Visual Vibration Analysis
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Photographing Black Holes with the Event Horizon Telescope - Past, Present and Future
Photographing Black Holes with the Event Horizon Telescope - Past, Present and Future - Kazu Akiyama MIT Haystack Observatory The Shadow of a Black Hole BH ~5.2 Rs Rs = 2GMBH/c2 (Hilbert 1916) Credit: Hung-Yi Pu Kazu Akiyama, NEROC Symposium 2020, Online, 2020/11/17 (Tue) Event Horizon Telescope Kazu Akiyama, NEROC Symposium 2020, Online, 2020/11/17 (Tue) Event Horizon Telescope Sgr A* EHT 50μas Credit: Hotaka Shiokawa M87 EHT 40μas Credit: Monika Moscibrodzka Kazu Akiyama, NEROC Symposium 2020, Online, 2020/11/17 (Tue) Units of the Angular Size Protractor:1 ticks = 1 degree x 1/60 = 1 arcmin x 1/60 = 1 arcsec x 1/1000 = 1 mas x 1/1000 = 1 μas 0.5 deg 30 arcmin 40 - 50 μas Kazu Akiyama, NEROC Symposium 2020, Online, 2020/11/17 (Tue) Event Horizon Telescope Collaboration >300 members, >59 institutes, >18 countries in North & South America, Europe, Asia, and Africa. Kazu Akiyama, NEROC Symposium 2020, Online, 2020/11/17 (Tue) Meet the Telescope SMT, Arizona LMT, Mexico IRAM 30m Spain APEX, Chile JCMT, Hawaii Photos: ALMA, Sven Dornbusch, Junhan Kim, Helge Rottmann, David Sanchez, Daniel Michalik, Jonathan Weintroub, William Montgomerie Meet the Telescope Photos: ALMA, Sven ALMA, Chile Dornbusch, Junhan Kim, Helge Rottmann, David Sanchez, Daniel Michalik, Jonathan Weintroub, William Montgomerie SPT, South Pole SMA, Hawaii From Observations to Images Kazu Akiyama, NEROC Symposium 2020, Online, 2020/11/17 (Tue) Credit: Lindy Blackburn EHT Hardware EHT Backend (R2DBE, Mark 6) Recording Rate: - VLBA, GMVA: 2-4 Gbps - EHT: 32 Gbps (2017), 64 Gbps (2018-) Kazu Akiyama, NEROC Symposium 2020, Online, 2020/11/17 (Tue) From Observations to Images MIT Haystack Observatory 8 TB x 8 HDD (x 92 modules) Credit: Bryce Vickmark Credit: Lindy Blackburn Kazu Akiyama, NEROC Symposium 2020, Online, 2020/11/17 (Tue) Data Calibration HOPS Pipeline (EHT-HOPS) CASA Pipeline (rPICARD) EHT AIPS Pipeline Blackburn et al. -
Survey of Noise in Image and Efficient Technique for Noise Reduction
International Journal of Science and Research (IJSR) ISSN (Online): 2319-7064 Index Copernicus Value (2015): 78.96 | Impact Factor (2015): 6.391 Survey of Noise in Image and Efficient Technique for Noise Reduction Arti Singh1, Madhu2 1, 2Research Scholar, Computer Science, BBAU University, Lucknow , Uttar Pradesh, India Abstract: Removing noise from the image is big challenge for researcher because removal of noise in image causes the artifacts and image blurring. Noise occurred in image during the time of capturing and transmission of the image. There are many methods for noise removal from the images. Many algorithms and techniques are available for removing noise from image, but each method exist their own assumptions, merits and demerits. Noise reduction algorithms for remove noise is totally depends on what type of noise occur in the image. In this paper, focus on some important type of noise and noise removal techniques is done. Keywords: Impulse noise, Gaussian noise , Speckle noise ,Poisson noise, mean filter, median filter ,etc 1. Introduction or over heated faulty component can cause noise arise in image because of sharp and sudden changes of Digital image processing is using of algorithms for image signal. 퐼 푖, 푗 푥 < 푙 improve quality order of digital image .This error on 퐼푠푝 푖, 푗 = image is called noise in image which do not reflect real 퐼푚푖푛 + 푌 퐼푚푎푥 −퐼푚푖푛 푥 > 푙 intensities of actual scene. There are two problems found x,y∈[0,1] are two uniformly distributed random variables in image processing: Blurring and image noise. Noise image occurred by many reasons: When we capture image from camera (scratches are available in camera). -
Performance Analysis of Spatial and Transform Filters for Efficient Image Noise Reduction
Performance Analysis of Spatial and Transform Filters for Efficient Image Noise Reduction Santosh Paudel Ajay Kumar Shrestha Pradip Singh Maharjan Rameshwar Rijal Computer and Electronics Computer and Electronics Computer and Electronics Computer and Electronics Engineering Engineering Engineering Engineering KEC, TU KEC, TU KEC, TU KEC, TU Lalitpur, Nepal Lalitpur, Nepal Lalitpur, Nepal Lalitpur, Nepal [email protected] [email protected] [email protected] [email protected] Abstract—During the acquisition of an image from its systems such as laser, acoustics and SAR (Synthetic source, noise always becomes integral part of it. Various Aperture Radar) images [3]. algorithms have been used in past to denoise the images. Image denoising still has scope for improvement. Visual This paper introduces different types of noise to be information transmitted in the form of digital images has considered in an image and analyzed for various spatial become a considerable method of communication in the and transforms domain filters by considering the image modern age, but the image obtained after transmission is metrics such as mean square error (MSE), root mean often corrupted due to noise. In this paper, we review the squared error (RMSE), Peak Signal to Noise Ratio existing denoising algorithms such as filtering approach (PSNR) and universal quality index (UQI). and wavelets based approach, and then perform their comparative study with bilateral filters. We use different II. BACKGROUND noise models to describe additive and multiplicative noise The Wavelet Transform (WT) is a powerful tool of in an image. Based on the samples of degraded pixel signal and image processing, which has been neighborhoods as inputs, the output of an efficient filtering successfully used in many scientific fields such as signal approach has shown a better image denoising performance. -
"Seeing a Black Hole" the First Image of a Black Hole from the Event Horizon Telescope
"Seeing a Black Hole" The First Image of a Black Hole from the Event Horizon Telescope Matthew Newby Temple University Department of Physics May 1, 2019 "Seeing a Black Hole" The First Image of a Black Hole from the Event Horizon Telescope ● Black Holes – a Background ● Techniques to observe M87* ● Implications Matthew Newby, Temple University, May 1, 2019 2 "Seeing a Black Hole" Matthew Newby, Temple University, May 1, 2019 3 What is a black hole? Classical escape velocity: Let vesc → c, and the escape velocity is greater than the speed of light → “Black” Matthew Newby, Temple University, May 1, 2019 4 In General Relativity Einstein (and Hilbert) Field Equation Metric tensor Stress-energy tensor Ricci curvature tensor Scalar curvature “Solution” (“source” term) Matthew Newby, Temple University, May 1, 2019 5 Schwarzschild Metric Spherically symmetric, isolated, vacuum solution: Constant rs Schwarzschild Radius: Looks like classical escape velocity! Matthew Newby, Temple University, May 1, 2019 6 Space-Time Interval ● τ is proper time ● t is time measured at infinity (τ∞) ● r, θ, φ, are Schwarzschild spherical coordinates (i.e., coordinates as viewed at infinity) ● ds is a path element in spacetime Matthew Newby, Temple University, May 1, 2019 7 General Relativistic Time Dilation Allow a photon emitted at r to travel to infinity; in that photon’s rest frame: Since the frequency of a photon is a proper time interval, this implies that the photon’s frequency (and energy) are lower as it travels away from a spherical mass. Matthew Newby, Temple University, May 1, 2019 8 The Event Horizon rs is the “Surface of infinite redshift” or event horizon The event horizon is the “surface” of a black hole. -
Nasa Tm- 77750 Nasa Technical Memorandum Nasa Tm-77750
NASA TM- 77750 NASA TECHNICAL MEMORANDUM NASA TM-77750 NASA-TM-77750 19850004171 PATTERNS OF BEHAVIOD<TN LODGINGS EXPOSED TO TRAFFIC NOISE Jacques Lambert, Francois Simonnet Translation of "Comportements dans l'habitat soumis au bruit de circulation". Institut de Recherche des Transports, Arcueil, France, Rapport de Recherche I.R.T. No. 47, September, 1980, pp 1-145. 11.,. NATIONAL AERONAUTICS AND SPACE ADMINISTRATION WASHINGTON D.C. 20546 NOVEMBER 1984 • • \ IT........ f.n.• PM. ,. II. 0 ... I. .M.,...·.c.......... NAS1\. TM.,-77750 .. , ...... S....... PATTERNS or' BEHAVIOR IN I. • .,.,. hie November, 1984 TF~FFIC LODGINGS EXPOSED TO NOISE • •. ,.,te-t". 0, ee. 70 A.......c.. I. ''''e''''. 0. H.. Jacques Lambert, Francois Simonnet 11...... "-'..... '. 1-------------------------1... e.......... 0......... t. ' .......... 0,.......'... N... et4 ........ MAS... .~C; 42 SCITRAN • lox S4S6 .' II. ,,,..,......., ...c.....4 r.__ • a _..,.... ClI·un. 'rraul.t1oll, 12. SU4t1~&:r"&;rD_==_ .. Sp.at MaiIliat~.t.io.....-----------..f VUD1qtOD. D~Ce ~0546 No Ate-f c... I'" ...........,.......Translatlon. .. of "COITInortements dans l'habltat. soumis au bruit de circulation".'" Institut de·Recherche des Transports, Arcuei1, France, Rapport de Recherche' I ~R •. ~.· No. 47, September, 1980, pp. 1-145. , .. M ......· Thresho1c values at which public services should intervene ~o attenuate the noise nuisance are defined. Observations were made in the field of daily life at .. home. Data was collecte<J. on the use of loe1gings, on effects of noise on health and sleep~ and on the incidence of running away from home. A correlation was made also with the equipment. and noise insulation of lodgings. The results s.how that abov.eGG dB in daytime, there are behavior patterns that are extreme so far as they modify in a considerable manner the way bf, life of-people, living in both collective housing Capartments) and in individual houses • • ~. -
Noise Assessment Activities
Noise assessment activities Interesting stories in Europe ETC/ACM Technical Paper 2015/6 April 2016 Gabriela Sousa Santos, Núria Blanes, Peter de Smet, Cristina Guerreiro, Colin Nugent The European Topic Centre on Air Pollution and Climate Change Mitigation (ETC/ACM) is a consortium of European institutes under contract of the European Environment Agency RIVM Aether CHMI CSIC EMISIA INERIS NILU ÖKO-Institut ÖKO-Recherche PBL UAB UBA-V VITO 4Sfera Front page picture: Composite that includes: photo of a street in Berlin redesigned with markings on the asphalt (from SSU, 2014); view of a noise barrier in Alverna (The Netherlands)(from http://www.eea.europa.eu/highlights/cutting-noise-with-quiet-asphalt), a page of the website http://rumeur.bruitparif.fr for informing the public about environmental noise in the region of Paris. Author affiliation: Gabriela Sousa Santos, Cristina Guerreiro, Norwegian Institute for Air Research, NILU, NO Núria Blanes, Universitat Autònoma de Barcelona, UAB, ES Peter de Smet, National Institute for Public Health and the Environment, RIVM, NL Colin Nugent, European Environment Agency, EEA, DK DISCLAIMER This ETC/ACM Technical Paper has not been subjected to European Environment Agency (EEA) member country review. It does not represent the formal views of the EEA. © ETC/ACM, 2016. ETC/ACM Technical Paper 2015/6 European Topic Centre on Air Pollution and Climate Change Mitigation PO Box 1 3720 BA Bilthoven The Netherlands Phone +31 30 2748562 Fax +31 30 2744433 Email [email protected] Website http://acm.eionet.europa.eu/ 2 ETC/ACM Technical Paper 2015/6 Contents 1 Introduction ...................................................................................................... 5 2 Noise Action Plans ......................................................................................... -
An Unprecedented Global Communications Campaign for the Event Horizon Telescope First Black Hole Image
An Unprecedented Global Communications Campaign Best for the Event Horizon Telescope First Black Hole Image Practice Lars Lindberg Christensen Colin Hunter Eduardo Ros European Southern Observatory Perimeter Institute for Theoretical Physics Max-Planck Institute für Radioastronomie [email protected] [email protected] [email protected] Mislav Baloković Katharina Königstein Oana Sandu Center for Astrophysics | Harvard & Radboud University European Southern Observatory Smithsonian [email protected] [email protected] [email protected] Sarah Leach Calum Turner Mei-Yin Chou European Southern Observatory European Southern Observatory Academia Sinica Institute of Astronomy and [email protected] [email protected] Astrophysics [email protected] Nicolás Lira Megan Watzke Joint ALMA Observatory Center for Astrophysics | Harvard & Suanna Crowley [email protected] Smithsonian HeadFort Consulting, LLC [email protected] [email protected] Mariya Lyubenova European Southern Observatory Karin Zacher Peter Edmonds [email protected] Institut de Radioastronomie de Millimétrique Center for Astrophysics | Harvard & [email protected] Smithsonian Satoki Matsushita [email protected] Academia Sinica Institute of Astronomy and Astrophysics Valeria Foncea [email protected] Joint ALMA Observatory [email protected] Harriet Parsons East Asian Observatory Masaaki Hiramatsu [email protected] Keywords National Astronomical Observatory of Japan Event Horizon Telescope, media relations, [email protected] black holes An unprecedented coordinated campaign for the promotion and dissemination of the first black hole image obtained by the Event Horizon Telescope (EHT) collaboration was prepared in a period spanning more than six months prior to the publication of this result on 10 April 2019. -
Analysis of Image Noise in Multispectral Color Acquisition
ANALYSIS OF IMAGE NOISE IN MULTISPECTRAL COLOR ACQUISITION Peter D. Burns Submitted to the Center for Imaging Science in partial fulfillment of the requirements for Ph.D. degree at the Rochester Institute of Technology May 1997 The design of a system for multispectral image capture will be influenced by the imaging application, such as image archiving, vision research, illuminant modification or improved (trichromatic) color reproduction. A key aspect of the system performance is the effect of noise, or error, when acquiring multiple color image records and processing of the data. This research provides an analysis that allows the prediction of the image-noise characteristics of systems for the capture of multispectral images. The effects of both detector noise and image processing quantization on the color information are considered, as is the correlation between the errors in the component signals. The above multivariate error-propagation analysis is then applied to an actual prototype system. Sources of image noise in both digital camera and image processing are related to colorimetric errors. Recommendations for detector characteristics and image processing for future systems are then discussed. Indexing terms: color image capture, color image processing, image noise, error propagation, multispectral imaging. Electronic Distribution Edition 2001. ©Peter D. Burns 1997, 2001 All rights reserved. COPYRIGHT NOTICE P. D. Burns, ‘Analysis of Image Noise in Multispectral Color Acquisition’, Ph.D. Dissertation, Rochester Institute of Technology, 1997. Copyright © Peter D. Burns 1997, 2001 Published by the author All rights reserved. No part of this work may be reproduced, stored in a retrieval system, or transmitted in any form, or by any means, electronic, mechanical, photocopying, recording or otherwise, without prior written permission of the copyright holder. -
Feature Extraction on Synthetic Black Hole Images
Feature Extraction on Synthetic Black Hole Images Joshua Yao-Yu Lin 1 George N. Wong 1 Ben S. Prather 1 Charles F. Gammie 1 2 3 Abstract 80 80 The Event Horizon Telescope (EHT) recently re- 60 60 leased the first horizon-scale images of the black 40 40 hole in M87. Combined with other astronomical 20 20 data, these images constrain the mass and spin of as 0 0 the hole as well as the accretion rate and magnetic µ 20 20 flux trapped on the hole. An important question − − 40 40 for EHT is how well key parameters such as spin − − 60 60 and trapped magnetic flux can be extracted from − − 80 80 − 75 50 25 0 25 50 75 − 75 50 25 0 25 50 75 present and future EHT data alone. Here we ex- − − − − − − plore parameter extraction using a neural network µas µas trained on high resolution synthetic images drawn from state-of-the-art simulations. We find that the Figure 1. Synthetic image examples. Left panel: full resolution neural network is able to recover spin and flux simulated black hole image based on numerical model of black with high accuracy. We are particularly interested hole accretion flow with M87-like parameters. Right panel: the in interpreting the neural network output and un- same simulated image convolved with 20µas FWHM Gaussian derstanding which features are used to identify, beam meant to represent the resolving power of the EHT. e.g., black hole spin. Using feature maps, we find that the network keys on low surface brightness with data from other sources, the EHT images constrain features in particular. -
Local Noise Action Plans
Practitioner Handbook for Local Noise Action Plans Recommendations from the SILENCE project SILENCE is an Integrated Project co-funded by the European Commission under the Sixth Framework Programme for R&D, Priority 6 Sustainable Development, Global Change and Ecosystems Guidance for readers Step 1: Getting started – responsibilities and competences • These pages give an overview on the steps of action planning and Objective To defi ne a leader with suffi cient capacities and competences to the noise abatement measures and are especially interesting for successfully setting up a local noise action plan. To involve all relevant stakeholders and make them contribute to the implementation of the plan clear competences with the leading department are needed. The END ... DECISION MAKERS and TRANSPORT PLANNERS. Content Requirements of the END and any other national or The current responsibilities for noise abatement within the local regional legislation regarding authorities will be considered and it will be assessed whether these noise abatement should be institutional settings are well fi tted for the complex task of noise considered from the very action planning. It might be advisable to attribute the leadership to beginning! another department or even to create a new organisation. The organisational settings for steering and carrying out the work to be done will be decided. The fi nancial situation will be clarifi ed. A work plan will be set up. If support from external experts is needed, it will be determined in this stage. To keep in mind For many departments, noise action planning will be an additional task. It is necessary to convince them of the benefi ts and the synergies with other policy fi elds and to include persons in the steering and working group that are willing and able to promote the issue within their departments. -
Measurement of Noise and Resolution in PET 1071 Large ROI in a Single Static Image
IOP PUBLISHING PHYSICS IN MEDICINE AND BIOLOGY Phys. Med. Biol. 55 (2010) 1069–1081 doi:10.1088/0031-9155/55/4/011 Simultaneous measurement of noise and spatial resolution in PET phantom images Martin A Lodge1, Arman Rahmim1 and Richard L Wahl1,2 1 Division of Nuclear Medicine, The Russell H. Morgan Department of Radiology and Radiological Sciences, Johns Hopkins University School of Medicine, Baltimore, MD, USA 2 Sidney Kimmel Comprehensive Cancer Center at Johns Hopkins, Johns Hopkins University School of Medicine, Baltimore, MD, USA E-mail: [email protected] Received 31 August 2009, in final form 21 December 2009 Published 28 January 2010 Online at stacks.iop.org/PMB/55/1069 Abstract As an aid to evaluating image reconstruction and correction algorithms in positron emission tomography, a phantom procedure has been developed that simultaneously measures image noise and spatial resolution. A commercially available 68Ge cylinder phantom (20 cm diameter) was positioned in the center of the field-of-view and two identical emission scans were sequentially performed. Image noise was measured by determining the difference between corresponding pixels in the two images and by calculating the standard deviation of these difference data. Spatial resolution was analyzed using a Fourier technique to measure the extent of the blurring at the edge of the phantom images. This paper addresses the noise aspects of the technique as the spatial resolution measurement has been described elsewhere. The noise measurement was validated by comparison with data obtained from multiple replicate images over a range of noise levels. In addition, we illustrate how simultaneous measurement of noise and resolution can be used to evaluate two different corrections for random coincidence events: delayed event subtraction and singles-based randoms correction. -
Interaction of Image Noise, Spatial Resolution, and Low Contrast Fine
Interaction of image noise, spatial resolution, and low contrast fine detail preservation in digital image processing Uwe Artmanna and Dietmar Wuellerb a,bImage Engineering, Augustinusstrasse 9d, 50226 Frechen, Germany; ABSTRACT We present a method to improve the validity of noise and resolution measurements on digital cameras. If non-linear adaptive noise reduction is part of the signal processing in the camera, the measurement results for image noise and spatial resolution can be good, while the image quality is low due to the loss of fine details and a watercolor like appearance of the image. To improve the correlation between objective measurement and subjective image quality we propose to supplement the standard test methods with an additional measurement of the texture preserving capabilities of the camera. The proposed method uses a test target showing white Gaussian noise. The camera under test reproduces this target and the image is analyzed. We propose to use the kurtosis of the derivative of the image as a metric for the texture preservation of the camera. Kurtosis is a statistical measure for the closeness of a distribution compared to the Gaussian distribution. It can be shown, that the distribution of digital values in the derivative of the image showing the chart becomes the more leptokurtic (increased kurtosis) the stronger the noise reduction has an impact on the image. Keywords: Noise, Noise Reduction, Texture, Resolution, Spatial Frequency, Kurtosis, MTF, SFR 1. INTRODUCTION ColorFoto is a German photography magazine with a focus on objective and complex tests on digital still camera systems. Since we started testing in 1997, the tests had to be adjusted from time to time to keep track with the development in the camera market, so the test results correlate with the subjective image quality, experienced by the user.