIX POORLY DESCRIBED CLOSE VISUAL DOUBLE STARS USING SPECKLE INTERFEROMETRY by Daniel B. Wallace Bachelor of Science, East Stroudsburg University, 2008 A Thesis Submitted to the Graduate Faculty of the University of North Dakota in partial fulfillment of the requirements for the degree of Master of Science Grand Forks, North Dakota May 2015 This thesis, submitted by Daniel B. Wallace in partial fulfillment of the requirements for the Degree of Master of Science from the University of North Dakota, has been read by the Faculty Advisory Committee under whom the work has been done and is hereby approved. Dr. Paul S. Hardersen Dr. Russell M. Genet Dr. Kent Clark This thesis is being submitted by the appointed advisory committee as having met all of the requirements of the School of Graduate Studies at the University of North Dakota and is hereby approved. -
The Power Spectrum Extended Technique Applied to Images Of
The power spectrum extended technique applied to images of binary stars in the infrared Eric Aristidi, Eric Cottalorda, Marcel Carbillet, Lyu Abe, Karim Makki, Jean-Pierre Rivet, David Vernet, Philippe Bendjoya To cite this version: Eric Aristidi, Eric Cottalorda, Marcel Carbillet, Lyu Abe, Karim Makki, et al.. The power spectrum extended technique applied to images of binary stars in the infrared. Adaptive Optics Systems VII, Dec 2020, Online Only, France. pp.123, 10.1117/12.2560453. hal-03071661 HAL Id: hal-03071661 https://hal.archives-ouvertes.fr/hal-03071661 Submitted on 16 Dec 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. The power spectrum extended technique applied to images of binary stars in the infrared Eric Aristidia, Eric Cottalordaa,b, Marcel Carbilleta, Lyu Abea, Karim Makkic, Jean-Pierre Riveta, David Vernetd, and Philippe Bendjoyaa aUniversit´eC^oted'Azur, Observatoire de la C^oted'Azur, CNRS, laboratoire Lagrange, France bArianeGroup, 51/61 route de Verneuil - BP 71040, 78131 Les Mureaux Cedex, France cLaboratoire d'informatique et syst`emes,Aix-Marseille Universit´e,France dUniversit´eC^oted'Azur, Observatoire de la C^oted'Azur, France ABSTRACT We recently proposed a new lucky imaging technique, the Power Spectrum Extended (PSE), adapted for image reconstruction of short-exposure astronomical images in case of weak turbulence or partial adaptive optics cor- rection. -
Spatially Resolved Ultraviolet Spectroscopy of the Great Dimming
Draft version August 13, 2020 A Typeset using L TEX default style in AASTeX63 Spatially Resolved Ultraviolet Spectroscopy of the Great Dimming of Betelgeuse Andrea K. Dupree,1 Klaus G. Strassmeier,2 Lynn D. Matthews,3 Han Uitenbroek,4 Thomas Calderwood,5 Thomas Granzer,2 Edward F. Guinan,6 Reimar Leike,7 Miguel Montarges` ,8 Anita M. S. Richards,9 Richard Wasatonic,10 and Michael Weber2 1Center for Astrophysics | Harvard & Smithsonian, 60 Garden Street, MS-15, Cambridge, MA 02138, USA 2Leibniz-Institut f¨ur Astrophysik Potsdam (AIP), Germany 3Massachusetts Institute of Technology, Haystack Observatory, 99 Millstone Road, Westford, MA 01886 USA 4National Solar Observatory, Boulder, CO 80303 USA 5American Association of Variable Star Observers, 49 Bay State Road, Cambridge, MA 02138 6Astrophysics and Planetary Science Department, Villanova University, Villanova, PA 19085, USA 7Max Planck Institute for Astrophysics, Karl-Schwarzschildstrasse 1, 85748 Garching, Germany, and Ludwig-Maximilians-Universita`at, Geschwister-Scholl Platz 1,80539 Munich, Germany 8Institute of Astronomy, KU Leuven, Celestinenlaan 200D B2401, 3001 Leuven, Belgium 9Jodrell Bank Centre for Astrophysics, University of Manchester, M13 9PL, Manchester UK 10Astrophysics and Planetary Science Department, Villanova University, Villanova, PA 19085 USA (Received June 26, 2020; Revised July 9, 2020; Accepted July 10, 2020; Published August 13, 2020) Submitted to ApJ ABSTRACT The bright supergiant, Betelgeuse (Alpha Orionis, HD 39801) experienced a visual dimming during 2019 December and the first quarter of 2020 reaching an historic minimum 2020 February 7−13. Dur- ing 2019 September-November, prior to the optical dimming event, the photosphere was expanding. At the same time, spatially resolved ultraviolet spectra using the Hubble Space Telescope/Space Tele- scope Imaging Spectrograph revealed a substantial increase in the ultraviolet spectrum and Mg II line emission from the chromosphere over the southern hemisphere of the star. -
Double Star Research, Instrumentation, & Education
Double Star Research, Instrumentation, & Education Summer Seminar Projects Edited by Jacob Hass Double Star Research, Instrumentation, & Education: Summer Seminar Projects Editor: Jacob Hass Associate Editors: Meghan Legg, Hope Moseley, & Sabrina Smith 192 Contents Introduction: Cal Poly Summer 2015 Astronomy Research and Development Seminar 194 Russell Genet Albireo: 260 Years of Astrometric Observations 204 Jacob Hass, Kevin Phung, Joseph Carro, Emily Hock, Donald Loveland, Tristan Nibbe, Zoe Sharp, Jenny Smit, & Russell Genet Detecting Faint Secondary Stars with Shaped Aperture Masks 218 Donald Loveland, Edward Foley, Russell Genet, Neil Zimmerman, David Rowe, Richard Harshaw, & Jimmy Ray Intensifiers: A Low Cost Solution for Observing Faint Double Stars? 227 Jacob Hass, Kevin Phung, & Jenny Smit Newtonian 17.5-inch Optical Tube Assembly 232 Kevin Phung, Jacob Hass, Victor Chen, Kevin Thompson, and Russell Genet Thirteen Potential Short-Arc Binaries Observed at Kitt Peak National Observatory 238 Richard Harshaw, Russell Genet, Jacob Hass, and Kevin Phung Being a Scientist While Teaching Science: Implementing Undergraduate Research Opportunities for Elementary Educators 253 Emily Hock and Zoë Sharp Incorporating Remote Robotic Telescopes into an Elementary Classroom Setting 258 Zoë Sharp and Emily Hock Mt Wilson 100-inch Speckle Interferometry Engineering Checkout 263 Russell M. Genet, David Rowe, Thomas Meneghini, Robert Buchheim, Reed Estrada, Chris Estrada, Pat Boyce, Grady Boyce, John Ridgely, Niels Smidth, Richard Harshaw, & John -
Speckle Imaging with VLT/NACO No-AO Mode
Telescopes and Instrumentation Speckle Imaging with VLT/NACO No-AO Mode Sridharan Rengaswamy1 object of interest. In the case of binary Holographic imaging of crowded fields Julien Girard1 stars, the binary nature can be visually was pioneered and presented by Rainer Willem-Jan de Wit1 identified from the peaks of the auto- Schödel (Schödel & Girard, 2012; Henri Boffin1 correlation. Schödel et al., 2013). Here we demon- strate how the NACO non-AO mode, Speckle interferometry has made signifi- coupled with the aforementioned speckle 1 ESO cant contributions to the field of binary image pro cessing technique, can be star research by creating several binary exploited to obtain near diffraction-limited star catalogues (e.g., Mason et al., 2013). images of objects of interest. We have Long-exposure stellar images recorded Since the energy spectrum does not developed the required pipeline data with large ground-based telescopes preserve the Fourier phase information, it reduction tool (Rengaswamy, Girard & are blurred due to the turbulent nature is not possible to obtain an image of the Montagnier, 2010) for reconstructing an of the atmosphere. The VLT employs object apart from the autocorrelation. image from the speckle data1. active and adaptive optics (AO) systems Hence there is a 180-degree ambiguity in to compensate for the deleterious the position angle of the binary star. In effects of the atmosphere in real time. 1977, Gerd Weigelt showed, experimen- Imaging binary stars The speckle imaging technique provides tally, that the phase of the complex triple an alternative way to achieve diffrac- product of the Fourier transform of the The study of binary stars is an important tion-limited imaging by post-processing images at three spatial frequencies (the branch of astrophysics. -
Speckle Interferometry with a Low Read-Noise CMOS Video Camera
Vol. 12 No. 3 Journal of Double Star Observations | March 2016 Ashcraft Speckle Interferometry with a Low Read-Noise CMOS Video Camera Clif Ashcraft Perrineville Observatory Abstract This paper demonstrates that speckle interferometry of close double stars (Rho < 1ʺ) can be done with a small (11 inch aperture) telescope equipped with a sensitive, low noise, and low read-noise CMOS camera. Introduction For the past several years I have not been active in double star observations while I became quite involved with high resolution planetary imaging. In the early years we did this with ordinary webcams like the Philips ToUcam, but more recently we began to use what I call “industrial strength” webcams: cameras developed by firms like The Imaging Source and Point Gray for machine vision and surveillance applications, but inexpensive enough for amateurs to afford and quite suitable for high resolution planetary work. For this we employed the so-called “lucky imaging” approach of aligning and stacking the best frames from videos taken at focal ratios long enough for Nyquist sampling of the planetary images. This area of amateur involvement has progressed rapidly to the point that we can now routinely take images of the Moon, Mars, Jupiter, and Saturn that not too many years ago took a NASA mission to obtain. For much of this period the cameras we used were based on mature CCD technology, but in recent years, cameras based upon sensitive, low noise CMOS sensors have become available, notably, the ASI series of cameras from ZWO. The amateur planetary imaging community immediately began to use them. -
Lucky Imaging: Beyond Binary Stars
LUCKY IMAGING: BEYOND BINARY STARS Thesis submitted for the degree of Doctor of Philosophy by Tim Staley Institute of Astronomy & Emmanuel College arXiv:1404.5907v1 [astro-ph.IM] 23 Apr 2014 University of Cambridge January 21, 2013 DECLARATION I hereby declare that this dissertation entitled Lucky Imaging: Beyond Binary Stars is not substantially the same as any that I have submitted for a degree or diploma or other qualification at any other University. I further state that no part of my thesis has already been or is being concurrently submitted for any such degree, diploma or other qualification. This dissertation is the result of my own work and includes nothing which is the outcome of work done in collaboration except where specifically indicated in the text. I note that chapter 1 and the first few sections of chapter 6 are intended as reviews, and as such contain little, if any, original work. They contain a number of images and plots extracted from other published works, all of which are clearly cited in the appropriate caption. Those parts of this thesis which have been published are as follows: • Chapters 3 and 4 contain elements that were published in Staley and Mackay (2010). However, the work has been considerably expanded upon for this document. • The planetary transit host binarity survey described in chapter 5 is soon to be submitted for publi- cation. This dissertation contains fewer than 60,000 words. Tim Staley Cambridge, January 21, 2013 iii ACKNOWLEDGEMENTS 1 2 This thesis has been typeset in LATEX using Kile and JabRef. Thanks to all the former IoA members who have contributed to the LaTeX template used to constrain the formatting. -
Four Shows for Fulldome from the Giant Screen Solar Storms Available in 2D and 3D Stereo
Vol. 40, No. 4 December 2011 Journal of the International Planetarium Society Chinese Art in the Sky: A Journey into the Unknown Page 14 Articles December 2011 Vol. 40 No. 4 8 Eise Eisinga: He reched for the starry heavens and gave the world a planetarium Executive Editor heavens and gave the world a planetarium Sharon Shanks Chris Janssen Ward Beecher Planetarium 14 Chinese Art in the Sky: A Journey into the Unknown Youngstown State University Mark J. Percey Mark J. Percy One University Plaza 18 What else can it be but LIPS? Karrie BerglunBerglungd Youngstown, Ohio 44555 USA 22 A payment in planetariums Alex Cherman +1 330-941-3619 22 A payment in planetariums Alex Cherman [email protected] 24 How we do it: Simple scheduling Adam Thanz 28 Under one Dome: Sir Thomas Brisbane Planetarium Advertising Coordinator Mark Rigby Dr. Dale Smith, Interim Coordinator 3036 IntegratingA Park for the reading Dark with the planetarium (See Publications Committee on page 3) 56 American planetarian in Italy also finds hisJohn roots C. Scala Joseph E. Ciotti Membership 38 A Park for the Dark Individual: $65 one year; $100 two years 58 American planetarian in Italy also finds his roots Institutional: $250 first year; $125 annual renewal Joseph E. Ciotti Library Subscriptions: $45 one year; $80 two years Columns All amounts in US currency 60 Book Reviews ...................................April S. Whitt Direct membership requests and changes of 65 Calendar of Events ..............................Loris Ramponi address to the Treasurer/Membership Chairman 35 Educational Horizons .........................Columns Jack L. Northrup 462 InBook Front Reviews of the .................................. -
Laser Speckle Photometry – Optical Sensor Systems for Condi- Tion and Process Monitoring
MATERIALS TESTING FOR JOINING AND ADDITIVE MANUFACTURING APPLICATIONS 213 Laser speckle photometry – Optical sensor systems for condi- tion and process monitoring Lili Chen, Ulana Cikalova, Beatrice Bendjus, Laser speckle photometry (LSP) is an innovative, non-destruc- Andreas Gommlich, Shohag Roy Sudip, tive monitoring technique based on the detection and analy- Carolin Schott, Juliane Steingroewer, Dresden, sis of thermally or mechanically activated speckle dynamics Matthias Belting, Aachen, and in a non-stationary optical field. With the development of Stefan Kleszczynski, Duisburg, Germany speckle theories, it has been found that speckle patterns carry information about surface characteristics. Therefore, LSP offers a great potential for the characterization of mate- rial properties and monitoring of manufacturing processes. In contrast to the speckle interferometry method, LSP is very simple and robust. The sample is illuminated by only one la- ser beam to generate a speckle pattern on the surface. The Article Information signals obtained are directly recorded by a CCD or CMOS Correspondence Address Dr.-Ing. Beatrice Bendjus camera. By appropriate optical solutions for the beam path, Fraunhofer Institute for Ceramic typically, resolutions of less than 10 μm are reached if larger Technologies and Systems IKTS Maria-Reiche-Str. 2 areas are illuminated. LSP is definitely a contactless, quick 01109 Dresden, Germany and quality relevant material characterization and defect de- E-mail: [email protected] tection method, allowing process monitoring in many indus- Keywords trial fields. Examples from online biotechnological monitoring Laser speckle photometry, process-monitoring, defect-monitoring, build-up welding, additive and laser based manufacturing demonstrate further poten- manufacturing, biomass tials of the method for process monitoring and controlling.