Holography 1 HOLOGRAPHY Introduction and Background The
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Comparison Between Digital Fresnel Holography and Digital Image-Plane Holography: the Role of the Imaging Aperture M
Comparison between Digital Fresnel Holography and Digital Image-Plane Holography: The Role of the Imaging Aperture M. Karray, Pierre Slangen, Pascal Picart To cite this version: M. Karray, Pierre Slangen, Pascal Picart. Comparison between Digital Fresnel Holography and Digital Image-Plane Holography: The Role of the Imaging Aperture. Experimental Mechanics, Society for Experimental Mechanics, 2012, 52 (9), pp.1275-1286. 10.1007/s11340-012-9604-6. hal-02012133 HAL Id: hal-02012133 https://hal.archives-ouvertes.fr/hal-02012133 Submitted on 26 Feb 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. Comparison between Digital Fresnel Holography and Digital Image-Plane Holography: The Role of the Imaging Aperture M. Karray & P. Slangen & P. Picart Abstract Optical techniques are now broadly used in the experimental analysis. Particularly, a theoretical analysis field of experimental mechanics. The main advantages are of the influence of the aperture and lens in the case of they are non intrusive and no contact. Moreover optical image-plane holography is proposed. Optimal filtering techniques lead to full spatial resolution displacement maps and image recovering conditions are thus established. enabling the computing of mechanical value also in high Experimental results show the appropriateness of the spatial resolution. -
Digital Holography Using a Laser Pointer and Consumer Digital Camera Report Date: June 22Nd, 2004
Digital Holography using a Laser Pointer and Consumer Digital Camera Report date: June 22nd, 2004 by David Garber, M.E. undergraduate, Johns Hopkins University, [email protected] Available online at http://pegasus.me.jhu.edu/~lefd/shc/LPholo/lphindex.htm Acknowledgements Faculty sponsor: Prof. Joseph Katz, [email protected] Project idea and direction: Dr. Edwin Malkiel, [email protected] Digital holography reconstruction: Jian Sheng, [email protected] Abstract The point of this project was to examine the feasibility of low-cost holography. Can viable holograms be recorded using an ordinary diode laser pointer and a consumer digital camera? How much does it cost? What are the major difficulties? I set up an in-line holographic system and recorded both still images and movies using a $600 Fujifilm Finepix S602Z digital camera and a $10 laser pointer by Lazerpro. Reconstruction of the stills shows clearly that successful holograms can be created with a low-cost optical setup. The movies did not reconstruct, due to compression and very low image resolution. Garber 2 Theoretical Background What is a hologram? The Merriam-Webster dictionary defines a hologram as, “a three-dimensional image reproduced from a pattern of interference produced by a split coherent beam of radiation (as a laser).” Holograms can produce a three-dimensional image, but it is more helpful for our purposes to think of a hologram as a photograph that can be refocused at any depth. So while a photograph taken of two people standing far apart would have one in focus and one blurry, a hologram taken of the same scene could be reconstructed to bring either person into focus. -
The Image of Truth: Photographic Evidence and the Power of Analogy
Articles The Image of Truth: Photographic Evidence and the Power of Analogy Jennifer L. Mnookin* We have but Faith: We cannot know For Knowledge is of things we see. Alfred Tennyson, In Memoriam' Maxims that urge the power of images are cultural commonplaces with which we are all too familiar: "a picture's worth a thousand words," "seeing is believing," and so forth.2 The photograph, in * Doctoral Fellow, American Bar Foundation. For useful comments and suggestions, particular thanks are due to Shari Diamond, Joshua Dienstag, Bob Gordon, Evelyn Fox Keller, Jim Liebman, Bob Mnookin, Stephen Robertson, Richard Ross, Christopher Tomlins, and the participants of the Chicago Legal History Forum and the Northwestern History and Philosophy of Science Seminar Series. Thanks, too, for the many thoughtful suggestions of the editors of the Yale Journal of Law & the Humanities, especially Barton Beebe, Jacob Cogan, and Beth Hillman. For research support during the course of working on this article, I thank the American Bar Foundation. 1. ALFRED TENNYSON, In Memoriam, in TENNYSON'S POETRY 119, 120 (Robert W. Hill, Jr. ed., 1971). 2. Some research lends credence to these adages. See, e.g., Brad E. Bell & Elizabeth F. Loftus, Vivid Persuasion in the Courtroom, 49 J. PERSONALITY ASSESSMENT 659 (1985) (claiming that "vivid" testimony is more persuasive than "pallid" testimony); William C. Cos- topoulos, Persuasion in the Courtroom, 10 DuO. L. REv. 384, 406 (1972) (suggesting that more Yale Journal of Law & the Humanities, Vol. 10, Iss. 1 [1998], Art. 1 Yale Journal of Law & the Humanities [Vol. 10: 1 particular, has long been perceived to have a special power of persuasion, grounded both in the lifelike quality of its depictions and in its claim to mechanical objectivity.3 Seeing a photograph almost functions as a substitute for seeing the real thing. -
Scanning Camera for Continuous-Wave Acoustic Holography
Scanning Camera for Continuous-Wave Acoustic Holography Hillary W. Gao, Kimberly I. Mishra, Annemarie Winters, Sidney Wolin, and David G. Griera) Department of Physics and Center for Soft Matter Research, New York University, New York, NY 10003, USA (Dated: 7 August 2018) 1 We present a system for measuring the amplitude and phase profiles of the pressure 2 field of a harmonic acoustic wave with the goal of reconstructing the volumetric sound 3 field. Unlike optical holograms that cannot be reconstructed exactly because of the 4 inverse problem, acoustic holograms are completely specified in the recording plane. 5 We demonstrate volumetric reconstructions of simple arrangements of objects using 6 the Rayleigh-Sommerfeld diffraction integral, and introduce a technique to analyze 7 the dynamic properties of insonated objects. a)[email protected] 1 Scanning Holographic Camera 8 Most technologies for acoustic imaging use the temporal and spectral characteristics of 1 9 acoustic pulses to map interfaces between distinct phases. This is the basis for sonar , and 2 10 medical and industrial ultrasonography . Imaging continuous-wave sound fields is useful for 3 11 industrial and environmental noise analysis, particularly for source localization . Substan- 12 tially less attention has been paid to visualizing the amplitude and phase profiles of sound 13 fields for their own sakes, with most effort being focused on visualizing the near-field acous- 14 tic radiation emitted by localized sources, a technique known as near-field acoustic holog- 4{6 15 raphy (NAH) . The advent of acoustic manipulation in holographically structured sound 7{11 16 fields creates a need for effective sound-field visualization. -
Digital Refocusing with Incoherent Holography
Digital Refocusing with Incoherent Holography Oliver Cossairt Nathan Matsuda Northwestern University Northwestern University Evanston, IL Evanston, IL [email protected] [email protected] Mohit Gupta Columbia University New York, NY [email protected] Abstract ‘adding’ and ‘subtracting’ blur to the point spread functions (PSF) of different scene points, depending on their depth. In Light field cameras allow us to digitally refocus a pho- a conventional 2D image, while it is possible to add blur to tograph after the time of capture. However, recording a a scene point’s PSF, it is not possible to subtract or remove light field requires either a significant loss in spatial res- blur without introducing artifacts in the image. This is be- olution [10, 20, 9] or a large number of images to be cap- cause 2D imaging is an inherently lossy process; the angular tured [11]. In this paper, we propose incoherent hologra- information in the 4D light field is lost in a 2D image. Thus, phy for digital refocusing without loss of spatial resolution typically, if digital refocusing is desired, 4D light fields are from only 3 captured images. The main idea is to cap- captured. Unfortunately, light field cameras sacrifice spa- ture 2D coherent holograms of the scene instead of the 4D tial resolution in order to capture the angular information. light fields. The key properties of coherent light propagation The loss in resolution can be significant, up to 1-2 orders are that the coherent spread function (hologram of a single of magnitude. While there have been attempts to improve point source) encodes scene depths and has a broadband resolution by using compressive sensing techniques [14], spatial frequency response. -
Digitizing the Harvard Observatory Plate Collection
Digitizing the Harvard Observatory Plate Collection Scanning the “Historic Sky” Our Goals: Find Funding to Construct a Scanner and Digitize the Harvard Astronomical Photographic Plate Collection. Make the results available in Online Storage. Jonathan E. Grindlay – Harvard Professor of Astronomy Elizabeth Griffin – WG Chair IAU Digitization and Preservation Alison Doane – Acting Curator of the Harvard Plate Stack Douglas J. Mink - Software and Data Archivist Bob Simcoe – Volunteer Associate & System designer Before photography, astronomers’ eyes were their only sensing device and hand drawing was the means of permanent recording. This severely limited the science they could accomplish. rjs Astronomy, as a science, made quantum leaps forward with the advent of photography. For the first time permanent, measurable photographic records made possible “offline” analysis of data. rjs The first daguerreotype of the moon was made by American physiologist J.W. Draper in 1840, involving a full 20 minute exposure. The first star was not recorded until 1850, when director of Harvard Observatory, W.C. Bond and Boston photographer J.A. Whipple, took a daguerreotype of Vega. The first photographic sky surveys were done at Harvard during the period of 1882-1886. Each photograph covered 15 degree squares of sky and recorded stars as faint as 8th magnitude. rjs The world’s collection of astronomical photographic images (estimated at 2 million glass plates) represents the costly output of over a century of devotion and skill by myriad astronomers. Harvard Observatory now has 500,000+ photographs, by far the largest collection and 25% of the world’s total. Harvard’s plates contain the most complete sky coverage of both the northern and southern sky over the longest time period – 1880 to 1989 rjs Since the 1980’s, astronomers have largely abandoned the use of photography. -
Imaging and Imaging Detectors
4–1 Imaging and Imaging Detectors 4–2 Introduction Detectors we have dealt with so far: non-imaging detectors. This lecture: imaging optical photons and X-rays Any imaging system has two parts: 1. Imaging optics In most applications, mirrors are used for imaging, although other techniques (variants of shadow cameras) are used, e.g., for γ-rays 2. Spatially resolved detector i.e., a detector capable of measuring where a photon hits it in the focal plane. This can be a photographic plate or film, but is normally a charge coupled device (CCD). Introduction 1 4–3 Optical Imaging, I Cassegrain telescope, after Wikipedia Reminder: Optical telescopes are usually reflectors: primary mirror secondary mirror detector → → Main characteristics of a telescope: collecting area (i.e., open area of telescope, πd2/4, where d: telescope diameter) • ∼ fpr small telescopes: angular resolution, • λ θ = 1.22 (4.1) d but do not forget the seeing! Imaging 1 4–4 Optical Imaging, II Optical telescopes are based on principle that reflection “just works” with metallic surfaces. For X-rays, things are more complicated... Snell’s law of refraction: sin α n α1 n2 1 1 = = n (4.2) sin α2 n1 θ where n index of refraction, and α1,2 angle wrt. 1 surface normal. If n 1: Total internal reflection Total reflection occurs for α2 = 90◦, i.e. for n < n α 2 1 sin α1,c = n cos θc = n (4.3) 2 ⇐⇒ with the critical angle θ = π/2 α . c − 1,c Clearly, total reflection is only possible for n< 1 Light in glass at glass/air interface: n = 1/1.6 = θc 50◦ = principle behind optical fibers. -
State-Of-The-Art in Holography and Auto-Stereoscopic Displays
State-of-the-art in holography and auto-stereoscopic displays Daniel Jönsson <Ersätt med egen bild> 2019-05-13 Contents Introduction .................................................................................................................................................. 3 Auto-stereoscopic displays ........................................................................................................................... 5 Two-View Autostereoscopic Displays ....................................................................................................... 5 Multi-view Autostereoscopic Displays ...................................................................................................... 7 Light Field Displays .................................................................................................................................. 10 Market ......................................................................................................................................................... 14 Display panels ......................................................................................................................................... 14 AR ............................................................................................................................................................ 14 Application Fields ........................................................................................................................................ 15 Companies ................................................................................................................................................. -
Full-Color See-Through Three-Dimensional Display Method Based on Volume Holography
sensors Article Full-Color See-Through Three-Dimensional Display Method Based on Volume Holography Taihui Wu 1,2 , Jianshe Ma 2, Chengchen Wang 1,2, Haibei Wang 2 and Ping Su 2,* 1 Department of Precision Instrument, Tsinghua University, Beijing 100084, China; [email protected] (T.W.); [email protected] (C.W.) 2 Tsinghua Shenzhen International Graduate School, Tsinghua University, Shenzhen 518055, China; [email protected] (J.M.); [email protected] (H.W.) * Correspondence: [email protected] Abstract: We propose a full-color see-through three-dimensional (3D) display method based on volume holography. This method is based on real object interference, avoiding the device limitation of spatial light modulator (SLM). The volume holography has a slim and compact structure, which realizes 3D display through one single layer of photopolymer. We analyzed the recording mechanism of volume holographic gratings, diffraction characteristics, and influencing factors of refractive index modulation through Kogelnik’s coupled-wave theory and the monomer diffusion model of photopolymer. We built a multiplexing full-color reflective volume holographic recording optical system and conducted simultaneous exposure experiment. Under the illumination of white light, full-color 3D image can be reconstructed. Experimental results show that the average diffraction efficiency is about 53%, and the grating fringe pitch is less than 0.3 µm. The reconstructed image of volume holography has high diffraction efficiency, high resolution, strong stereo perception, and large observing angle, which provides a technical reference for augmented reality. Citation: Wu, T.; Ma, J.; Wang, C.; Keywords: holographic display; volume holography; photopolymer; augmented reality Wang, H.; Su, P. -
3D-Integrated Metasurfaces for Full-Colour Holography Yueqiang Hu 1, Xuhao Luo1, Yiqin Chen1, Qing Liu1,Xinli1,Yasiwang1,Naliu2 and Huigao Duan1
Hu et al. Light: Science & Applications (2019) 8:86 Official journal of the CIOMP 2047-7538 https://doi.org/10.1038/s41377-019-0198-y www.nature.com/lsa ARTICLE Open Access 3D-Integrated metasurfaces for full-colour holography Yueqiang Hu 1, Xuhao Luo1, Yiqin Chen1, Qing Liu1,XinLi1,YasiWang1,NaLiu2 and Huigao Duan1 Abstract Metasurfaces enable the design of optical elements by engineering the wavefront of light at the subwavelength scale. Due to their ultrathin and compact characteristics, metasurfaces possess great potential to integrate multiple functions in optoelectronic systems for optical device miniaturisation. However, current research based on multiplexing in the 2D plane has not fully utilised the capabilities of metasurfaces for multi-tasking applications. Here, we demonstrate a 3D-integrated metasurface device by stacking a hologram metasurface on a monolithic Fabry–Pérot cavity-based colour filter microarray to simultaneously achieve low-crosstalk, polarisation-independent, high-efficiency, full-colour holography, and microprint. The dual functions of the device outline a novel scheme for data recording, security encryption, colour displays, and information processing. Our 3D integration concept can be extended to achieve multi-tasking flat optical systems by including a variety of functional metasurface layers, such as polarizers, metalenses, and others. Introduction dimensional (3D) integration of discrete metasurfaces. For 1234567890():,; 1234567890():,; 1234567890():,; 1234567890():,; Metasurfaces open a new paradigm to design optical example, anisotropic structures or interleaved subarrays elements by shaping the wavefront of electromagnetic have been specifically arranged in a 2D plane to obtain – waves by tailoring the size, shape, and arrangement of multiplexed devices10,16 18. To reduce crosstalk, plas- – subwavelength structures1 3. -
Some Applications of Natural Color Photography in Mineralogy B
SOME APPLICATIONS OF NATURAL COLOR PHOTOGRAPHY IN MINERALOGY B. M. Snaus, Smith College,Northampton, Massachusetts. The use of natural color photographs or color transparenciesl in mineralogy and petrography is still in the initial stage of application, although hand-colored lantern slides have, for a long time, been em- ployed by teachers and lecturers on these subjects. During the past decade improvements have been made in the art of color photography, and at present there are several good color plates on the market. These are known as screenplates. In one type the color elements,red, green and blue-violet, are incorporated in an irregular mosaic forming a color screen, which is placed between the glass plate or film and the photo- graphic emulsion. In another type the color screen involves a separate plate consisting of a regular pattern of square or other ruled elements having the same colors in a gelatin coating. The former is known as a combination screenplate, or film, of which the Lumiere Autochrome film and the Agfa color plate are examples; the latter are referred to as sepa- rate screen plates, and the well known Finlay color plate is the out- standing example. The production of a positive picture on a combination plate involves a comparatively simple reversing process,during the finishing operations. With the separate screen plate a negative is made on a separate pan- chromatic plate which is exposed while pressedin contact, emulsion to t'taking emulsion, with a color screen known as the screen." The glass side of the latter is held towards the lens. -
Ccd Cameras for Cosmology
CCD CAMERAS FOR COSMOLOGY From images to cosmological parameters PAU Academic training Eusebio Sánchez Álvaro December 2007 CIEMAT (Madrid) Outline Introduction CCDs Properties of CCDs CCD types Sources of Noise Steps to reduce data CCDs .vs. Photographic plates Cameras Examples of cameras Diagram of a camera Other aspects PAU Academic training Eusebio Sánchez Álvaro December 2007 CIEMAT (Madrid) Introduction: Cosmology New Standard model of Cosmology Dark Matter Dark Energy To study cosmological parameters a large sky area a lot of objects are needed SURVEYS PAU Academic training Eusebio Sánchez Álvaro December 2007 CIEMAT (Madrid) From CCDs to cosmology We are interested in how we go from CCD-images to cosmology What is needed to obtain scientific results: The Source Atmosphere: seeing, … Telescope + optics: PSF… Camera + electronics + DaQ: This is what we talk about today Pipeline Analysis PAU Academic training Eusebio Sánchez Álvaro December 2007 CIEMAT (Madrid) From CCDs to Cosmology 3 main steps: (1) “Low-level” processing: • Bias removal (offset of charge in each pixel) • Flat-fielding • Fringe subtraction • Identification of cosmic-rays and satellites • Sky background subtraction (2) “Higher-Level” processing • Detection of objects (stars, galaxies, other…) • Astrometry (link between pixel coordinate and position on the sky) • Calibration (link between numbers in the image and photons from the source) (3) Analysis • Photometry, morphology, cosmology This talk is about (1), Alberto´s talks will be mainly about (2) and Licia´s