Frequency Multiplication in Silicon Nanowires
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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. -
Applied Engineering Using Schumann Resonance for Earthquakes Monitoring
applied sciences Article Applied Engineering Using Schumann Resonance for Earthquakes Monitoring Jose A. Gazquez 1,2, Rosa M. Garcia 1,2, Nuria N. Castellano 1,2 ID , Manuel Fernandez-Ros 1,2 ID , Alberto-Jesus Perea-Moreno 3 ID and Francisco Manzano-Agugliaro 1,* ID 1 Department Engineering, University of Almeria, CEIA3, 04120 Almeria, Spain; [email protected] (J.A.G.); [email protected] (R.M.G.); [email protected] (N.N.C.); [email protected] (M.F.-R.) 2 Research Group of Electronic Communications and Telemedicine TIC-019, 04120 Almeria, Spain 3 Department of Applied Physics, University of Cordoba, CEIA3, Campus de Rabanales, 14071 Córdoba, Spain; [email protected] * Correspondence: [email protected]; Tel.: +34-950-015396; Fax: +34-950-015491 Received: 14 September 2017; Accepted: 25 October 2017; Published: 27 October 2017 Abstract: For populations that may be affected, the risks of earthquakes and tsunamis are a major concern worldwide. Therefore, early detection of an event of this type in good time is of the highest priority. The observatories that are capable of detecting Extremely Low Frequency (ELF) waves (<300 Hz) today represent a breakthrough in the early detection and study of such phenomena. In this work, all earthquakes with tsunami associated in history and all existing ELF wave observatories currently located worldwide are represented. It was also noticed how the southern hemisphere lacks coverage in this matter. In this work, the most suitable locations are proposed to cover these geographical areas. Also, ELF data processed obtained from the observatory of the University of Almeria in Calar Alto, Spain are shown. -
Through-The-Earth Electromagnetic Trapped Miner Location Systems. a Review
Open File Report: 127-85 THROUGH-THE-EARTH ELECTROMAGNETIC TRAPPED MINER LOCATION SYSTEMS. A REVIEW By Walter E. Pittman, Jr., Ronald H. Church, and J. T. McLendon Tuscaloosa Research Center, Tuscaloosa, Ala. UNITED STATES DEPARTMENT OF THE INTERIOR BUREAU OF MINES Research at the Tuscaloosa Research Center is carried out under a memorandum of agreement between the Bureau of Mines, U. S. Department of the Interior, and the University of Alabama. CONTENTS .Page List of abbreviations ............................................. 3 Abstract .......................................................... 4 Introduction ...................................................... 4 Early efforts at through-the-earth communications ................. 5 Background studies of earth electrical phenomena .................. 8 ~ationalAcademy of Engineering recommendations ................... 10 Theoretical studies of through-the-earth transmissions ............ 11 Electromagnetic noise studies .................................... 13 Westinghouse - Bureau of Mines system ............................ 16 First phase development and testing ............................. 16 Second phase development and testing ............................ 17 Frequency-shift keying (FSK) beacon signaler .................... 19 Anomalous effects ................................................ 20 Field testing and hardware evolution .............................. 22 Research in communication techniques .............................. 24 In-mine communication systems .................................... -
What Is Rf? It's Like Magic
Originally appeared in the December 2011 issue of Communications Technology. WHAT IS RF? IT’S LIKE MAGIC By RON HRANAC The cable industry has, since the very first systems in the late 1940s, embraced and been based on radio frequency (RF) technology. These days, we’ve also embraced the digital world — and a subset of digital technology called Internet protocol (IP) — but RF still is needed in most cable networks to transport digital data to and from devices in our subscribers’ homes. The answer to the question in the title of this month’s column is far more complicated than it seems initially. A good place to start is with an explanation of “R” and “F.” What’s radio frequency? Here’s one high-level perspective: It’s that portion of the electromagnetic spectrum from a few kilohertz to about 300 gigahertz. The radio-frequency part of the electromagnetic spectrum is further broken down into two chunks: radio waves and microwaves. Some references define radio waves as those with a frequency starting at about 3 kHz (the beginning of the very low frequency [VLF] band) and extending to 300 MHz (the beginning of the ultra high frequency [UHF] band), with microwaves covering roughly 300 MHz to 300 GHz. The latter is the beginning of the far infrared (FIR) portion of the electromagnetic spectrum. Other references have microwaves starting at frequencies higher than 300 MHz; indeed, many RF engineers consider the microwave spectrum to be higher than about 1 GHz. Radio frequency also can be defined as a rate of oscillation within the 3 kHz to 300 GHz range (more on this in a moment). -
The Effect of the Ionosphere on Ultra-Low-Frequency Radio-Interferometric Observations? F
A&A 615, A179 (2018) Astronomy https://doi.org/10.1051/0004-6361/201833012 & © ESO 2018 Astrophysics The effect of the ionosphere on ultra-low-frequency radio-interferometric observations? F. de Gasperin1,2, M. Mevius3, D. A. Rafferty2, H. T. Intema1, and R. A. Fallows3 1 Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands e-mail: [email protected] 2 Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany 3 ASTRON – the Netherlands Institute for Radio Astronomy, PO Box 2, 7990 AA Dwingeloo, The Netherlands Received 13 March 2018 / Accepted 19 April 2018 ABSTRACT Context. The ionosphere is the main driver of a series of systematic effects that limit our ability to explore the low-frequency (<1 GHz) sky with radio interferometers. Its effects become increasingly important towards lower frequencies and are particularly hard to calibrate in the low signal-to-noise ratio (S/N) regime in which low-frequency telescopes operate. Aims. In this paper we characterise and quantify the effect of ionospheric-induced systematic errors on astronomical interferometric radio observations at ultra-low frequencies (<100 MHz). We also provide guidelines for observations and data reduction at these frequencies with the LOw Frequency ARray (LOFAR) and future instruments such as the Square Kilometre Array (SKA). Methods. We derive the expected systematic error induced by the ionosphere. We compare our predictions with data from the Low Band Antenna (LBA) system of LOFAR. Results. We show that we can isolate the ionospheric effect in LOFAR LBA data and that our results are compatible with satellite measurements, providing an independent way to measure the ionospheric total electron content (TEC). -
Methods and Experiments for Sensing Variations in Solar Activity and Defining Their Impact on Heart Variability
sensors Article Methods and Experiments for Sensing Variations in Solar Activity and Defining Their Impact on Heart Variability Michael Hanzelka 1,*, Jiˇrí Dan 2, Zoltán Szabó 1 , ZdenˇekRoubal 1, PˇremyslDohnal 1 and Radim Kadlec 1 1 Department of Theoretical and Experimental Electrical Engineering, Brno University of Technology, 616 00 Brno, Czech Republic; [email protected] (Z.S.); [email protected] (Z.R.); [email protected] (P.D.); [email protected] (R.K.) 2 Department of Psychology, Faculty of Arts and Letter, Catholic University in Ružomberok, 034 01 Ružomberok, Slovakia; [email protected] * Correspondence: [email protected]; Tel.: +420-54114-6280 Abstract: This paper evaluates variations in solar activity and their impact on the human nervous system, including the manner in which human behavior and decision-making reflect such effects in the context of (symmetrical) social interactions. The relevant research showed that solar activity, manifesting itself through the exposure of the Earth to charged particles from the Sun, affects heart variability. The evaluation methods focused on examining the relationships between selected psychophysiological data and solar activity, which generally causes major alterations in the low-level electromagnetic field. The investigation within this paper revealed that low-level EMF changes are among the factors affecting heart rate variability and, thus, also variations at the spectral level of the rate, in the VLF, (f = 0.01–0.04 Hz), LF (f = 0.04–0.15 Hz), and HF (f = 0.15 až 0.40 Hz) bands. The results of the presented experiments can also be interpreted as an indirect explanation of sudden Citation: Hanzelka, M.; Dan, J.; Szabó, Z.; Roubal, Z.; Dohnal, P.; deaths and heart failures. -
A Novel Database of Bio-Effects from Non-Ionizing Radiation
A Novel Database of Bio-Effects From Non-Ionizing Radiation by Leach VA, Weller S and Redmayne M. ORSAA paper ID: 3088 OPEN SOURCE: https://www.degruyter.com/view/journals/reveh/33/3/article-p273.xml Rev Environ Health 2018; aop Review Victor Leach*, Steven Weller and Mary Redmayne A novel database of bio-effects from non-ionizing radiation https://doi.org/10.1515/reveh-2018-0017 Received March 18, 2018; accepted May 6, 2018 Introduction Abstract: A significant amount of electromagnetic field/ The environmental profile of man-made electromagnetic electromagnetic radiation (EMF/EMR) research is availa- field (EMF) and associated radiation [electromagnetic ble that examines biological and disease associated end- radiation (EMR)] over the last several decades has grown points. The quantity, variety and changing parameters in by 12 orders of magnitude (1012) [1] and is now considered the available research can be challenging when under- one of the major sources of environmental pollution. taking a literature review, meta-analysis, preparing a During more recent years, the use of mobile phones study design, building reference lists or comparing find- in close proximity to the brain has become a major focus ings between relevant scientific papers. The Oceania of much research. Successful marketing and subsequent Radiofrequency Scientific Advisory Association (ORSAA) uptake have necessitated an on-going increase in the has created a comprehensive, non-biased, multi-cate- number of mobile phone base stations being deployed, gorized, searchable database of papers on non-ionizing contributing to increasing levels of background, environ- EMF/EMR to help address these challenges. It is regu- mental non-ionizing radiation. -
An Agile Laser with Ultra-Low Frequency Noise and High Sweep Linearity
An agile laser with ultra-low frequency noise and high sweep linearity Haifeng Jiang 1,* , Fabien Kéfélian 2, Pierre Lemonde1, André Clairon 1 and Giorgio Santarelli 1 1Laboratoire National de Métrologie et d’Essais–Système de Références Temps-Espace, Observatoire de Paris, UPMC and CNRS, 61 Avenue de l’Observatoire, 75014 Paris, France 2Laboratoire de Physique des Lasers, Université Paris 13 and CNRS, 99 Avenue Jean-Baptiste Clément, 93430 Villetaneuse, France *[email protected] Abstract: We report on a fiber-stabilized agile laser with ultra-low frequency noise. The frequency noise power spectral density is comparable to that of an ultra-stable cavity stabilized laser at Fourier frequencies higher than 30 Hz. When it is chirped at a constant rate of ~ 40 MHz/s, the max non-linearity frequency error is about 50 Hz peak-to-peak over more than 600 MHz tuning range. The Rayleigh backscattering is found to be a significant frequency noise source dependent on fiber length, chirping rate and the power imbalance of the interferometer arms. We analyze this effect both theoretically and experimentally and put forward techniques to reduce this noise contribution. OCIS codes: (140.0140) Lasers and laser optics; (140.3425) Laser stabilization; (140.3518) Lasers, frequency modulated; (140.3600) Lasers, tunable; (290.5870) Scattering, Rayleigh. References and links 1. M. Harris, G. N. Pearson, J. M. Vaughan, D. Letalick, and C. Karlsson, “The role of laser coherence length in continuous-wave coherent laser radar,” J. Mod. Opt., 45 , 1567-1581, (1998). 2. R. W. Fox, C. W. Gates, and L. W. Hollberg, in Cavity-Enhanced Spectroscopies, R. -
Principes Et Utilisations RF Power Sources: Principles And
Alimentations RF: Principes et utilisations RF Power Sources: Principles and Use Erik V. Johnson LPICM-CNRS, Ecole Polytechnique Erik V. Johnson, 1 LPICM-CNRS, Ecole Polytechnique Erik V. Johnson, LPICM-CNRS, Ecole Polytechnique Erik V. Johnson, LPICM-CNRS, Ecole Polytechnique Erik V. Johnson, LPICM-CNRS, Ecole Polytechnique Erik V. Johnson, LPICM-CNRS, Ecole Polytechnique Erik V. Johnson, LPICM-CNRS, Ecole Polytechnique Erik V. Johnson, LPICM-CNRS, Ecole Polytechnique Erik V. Johnson, LPICM-CNRS, Ecole Polytechnique Erik V. Johnson, LPICM-CNRS, Ecole Polytechnique Outline – RF Power Sources • Frequencies of operation • ITU/STM Frequency bands for RF plasmas • Amplifiers vs Power Sources • Input and Output Power • Expected impedance and matching • Gain compression • Harmonics (THD and dBc) • Classes of Amplifier • Class A – Wideband amplifier • Classes B to E – Narrow band Erik V. Johnson, LPICM-CNRS, Ecole Polytechnique What do we mean by RF plasma excitation Technically, all frequencies at which we can generate EM waves through oscillations in a macroscopic dipole/antenna are radio frequencies. Direct current (0 Hz) does not generate an EM wave, and optical frequency waves are not generated in the same way (and physics is different). For plasmas, we are particularly interested in the band of frequencies where electrons can respond but ions are too heavy, and things are still technologically manageable. Erik V. Johnson, LPICM-CNRS, Ecole Polytechnique Radio Frequencies and ISM Bands International Telecommunications Union has split up spectrum into named bands. Frequencies of 1 GHz and above are conventionally called microwave,[7] while frequencies of 30 GHz and above are designated millimeter wave. Erik V. Johnson, LPICM-CNRS, Ecole Polytechnique ITU Band name Abbrev. -
Passive Ultra-Low Frequency Electromagnetic Detection Coal Bed Methane Technology and Application
PASSIVE ULTRA-LOW FREQUENCY ELECTROMAGNETIC DETECTION TECHNOLOGY FOR COAL BED METHANE AND ITS APPLICATION Qin Qiming, Li Baishou, Li Peijun, Zhang Zexun, Ye Xia, Cui Rongbo School of Earth and Space Sciences, Peking University, Beijing, 100871 [email protected] KEYWORDS: Ultra-Low Frequency Electromagnetic Wave, CBM Exploration, Geophysical Method ABSTRACT: Based on analysis of the significance of the coal bed methane exploration and development and the deficiency of the conventional coal bed methane exploration methods, the paper proposes a new technology of coal bed methane exploration with natural-source (passive) ultra-low frequency electromagnetic waves. The principles of passive ultra-low frequency electromagnetic detection and the mechanism of coal bed methane exploration are first introduced. The paper then shows the coal bed methane explorationexperiments and the latest research results in the Qinshui Basin of Shanxi using BD-6-ultra-low frequency electromagnetic detector developed by Peking University. Finally, the further application of the technology in the exploration of coal bed methane is discussed. 1. INTRODUCTION methane. Based on prior knowledge, through signal parameters inversion and quantitative analysis of the electromagnetic Commonly known as gas, coal bed methane (CBM) is a spectrum, we can quickly and efficiently obtain information of unconventional natural gas. It consists mostly of methane (CH4) the spatial distribution, storage conditions and enrichment but may also contain trace amounts of carbon dioxide and/or degree of coal bed methane, then narrowing detecting target [1] nitrogen. As the CBM is flammable and explosive, it has to reduce drilling costs and improve the efficiency of drilling, to become a main bottlenecks of the safety production. -
Mathematical Analysis of Super Low Frequency Ground Loop Receiving Antennas
Appl. Math. Inf. Sci. 7, No. 3, 1087-1092 (2013) 1087 Applied Mathematics & Information Sciences An International Journal ⃝c 2013 NSP Natural Sciences Publishing Cor. Mathematical Analysis of Super Low Frequency Ground Loop Receiving Antennas Hui Xie1, Ming Yang2 and Long Ji3 1Electronics Engineering College, Navy University of engineering, Wuhan 430033, China 2Unit 91404 of PLA, Qinhuangdao 066000, China 3702 repair factory of Navy, Shanghai 200434, China Received: 20 Sep. 2012, Revised: 30 Dec. 2012, Accepted: 14 Jan. 2013 Published online: 1 May 2013 Abstract: A compact super low frequency receiving antenna in the form of a loop can be built for which the induced atmospheric noise voltage dominates both the antennas thermal noise voltage and preamplifier noise. Air-core and ferromagnetic-core ground loop receiving antennas were introduced, and mathematical calculation methods to analyse the ENF spectrum of the atmospheric noise and thermal noise were derived. The research identified the roles played by the various contributing factors such as antenna dimensions, wire conductivity, ferromagnetic-core permeability, etc. One air-core and three ferromagnetic-core antennas were designed, and a compromise core design was recommend, which takes advantage of the improvement that ferromagnetic cores can provide while largely avoiding the disadvantages. Keywords: super low frequency, loop receiving antenna, air-core loop, ferromagnetic core loop 1. Introduction factor of self-resonance may increase the output signal voltage, this is more than offset by a concomitant increase The two most conventional super low frequency (SLF) in the resistance of the antenna [4]. Usually, therefore, at receiving antennas are the whip and the loop. -
Ultra Low Frequency Infrasonic Measurement System
Rasmus Trock Kinnerup, s052256 Ultra Low Frequency Infrasonic Measurement System Master's Thesis, July 2011 Abstract An infrasonic measurement system is built capable of sensing acoustic signals down to 10 mHz which is advantageous for measurements of wind farm noise or sonic boom shapers. The system consists of an electric preamplifier built into a housing and a G.R.A.S. 40AZ 1 2 -inch prepolarized condenser microphone with a closed vent configuration. The total system has a dynamic range of 94 dB and a lower limiting -3 dB cutoff frequency of 8 mHz. The preamplifier connects the microphone signal directly to the input of an op-amp with an input resistance of 10 TΩ, one of the industry's highest, which forms a high pass filter with the microphone capacitance of 20 pF. The bias current is supplied to the input node by two diode-connected FETs. The big challenge has been to sense the sound signal from the capacitive microphone with a high enough input impedance of the preamplifier to avoid an inherent cutoff of frequencies of interest. Being able to measure down to ultra low frequencies in the infrasonic frequency range will aid actors in the debate on wind turbine noise. Sonic booms from supersonic flights include frequencies down to 10 mHz and this measurement system will aid scientists trying to modify the N-shaped shock wave at high level which prohibits flights in land zones. To my wife Cathrine and our children Alfred and Carla Preface This report is a Master's Thesis in Electrical Engineering at the Department of Electrical Engineering at the Technical University of Denmark.