Electromagnetic Radiation and Human Health: a Review of Sources and Effects
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Observation of Strong Nonlinear Interactions in Parametric Down
Observation of strong nonlinear interactions in parametric down- conversion of x-rays into ultraviolet radiation Authors: S. Sofer1*, O. Sefi1*, E. Strizhevsky1, S.P. Collins2, B. Detlefs3, Ch.J. Sahle3, and S. Shwartz1 *S. Sofer and O. Sefi contributed equally to this work. Affiliations: 1Physics Department and Institute of Nanotechnology, Bar-Ilan University, Ramat Gan, 52900 Israel 2 Diamond Light Source, Harwell Science and Innovation Campus, Didcot OX11 0DE, United Kingdom 3 ESRF – The European Synchrotron, CS 40220, 38043 Grenoble Cedex 9, France. Summary: Nonlinear interactions between x-rays and long wavelengths can be used as a powerful atomic scale probe for light-matter interactions and for properties of valence electrons. This probe can provide novel microscopic information in solids that existing methods cannot reveal, hence to advance the understanding of many phenomena in condensed matter physics. However, thus far, reported x-ray nonlinear effects were very small and their observations required tremendous efforts. Here we report the observation of unexpected strong nonlinearities in parametric down-conversion (PDC) of x-rays to long wavelengths in gallium arsenide (GaAs) and in lithium niobate (LiNbO3) crystals, with efficiencies that are about 4 orders of magnitude stronger than the efficiencies measured in any material studied before. These strong nonlinearities cannot be explained by any known theory and indicate on possibilities for the development of a new spectroscopy method that is orbital and band selective. In this work we demonstrate the ability to use PDC of x-rays to investigate the spectral response of materials in a very broad range of wavelengths from the infrared regime to the soft x-ray regime. -
WWVB: a Half Century of Delivering Accurate Frequency and Time by Radio
Volume 119 (2014) http://dx.doi.org/10.6028/jres.119.004 Journal of Research of the National Institute of Standards and Technology WWVB: A Half Century of Delivering Accurate Frequency and Time by Radio Michael A. Lombardi and Glenn K. Nelson National Institute of Standards and Technology, Boulder, CO 80305 [email protected] [email protected] In commemoration of its 50th anniversary of broadcasting from Fort Collins, Colorado, this paper provides a history of the National Institute of Standards and Technology (NIST) radio station WWVB. The narrative describes the evolution of the station, from its origins as a source of standard frequency, to its current role as the source of time-of-day synchronization for many millions of radio controlled clocks. Key words: broadcasting; frequency; radio; standards; time. Accepted: February 26, 2014 Published: March 12, 2014 http://dx.doi.org/10.6028/jres.119.004 1. Introduction NIST radio station WWVB, which today serves as the synchronization source for tens of millions of radio controlled clocks, began operation from its present location near Fort Collins, Colorado at 0 hours, 0 minutes Universal Time on July 5, 1963. Thus, the year 2013 marked the station’s 50th anniversary, a half century of delivering frequency and time signals referenced to the national standard to the United States public. One of the best known and most widely used measurement services provided by the U. S. government, WWVB has spanned and survived numerous technological eras. Based on technology that was already mature and well established when the station began broadcasting in 1963, WWVB later benefitted from the miniaturization of electronics and the advent of the microprocessor, which made low cost radio controlled clocks possible that would work indoors. -
Understanding Infrared Light
TEACHER/PARENT ACTIVITY MANUAL Joint Polar Satellite System Understanding Infrared Light This activity educates students about the electromagnetic spectrum, or different forms of light detected by Earth observing satellites. The Joint Polar Satellite System (JPSS), a collaborative effort between NOAA and NASA, detects various wavelengths of the electromagnetic spectrum including infrared light to measure the temperature of Earth’s surface, oceans, and atmosphere. The data from these measurements provide the nation with accurate weather forecasts, hurricane warnings, wildfire locations, and much more! Provided is a list of materials that can be purchased to complete several learning activities, including simulating infrared light by constructing homemade infrared goggles. Learning Objectives Next Generation Science Standards (Grades 5–8) Performance Disciplinary Description Expectation Core Ideas 4-PS4-1 PS4.A: • Waves, which are regular patterns of motion, can be made in water Waves and Their Wave Properties by disturbing the surface. When waves move across the surface of Applications in deep water, the water goes up and down in place; there is no net Technologies for motion in the direction of the wave except when the water meets a Information Transfer beach. (Note: This grade band endpoint was moved from K–2.) • Waves of the same type can differ in amplitude (height of the wave) and wavelength (spacing between wave peaks). 4-PS4-2 PS4.B: An object can be seen when light reflected from its surface enters the Waves and Their Electromagnetic eyes. Applications in Radiation Technologies for Information Transfer 4-PS3-2 PS3.B: Light also transfers energy from place to place. -
Ultraviolet – Visible Spectroscopy for Determination of Α- and Β-Acids in Beer Hops Katharine Chau Lab Partner: Logan Bi
Ultraviolet – Visible Spectroscopy for Determination of α- and β-acids in Beer Hops Katharine Chau Lab Partner: Logan Billings TA: Kevin Fischer Date lab performed: 3/20/2018 Date report submitted: 4/9/2018 ABSTRACT: In this experiment, the content of α- and β-acids in beer hops is found through UV-Vis spectroscopic analysis. Three samples will be prepared by extracting finely grained hops through methanol and diluting with methanolic NaOH. The spectrums obtained give a constant overall shape. The experiment was done to find out the concentration of the third component from degraded α- and β-acids that is also existing in the hops samples with the help of the calculated concentrations of α- and β-acids. From the calculated results, the average concentration of the third component in all three samples was 0.061 g/L. INTRODUCTION: UV-Vis spectroscopy is a useful absorption or reflectance spectroscopy that helps determine the quantity of analytes by detecting the absorptivity or reflectance of a sample under ultra-violet to visible light wavelength range (1). In this experiment, the absorptivity of the samples were measured and the content of different components were determined from the spectrum. In this lab, UV-Vis spectroscopy was used in to obtain absorbance spectrums of α- and β- acids found in difference hops samples. The structures of α- and β-acids are shown as the Fig. 1 below. Figure 1. Structures of major α- and β-acids found in hops By understanding the content of α-acid in the hops, the bitterness flavor of beer can be controlled since the bitterness is formed by the iso-form of α-acid through isomization of α-acid. -
Kindergarten High Frequency Word List
Kindergarten High Frequency Word List The following 40 words are the high frequency Kindergarten words. They are divided according to their probability of occurring in the corresponding DRA text levels. However, many of these words can occur throughout all levels. The goal is for all students to read, write, and use these words correctly by the end of Kindergarten. Level 1 Level 2 Level 3 Level 4 Level 5 a me to yes big I go in cat for is at on dog he the you like up she mom we my with this dad it by said look can no love play went see am do was and C:\Users\metcalfr\Downloads\K_5_High_Frequency_Word_Lists (2).docx October 2014 First Grade High Frequency Word list The goal is for all students to read, write, and use these words (and words from the kindergarten word list) correctly by the end of first grade. after have please all her saw an here should are him so as his some be I’m thank because if that but into them came just then come know they could little there day make us did many very end new want from not were get of what goes one when going or where good our who had out will has over would your C:\Users\metcalfr\Downloads\K_5_High_Frequency_Word_Lists (2).docx October 2014 Second Grade High Frequency Word List The goal is for all students to read, write, and use these words (and the words from preceding grade level word lists) correctly by the end of second grade. -
Energy Distribution of Optical Radiation Emitted by Electrical Discharges in Insulating Liquids
energies Article Energy Distribution of Optical Radiation Emitted by Electrical Discharges in Insulating Liquids Michał Kozioł Faculty of Electrical Engineering, Automatic Control and Informatics, Opole University of Technology, Proszkowska 76, 45-758 Opole, Poland; [email protected] Received: 26 March 2020; Accepted: 29 April 2020; Published: 1 May 2020 Abstract: This article presents the results of the analysis of energy distribution of optical radiation emitted by electrical discharges in insulating liquids, such as synthetic ester, natural ester, and mineral oil. The measurements of optical radiation were carried out on a system of needle–needle type electrodes and on a system for surface discharges, which were immersed in brand new insulating liquids. Optical radiation was recorded using optical spectrophotometry method. On the basis of the obtained results, potential possibilities of using the analysis of the energy distribution of optical radiation as an additional descriptor for the recognition of individual sources of electric discharges were indicated. The results can also be used in the design of various types of detectors, as well as high-voltage diagnostic systems and arc protection systems. Keywords: optical radiation; electrical discharges; insulating liquids; energy distribution 1. Introduction One of the characteristic features of electrical discharges is the emission to the space in which they occur, an electromagnetic wave with a very wide range. Such typical ranges of emitted radiation include ionizing radiation, such as X-rays, optical radiation, acoustic emission, and radio wave emission. Based on most of these emitted ranges, diagnostic methods were developed, which enables the detection and location of the source of electrical discharges, which is a great achievement in the diagnostics of high-voltage electrical insulating devices [1–4]. -
Relationship Between X-Ray and Ultraviolet Emission of Flares From
A&A 431, 679–686 (2005) Astronomy DOI: 10.1051/0004-6361:20041201 & c ESO 2005 Astrophysics Relationship between X-ray and ultraviolet emission of flares from dMe stars observed by XMM-Newton U. Mitra-Kraev1,L.K.Harra1,M.Güdel2, M. Audard3, G. Branduardi-Raymont1 ,H.R.M.Kay1,R.Mewe4, A. J. J. Raassen4,5, and L. van Driel-Gesztelyi1,6,7 1 Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UK e-mail: [email protected] 2 Paul Scherrer Institut, Würenlingen & Villigen, 5232 Villigen PSI, Switzerland 3 Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027, USA 4 SRON National Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands 5 Astronomical Institute “Anton Pannekoek”, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands 6 Observatoire de Paris, LESIA, 92195 Meudon, France 7 Konkoly Observatory, 1525 Budapest, Hungary Received 30 April 2004 / Accepted 30 September 2004 Abstract. We present simultaneous ultraviolet and X-ray observations of the dMe-type flaring stars AT Mic, AU Mic, EV Lac, UV Cet and YZ CMi obtained with the XMM-Newton observatory. During 40 h of simultaneous observation we identify 13 flares which occurred in both wave bands. For the first time, a correlation between X-ray and ultraviolet flux for stellar flares has been observed. We find power-law relationships between these two wavelength bands for the flare luminosity increase, as well as for flare energies, with power-law exponents between 1 and 2. We also observe a correlation between the ultraviolet flare energy and the X-ray luminosity increase, which is in agreement with the Neupert effect and demonstrates that chromospheric evaporation is taking place. -
High Frequency Communications – an Introductory Overview
High Frequency Communications – An Introductory Overview - Who, What, and Why? 13 August, 2012 Abstract: Over the past 60+ years the use and interest in the High Frequency (HF -> covers 1.8 – 30 MHz) band as a means to provide reliable global communications has come and gone based on the wide availability of the Internet, SATCOM communications, as well as various physical factors that impact HF propagation. As such, many people have forgotten that the HF band can be used to support point to point or even networked connectivity over 10’s to 1000’s of miles using a minimal set of infrastructure. This presentation provides a brief overview of HF, HF Communications, introduces its primary capabilities and potential applications, discusses tools which can be used to predict HF system performance, discusses key challenges when implementing HF systems, introduces Automatic Link Establishment (ALE) as a means of automating many HF systems, and lastly, where HF standards and capabilities are headed. Course Level: Entry Level with some medium complexity topics Agenda • HF Communications – Quick Summary • How does HF Propagation work? • HF - Who uses it? • HF Comms Standards – ALE and Others • HF Equipment - Who Makes it? • HF Comms System Design Considerations – General HF Radio System Block Diagram – HF Noise and Link Budgets – HF Propagation Prediction Tools – HF Antennas • Communications and Other Problems with HF Solutions • Summary and Conclusion • I‟d like to learn more = “Critical Point” 15-Aug-12 I Love HF, just about On the other hand… anybody can operate it! ? ? ? ? 15-Aug-12 HF Communications – Quick pretest • How does HF Communications work? a. -
Protecting Workers from Ultraviolet Radiation
Protecting Workers from Ultraviolet Radiation Editors: Paolo Vecchia, Maila Hietanen, Bruce E. Stuck Emilie van Deventer, Shengli Niu International Commission on Non-Ionizing Radiation Protection In Collaboration with: International Labour Organization World Health Organization ICNIRP 14/2007 International Commission on Non-Ionizing Radiation Protection ICNIRP Cataloguing in Publication Data Protecting Workers from Ultraviolet Radiation Protection ICNIRP 14/2007 1. Ultraviolet Radiation 2. Biological effects 3. Non-Ionizing Radiation ISBN 978-3-934994-07-2 The International Commission on Non-Ionizing Radiation Protection welcomes requests for permission to reproduce or translate its publications, in part or full. Applications and enquiries should be addressed to the Scientific Secretariat, which will be glad to provide the latest information on any changes made to the text, plans for new editions, and reprints and translations already available. © International Commission on Non-Ionizing Radiation Protection 2007 Publications of the International Commission on Non-Ionizing Radiation Protection enjoy copyright protection in accordance with the provisions of Protocol 2 of the Universal Copyright Convention. All rights reserved. ICNIRP Scientific Secretary Dr. G. Ziegelberger Bundesamt für Strahlenschutz Ingolstädter Landstraße 1 85764 Oberschleißheim Germany Tel: (+ 49 1888) 333 2156 Fax: (+49 1888) 333 2155 e-mail: [email protected] www.icnirp.org Printed by DCM, Meckenheim International Commission on Non-Ionizing Radiation Protection The International Commission on Non-Ionizing Radiation Protection (ICNIRP) is an independent scientific organization whose aims are to provide guidance and advice on the health hazards of non-ionizing radiation exposure. ICNIRP was established to advance non-ionizing radiation protection for the benefit of people and the environment. -
EHC 238 Front Pages Final.Fm
This report contains the collective views of an international group of experts and does not necessarily represent the decisions or the stated policy of the International Commission of Non- Ionizing Radiation Protection, the International Labour Organization, or the World Health Organization. Environmental Health Criteria 238 EXTREMELY LOW FREQUENCY FIELDS Published under the joint sponsorship of the International Labour Organization, the International Commission on Non-Ionizing Radiation Protection, and the World Health Organization. WHO Library Cataloguing-in-Publication Data Extremely low frequency fields. (Environmental health criteria ; 238) 1.Electromagnetic fields. 2.Radiation effects. 3.Risk assessment. 4.Envi- ronmental exposure. I.World Health Organization. II.Inter-Organization Programme for the Sound Management of Chemicals. III.Series. ISBN 978 92 4 157238 5 (NLM classification: QT 34) ISSN 0250-863X © World Health Organization 2007 All rights reserved. Publications of the World Health Organization can be obtained from WHO Press, World Health Organization, 20 Avenue Appia, 1211 Geneva 27, Switzerland (tel.: +41 22 791 3264; fax: +41 22 791 4857; e- mail: [email protected]). Requests for permission to reproduce or translate WHO publications – whether for sale or for noncommercial distribution – should be addressed to WHO Press, at the above address (fax: +41 22 791 4806; e-mail: [email protected]). The designations employed and the presentation of the material in this publication do not imply the expression of any opinion whatsoever on the part of the World Health Organization concerning the legal status of any country, territory, city or area or of its authorities, or concerning the delimitation of its frontiers or boundaries. -
How Do Radioactive Materials Move Through the Environment to People?
5. How Do Radioactive Materials Move Through the Environment to People? aturally occurring radioactive materials Radionuclides can be removed from the air in Nare present in our environment and in several ways. Particles settle out of the our bodies. We are, therefore, continuously atmosphere if air currents cannot keep them exposed to radiation from radioactive atoms suspended. Rain or snow can also remove (radionuclides). Radionuclides released to them. the environment as a result of human When these particles are removed from the activities add to that exposure. atmosphere, they may land in water, on soil, or Radiation is energy emitted when a on the surfaces of living and non-living things. radionuclide decays. It can affect living tissue The particles may return to the atmosphere by only when the energy is absorbed in that resuspension, which occurs when wind or tissue. Radionuclides can be hazardous to some other natural or human activity living tissue when they are inside an organism generates clouds of dust containing radionu- where radiation released can be immediately clides. absorbed. They may also be hazardous when they are outside of the organism but close ➤ Water enough for some radiation to be absorbed by Radionuclides can come into contact with the tissue. water in several ways. They may be deposited Radionuclides move through the environ- from the air (as described above). They may ment and into the body through many also be released to the water from the ground different pathways. Understanding these through erosion, seepage, or human activities pathways makes it possible to take actions to such as mining or release of radioactive block or avoid exposure to radiation. -
Cisco Broadband Data Book
Broadband Data Book © 2020 Cisco and/or its affiliates. All rights reserved. THE BROADBAND DATABOOK Cable Access Business Unit Systems Engineering Revision 21 August 2019 © 2020 Cisco and/or its affiliates. All rights reserved. 1 Table of Contents Section 1: INTRODUCTION ................................................................................................. 4 Section 2: FREQUENCY CHARTS ........................................................................................ 6 Section 3: RF CHARACTERISTICS OF BROADCAST TV SIGNALS ..................................... 28 Section 4: AMPLIFIER OUTPUT TILT ................................................................................. 37 Section 5: RF TAPS and PASSIVES CHARACTERISTICS ................................................... 42 Section 6: COAXIAL CABLE CHARACTERISTICS .............................................................. 64 Section 7: STANDARD HFC GRAPHIC SYMBOLS ............................................................. 72 Section 8: DTV STANDARDS WORLDWIDE ....................................................................... 80 Section 9: DIGITAL SIGNALS ............................................................................................ 90 Section 10: STANDARD DIGITAL INTERFACES ............................................................... 100 Section 11: DOCSIS SIGNAL CHARACTERISTICS ........................................................... 108 Section 12: FIBER CABLE CHARACTERISTICS ...............................................................