Scaled Modeling and Measurement for Studying Radio Wave Propagation in Tunnels
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Numerical Modelling of VLF Radio Wave Propagation Through Earth-Ionosphere Waveguide and Its Application to Sudden Ionospheric Disturbances
Numerical Modelling of VLF Radio Wave Propagation through Earth-Ionosphere Waveguide and its application to Sudden Ionospheric istur!ances Thesis submitted for the degree of octor of Philosoph# (Science% in Ph#sics (Theoretical) of the &niversity of 'alcutta Su(a# Pal Ma#8, )*+, CERTIFICATE FROM THE SUPERVISOR This is to certify that the thesis entitled "Numerical Modelling of VLF Radio Wave Propagation through Earth-Ionosphere waveguide and its application to !udden Ionospheric Distur#ances", submitted by Mr. Sujay Pal who got his name registered on $%&$'&%$(( for the award of Ph.D. )!cience* degree of the Universit, of Calcutta. absolutely based upon his own work under the supervision of Professor !andip K. Cha0ra#arti and that neither this thesis nor any part of it has been submitted for any degree/diploma or any other academic award anywhere before. Prof. !andip K. -ha0ra#arti Senior Professor & Head Department of #strophysics & Cosmology S. N. Bose National Centre for Basic Sciences JD Block, Sector())), Salt *ake, +olkata 7---./, India TO My PARENTS i ABSTRACT Very Low Frequency (VLF) radio waves with frequency in the range 3 30 kHz ∼ propagate within the Earth-ionosphere waveguide (EIWG) for#ed $y the Earth as the %ower $oundary and the %ower ionosphere (50 100 k#) as the upper $oundary ∼ of the waveguide. These waves are generated from #an-#ade transmitters as wel% as fro# lightnings or other natura% sources( *tudy of these waves is very i#portant since they are the only tool to diagnose the %ower ionosphere( Lower part of the Earth+s ionosphere ranging &0 90 km is known as the -- ∼ region of the ionosphere( *olar Lyman-α radiation at '.'./ n# and EUV radiation in 80 '''.& n# are #ain%y responsib%e for for#ing the --region through the ∼ ionization of 123N 23O 2 during day time( The VLF propagation takes p%ace $etween the Earth+s surface and the --region at the day time. -
Ground Penetrating Abilities of a New Coherent Radio Wave And
TECHNICAL pApEr Ground penetrating abilities of a new coherent radio wave and microwave imaging spectrometer G C Stove, M J Robinson, G D C Stove, and A Odell, Adrock; J McManus, Department of Earth Sciences, University of St Andrews he early use of synthetic aperture each subsurface rock layer. The aim transmitted ADR beams typically pulsed electromagnetic radio radar (SAR) and light detection of this article is to report on tests operate within the frequency range waves, microwaves, millimetric, or Tand ranging (Lidar) systems from of the subsurface Earth penetration of 1-100MHz (Stove 2005). sub-millimetric radio waves from aircraft and space shuttles revealed capabilities of a new spectrometer In recent years, the technology materials which permit the applied the ability of the signals to penetrate as well as its ability to recognize for the production of laser light energy to pass through the material. the ground surface. Atomic dielectric many sedimentary, igneous and has become widely available, and The resonant energy response resonance (ADR) technology was metamorphic rock types in real- applications of this medium to can be measured in terms of energy, developed as an improvement over world conditions. the examination of materials are frequency, and phase relationships. SAR and ground penetrating radar Although GPRs are now constantly expanding. Although the The precision with which the (GPR) to achieve deeper penetration popular as non-destructive testing earlier applications concentrated process can be measured helps of the Earth’s subsurface through the tools, their analytical capabilities on the use of visible laser light, define the unique interactive atomic creation and use of a novel type of are rather restricted and imaging the development of systems using or molecular response behaviour of coherent beam. -
Propagation Analysis of a 900 Mhz Spread Spectrum Centralized Traffic Signal Control System
PROPAGATION ANALYSIS OF A 900 MH Z SPREAD SPECTRUM CENTRALIZED TRAFFIC SIGNAL CONTROL SYSTEM Brian L. Urban, AS, BS, EIT Thesis Prepared for the Degree of MASTER OF SCIENCE UNIVERSITY OF NORTH TEXAS May 2006 APPROVED: Perry McNeill, Major Professor Michael Kozak, Committee Member Shuping Wang, Committee Member Bernard Vokoun, Committee Member Vijay Vaidyanathan, Departmental Program Coordinator Albert B. Grubbs, Chair of the Department of Engineering Technology Oscar Garcia, Dean of the College of Engineering Sandra L. Terrell, Dean of the Robert B. Toulouse School of Graduate Studies Urban, Brian L., Propagation analysis of a 900 MHz spread spectrum centralized traffic signal control system. Master of Science (Engineering Technology), May 2006, 88 pp., 20 tables, 27 illustrations, references, 25 titles. The objective of this research is to investigate different propagation models to determine if specified models accurately predict received signal levels for short path 900 MHz spread spectrum radio systems. The City of Denton, Texas provided data and physical facilities used in the course of this study. The literature review indicates that propagation models have not been studied specifically for short path spread spectrum radio systems. This work should provide guidelines and be a useful example for planning and implementing such radio systems. The propagation model involves the following considerations: analysis of intervening terrain, path length, and fixed system gains and losses. Copyright 2006 by Brian L. Urban ii ACKNOWLEDGEMENTS I acknowledge the following people for their efforts and contributions to my thesis. It would not have been completed without them. Special thanks to the author’s thesis advisor, Dr. -
VLF Radio Observations and Modeling
INDIAN CENTRE FOR SPACE PHYSICS ANNUAL REPORT (2013-2014) TABLE OF CONTENTS Report of the Governing Body 3 Governing Body of the Centre 4 Members of the Research Advisory Council 4 Academic Council Members 4 In-Charge, Academic Affairs 4 Dean (Academic) and Finance Officer 4 Administrative Officer 4 Public Information Officer 5 In Charge of the Departments 5 Faculty Members 5 Honorary Faculty Members 5 Project Scientists 5 Post-Doctoral Fellows 5 Senior Research Fellows 5 Junior Research Fellows 6 ICTP Senior Research Fellow 6 Visiting Research Scholars 6 Engineers / Laboratory Staff 6 Office Staff 6 Security Staff 6 Research Facilities at the Head Quarter 7 Facilities at other branches of the Centre 7 Brief Profiles of the Scientists of the Centre 7 Research Work Published or Accepted for Publication 10 Books and In Books 14 Members of Scientific Societies/Committees 15 Ph.D. degree Received 15 Ph.D. Thesis Submitted 15 Course of lectures offered by ICSP members 15 Participation in National/International Conferences & Symposia 16 Workshops / Seminars / Conferences etc. organized 17 Visits abroad from the Centre 17 Major Visitors to the Centre 17 Collaborative Research and Project Work 17 M.Sc. projects guided by ICSP members 18 Summary of the Research Activities of the Scientists at the Centre 19 The ionospheric and earthquake research centre (IERC) 38 Activities of the Indian Centre for Space Physics, Malda Branch 40 Auditors Report to the Members 42 Published by: Indian Centre for Space Physics, Chalantika 43, Garia Station Road, Garia, Kolkata 700084 EPABX +91-33-2436-6003 and +91-33-2462-2153 Extension Numbers: Department of Ionospheric Science: 21 Department of Astrochemistry/Astrobiology: 22 Accounts: 23 Seminar Room: 24 Computer room: 25 Department of High Energy Radiation: 26 X-ray Laboratory: 27 Fax: +91-33-2462-2153 E-mail: [email protected] Website: http://csp.res.in Front Cover: Superposed photos of the earth taken from a camera on board a balloon borne mission and the sky at Ionospheric and Earthquake Research Center of ICSP taken by Mr. -
Electromagnetic Spectrum
Electromagnetic Spectrum Why do some things have colors? What makes color? Why do fast food restaurants use red lights to keep food warm? Why don’t they use green or blue light? Why do X-rays pass through the body and let us see through the body? What has the radio to do with radiation? What are the night vision devices that the army uses in night time fighting? To find the answers to these questions we have to examine the electromagnetic spectrum. FASTER THAN A SPEEDING BULLET MORE POWERFUL THAN A LOCOMOTIVE These words were used to introduce a fictional superhero named Superman. These same words can be used to help describe Electromagnetic Radiation. Electromagnetic Radiation is like a two member team racing together at incredible speeds across the vast regions of space or flying from the clutches of a tiny atom. They travel together in packages called photons. Moving along as a wave with frequency and wavelength they travel at the velocity of 186,000 miles per second (300,000,000 meters per second) in a vacuum. The photons are so tiny they cannot be seen even with powerful microscopes. If the photon encounters any charged particles along its journey it pushes and pulls them at the same frequency that the wave had when it started. The waves can circle the earth more than seven times in one second! If the waves are arranged in order of their wavelength and frequency the waves form the Electromagnetic Spectrum. They are described as electromagnetic because they are both electric and magnetic in nature. -
HF Radio Propagation
Introduction to HF Radio Propagation 1. The Ionosphere 1.1 The Regions of the Ionosphere In a region extending from a height of about 50 km to over 500 km, most of the molecules of the atmosphere are ionised by radiation from the Sun. This region is called the ionosphere (see Figure 1.1). Ionisation is the process in which electrons, which are negatively charged, are removed from neutral atoms or molecules to leave positively charged ions and free electrons. It is the ions that give their name to the ionosphere, but it is the much lighter and more freely moving electrons which are important in terms of HF (high frequency) radio propagation. The free electrons in the ionosphere cause HF radio waves to be refracted (bent) and eventually reflected back to earth. The greater the density of electrons, the higher the frequencies that can be reflected. During the day there may be four regions present called the D, E, F1 and F2 regions. Their approximate height ranges are: • D region 50 to 90 km; • E region 90 to 140 km; • F1 region 140 to 210 km; • F2 region over 210 km. At certain times during the solar cycle the F1 region may not be distinct from the F2 region with the two merging to form an F region. At night the D, E and F1 regions become very much depleted of free electrons, leaving only the F2 region available for communications. Only the E, F1 and F2 regions refract HF waves. The D region is very important though, because while it does not refract HF radio waves, it does absorb or attenuate them (see Section 1.5). -
Critical Thinking Activity: the Electromagnetic Spectrum
Student Sheet 1 CRITICAL THINKING ACTIVITY: THE ELECTROMAGNETIC SPECTRUM There are many kinds of energy in the universe. The energy given off from the sun is radiant energy, scientifically called electromagnetic radiation. Produced by nuclear reactions at the core of the sun, this energy streams from the surface of the sun in waves of different lengths. The shortest and longest wavelengths are invisible to our eyes, but the medium wavelengths are the visible radiation we call sunlight. Most of the sun’s energy is released in these visible wavelengths. All substances have kinetic energy that is expressed by vibrations of their atoms or molecules. The vibrations result in radiation. The electromagnetic (EM) spectrum is a name given to all of the different types of radiation. Electromagnetic radiation is energy that spreads out as it travels. Visible light radiation that comes from a lamp in someone’s house or radio wave radiation that comes from a radio station are two types of electromagnetic radiation. Other examples of EM radiation are microwaves, infrared and ultraviolet radiation, X- rays and gamma rays. Hotter, more energetic objects and events create higher energy radiation than cool objects. Only extremely hot objects or particles moving at very high speeds can create high-energy radiation like X-rays and gamma rays. 1 Student Sheet 2 A common assumption is that radio waves are completely different than X-rays and gamma rays. They are produced in very different ways, and we detect them in different ways. However, radio waves, visible light, X-rays, and all the other parts of the electromagnetic spectrum are fundamentally the same. -
Time and Frequency Users' Manual
,>'.)*• r>rJfl HKra mitt* >\ « i If I * I IT I . Ip I * .aference nbs Publi- cations / % ^m \ NBS TECHNICAL NOTE 695 U.S. DEPARTMENT OF COMMERCE/National Bureau of Standards Time and Frequency Users' Manual 100 .U5753 No. 695 1977 NATIONAL BUREAU OF STANDARDS 1 The National Bureau of Standards was established by an act of Congress March 3, 1901. The Bureau's overall goal is to strengthen and advance the Nation's science and technology and facilitate their effective application for public benefit To this end, the Bureau conducts research and provides: (1) a basis for the Nation's physical measurement system, (2) scientific and technological services for industry and government, a technical (3) basis for equity in trade, and (4) technical services to pro- mote public safety. The Bureau consists of the Institute for Basic Standards, the Institute for Materials Research the Institute for Applied Technology, the Institute for Computer Sciences and Technology, the Office for Information Programs, and the Office of Experimental Technology Incentives Program. THE INSTITUTE FOR BASIC STANDARDS provides the central basis within the United States of a complete and consist- ent system of physical measurement; coordinates that system with measurement systems of other nations; and furnishes essen- tial services leading to accurate and uniform physical measurements throughout the Nation's scientific community, industry, and commerce. The Institute consists of the Office of Measurement Services, and the following center and divisions: Applied Mathematics -
Gamma Ray Bursts
An Information & Activity Booklet Grades 5-8 1999-2000 StarChild - a Learning Center for Young Astronomers EG-1999-08-001-GSFC WRITTEN BY: Dr. Elizabeth Truelove and Mrs. Joyce Dejoie Lakeside Middle School Evans, Georgia This booklet, along with its matching poster, is meant to be used in conjunction with the StarChild Web site or CD-ROM. http://starchild.gsfc.nasa.gov/ TABLE OF CONTENTS Table of Contents...................................................................................................................i Association with National Mathematics and Science Standards.............................................ii Preface.................................................................................................................................. 1 Introduction to Gamma-Ray Bursts (GRBs).......................................................................... 2 Level 2 Activities Related to Gamma-Ray Bursts.................................................................. 5 A Timely Matter........................................................................................................ 5 Electromagnetic Notation .......................................................................................... 7 Telescopic Trivia....................................................................................................... 9 From Billions to Nonillions ..................................................................................... 10 High-Energy Word Search...................................................................................... -
IJEST Template
Research & Reviews: Journal of Space Science & Technology ISSN: 2321-2837 (Online), ISSN: 2321-6506 V(Print) Volume 6, Issue 2 www.stmjournals.com Diurnal Variation of VLF Radio Wave Signal Strength at 19.8 and 24 kHz Received at Khatav India (16o46ʹN, 75o53ʹE) A.K. Sharma1, C.T. More2,* 1Department of Physics, Shivaji University, Kolhapur, Maharashtra, India 2Department of Physics, Miraj Mahavidyalaya, Miraj, Maharashtra, India Abstract The period from August 2009 to July 2010 was considered as a solar minimum period. In this period, solar activity like solar X-ray flares, solar wind, coronal mass ejections were at minimum level. In this research, it is focused on detailed study of diurnal behavior of VLF field strength of the waves transmitted by VLF station NWC Australia (19.8 kHz) and VLF station NAA, America (24 kHz). This research was carried out by using VLF Field strength Monitoring System located at Khatav India (16o46ʹN, 75o53ʹE) during the period August 2009 to July 2010. This study explores how the ionosphere and VLF radio waves react to the solar radiation. In case of NWC (19.8 kHz), the signal strength recording shows diurnal variation which depends on illumination of the propagation path by the sunlight. This also shows that the signal strength varies according to the solar zenith angle during daytime. In case of VLF signal transmitted by NAA at 24 kHz, the number of sunrises and sunsets are observed in VLF signal strength due to the variations of illumination of the D-region during daytime. In both the cases, the signal strength is more stable during daytime and fluctuating during nighttime due to the presence and absence of D-region during daytime and nighttime respectively. -
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IEICE Communications Express, Vol.6, No.6, 405–410 Performance enhancement by beam tilting in SD transmission utilizing two-ray fading Tomohiro Seki1a), Ken Hiraga2, Kazumitsu Sakamoto2, and Maki Arai2 1 College of Industrial Technology, Department of Electrical and Electronic Engineering, Nihon University, 1–2–1 Izumicho, Narashino 275–8575, Japan 2 NTT Network Innovation Laboratories, NTT Corporation, 1–1 Hikarinooka, Yokosuka 239–0847, Japan a) [email protected] Abstract: A method is proposed for enhancing the transmission perform- ance in a spatial division transmission system that utilizes the fading characteristics of two-ray ground reflection propagation. The method is tilting the elevation angle of antenna beams purposely towards out of the communicating peer. Using ray-tracing simulation, it is shown that the performance of the system is significantly improved when high-gain anten- nas with narrow beamwidth are used. Keywords: two-ray fading, parallel transmission Classification: Antennas and Propagation References [1] K. Hiraga, K. Sakamoto, M. Arai, T. Seki, T. Nakagawa, and K. Uehara, “Spatial division transmission without signal processing for MIMO detection utilizing two-ray fading,” IEICE Trans. Commun., vol. E97.B, no. 11, pp. 2491–2501, 2014. DOI:10.1587/transcom.E97.B.2491 [2] C. Cordeiro, “IEEE doc.:802.11-09/1153r2,” p. 4, 2009. [3] Wilocity: Wil6200 Chipset Datasheet. [Online]. http://wilocity.com/resources/ Wil6200-Brief.pdf. [4] W. L. Stutzman, “Estimating directivity and gain of antennas,” IEEE Antennas Propag. Mag., vol. 40, no. 4, pp. 7–11, Aug. 1998. DOI:10.1109/74.730532 [5] D. Parsons, The Mobile Radio Propagation Channel, ch. -
Theory on the Propagation of UHF Radio Waves in Coal Mine Tunnels
Theory of the Propagation of UHF Radio Waves in Coal Mine Tunnels ALFRED G. EXSLIE, ROBERT L. LAGACE, MEMBER, IEEE, AND PETER F. STRONG Abstract-The theoretical study of WFradio communication in coal mines, with particular reference to the rate of loss of signal strength along a tunnel, and from one tunnel to another around a comer is the concern of this -paper. - Of prime interest are the nature ....... .......-.. of the propagation mechanism and the prediction of the radio ....... ...... frequency that propagates with the smallest loss. The theoretical results are compared with published measurements. This work was Fig. 1. Wave guide geometry. part of an investigation of new ways to reach and extend two-way communications to the key individuals who are highly mobile within the sections and haulageways of coal mines. ~orkby AIarcatili and Schmeltzer r2] and by Glaser [3], which applies to waveguides of circular and parallel-plate INTRODUCTION geometry in a medium of uniform dielectric constant. We present in the body of the paper the main features of the T FREQUENCIES in the range of 200-4000 MHz propagation of UHF waves in tunnels. Details of the A the rock and coal bounding a coal mine tunnel act as derivations are contained in the accompanying appendices. relatively low-loss dielectrics with dielectric constants in the range 5-10. Under these conditions a reasonable THE FUXDARIEXTAL (1,l) WAVEGUIDE MODES hypothesis is that transmission takes the form of wave- guide propagation in a tunnel, since the wavelengths of The propagation modes with the lowest attenuation the UHF waves are smaller than the tunnel dimensions.