Introduction to Mobile Radio Propagation and Characterization of Frequency Bands
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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. -
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. -
Regulation on Collective Frequencies for Licence-Exempt Radio Transmitters and on Their Use
FICORA 15 AIH/2015 M 1 (22) Unofficial translation Regulation on collective frequencies for licence-exempt radio transmitters and on their use Issued in Helsinki on 6 February 2015 The Finnish Communications Regulatory Authority (FICORA) has, under section 39(3 and 4) of the Information Society Code of 7 November 2014 (917/2014), laid down: Chapter 1 General provisions Section 1 The oObjective of the Regulation This Regulation lays down provisions on collective frequencies for as well as use and registration of such radio transmitters whose conformity with requirements has been attested in such a way as laid down in the Information Society Code, and for the possession and use of which a radio licence is not required. Section 2 Scope of application This Regulation applies to the following radio transmitters which operate only on the collective frequencies assigned in this Regulation and whose conformity with requirements has been attested in such a way as mentioned in section 257 or section 352 of the Information Society Code: 1) cordless CT1 telephones taken into use on 31 December 2003 at the latest, cordless CT2 telephones taken into use on 31 December 2004 at the latest, and DECT equipment; 2) mobile terminals and other terminals for GSM, UMTS, digital broadband mobile networks and terrestrial systems capable of providing electronic communications services; 3) LA telephones (national Citizen Band equipment) which have been approved according to the regulations of 25 March 1981 by the General Directorate of Posts and Telecommunications -
Antennas for 136Khz Index
ON7YD, longwave, 136kHz, antennas Page 1 of 51 ON7YD Antennas for 136kHz About this page : The main object of this page is to provide information. It has been deliberately kept simple, no fancy and flashy tricks, in order to achieve maximum compatibility for the different browsers and to allow fast downloading. Any comments and/or suggestions are welcome at : [email protected] last updated on 8 July 2004 Index 1. Introduction 2. Short vertical antennas 1. Vertical monopole antenna 2. Short vertical monopole 3. Vertical antenna with capacitive toploading 4. Umbrella antenna 5. Capacitive toploading of single-tower antennas 6. Spiral toploaded antenna 7. Vertical antenna with inductive toploading 8. Vertical antenna with capacitive and inductive toploading 9. Vertical antenna with tuned counterpoise 10. Meander antenna 11. Antenna with multiple vertical elements 12. Using a non isolated antenna-tower as LF-antenna 13. Antennas with a long horizontal section 14. Helical antenna 15. Short vertical dipole 16. Why a horizontal dipole is a rather unefficient antenna on LF 17. Safety precautions 18. Bringing a short vertical monopole to resonance 1. Loading coil 2. Coil losses : the Q-factor 3. Variometer 4. Tapped coil 5. Impedance matching 6. Bandwidth considerations 3. Efficiency of antenna systems on LF (short vertical antennas) 1. Antenna system 2. Efficiency 3. Antenna system efficiency, antenna directivity, ERP, EIRP and EMRP 4. Optimizing the antenna system efficiency 5. Enviromental losses 6. Ground loss 1. Type (composition) of the soil 2. Frequency 3. Shape and dimensions of the antenna 4. Radial system and ground rods 4. Measuring ERP on LF http://www.qsl.net/on7yd/136ant.htm 12/19/2006 ON7YD, longwave, 136kHz, antennas Page 2 of 51 1. -
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). -
The Transatlantic on 2200 Meters
The Transatlantic on 2200 Meters Joe Craig, VO1NA and Alan Melia, G3NYK here has been much excite- ment below our so-called top Longing for the days when amateurs built band at 1.8 MHz. At less than T one-tenth this frequency, near their own gear and DX was big news? 136 kHz, you will find many amateurs en- joying QSOs using a variety of modes. Al- They’re back again...on the “top” top band. though US and Canadian amateurs need special permission to transmit here, there is a 2200 meter amateur band in many pared with the thickness (about 30 km) of in north Nova Scotia. Other, regularly heard European countries and in New Zealand. the daytime absorbing D-layer. Unlike HF calls in the early days of tests was the well Aside from its low frequency, the most strik- frequencies, LF has a substantial ground- known MF station of Jack, VE1ZZ and the ing thing about the 135.8-138.8 kHz band is wave service area, with the wave front being late Larry Kayser, VA3LK. its narrow width—only 2.1 kHz, barely wide bent to follow the curvature of the Earth to Daytime propagation is mainly ground enough to admit a single SSB transmission. some extent. In daytime, there is an absorb- wave, but at extreme range (in excess of Huge sources of interference are present ing ionized region, formed by photo-disso- 1500 km) there is a significant daytime in the band. In Greece, the Navy transmitter ciation, which corresponds to the D-layer ionospheric component. -
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 -
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. -
Etsi En 302 208 V3.1.1 (2016-11)
ETSI EN 302 208 V3.1.1 (2016-11) HARMONISED EUROPEAN STANDARD Radio Frequency Identification Equipment operating in the band 865 MHz to 868 MHz with power levels up to 2 W and in the band 915 MHz to 921 MHz with power levels up to 4 W; Harmonised Standard covering the essential requirements of article 3.2 of the Directive 2014/53/EU 2 ETSI EN 302 208 V3.1.1 (2016-11) Reference REN/ERM-TG34-264 Keywords harmonised standard, ID, radio, RFID, SRD ETSI 650 Route des Lucioles F-06921 Sophia Antipolis Cedex - FRANCE Tel.: +33 4 92 94 42 00 Fax: +33 4 93 65 47 16 Siret N° 348 623 562 00017 - NAF 742 C Association à but non lucratif enregistrée à la Sous-Préfecture de Grasse (06) N° 7803/88 Important notice The present document can be downloaded from: http://www.etsi.org/standards-search The present document may be made available in electronic versions and/or in print. The content of any electronic and/or print versions of the present document shall not be modified without the prior written authorization of ETSI. In case of any existing or perceived difference in contents between such versions and/or in print, the only prevailing document is the print of the Portable Document Format (PDF) version kept on a specific network drive within ETSI Secretariat. Users of the present document should be aware that the document may be subject to revision or change of status. Information on the current status of this and other ETSI documents is available at https://portal.etsi.org/TB/ETSIDeliverableStatus.aspx If you find errors in the present document, please send your comment to one of the following services: https://portal.etsi.org/People/CommiteeSupportStaff.aspx Copyright Notification No part may be reproduced or utilized in any form or by any means, electronic or mechanical, including photocopying and microfilm except as authorized by written permission of ETSI. -
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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. -
Low RF Power Harvesting Circuit for Wireless Sensor Nodes in Industrial Plants
Low RF Power Harvesting Circuit for Wireless Sensor Nodes In Industrial Plants Issam Chaour∗† Olfa Kanoun∗ and Ahmed Fakhfakh† ∗Chair for Measurement and Sensor Technology, Technische Universitat¨ Chemnitz , GERMANY †National Engineering School of Sfax, University of Sfax, Sfax, TUNISIA Email: [email protected] Abstract—Techniques and methods of energy harvesting are developed to recuperate energy coming from the ambiance to be transmitted to electronic systems. Energy should be useful in specific applications, to generate a certain voltage level and make capable of delivering a recommended Power to the load. So, the main challenge for energy harvesting is to obtain a significant amount of power efficiently from the environment. This paper describes an overview of power transfer systems and methods of charging low power sensors in industrial plants using harvested RF signals. It introduces a scheme investigation of the RF harvester consisting of receiver antenna and a rectifier circuit to convert the RF signal to DC voltage. Low power consumption Fig. 1. System diagram for RF energy harvesting sensor application. circuits are used to achieve the target of highest conceivable efficiency in order to produce the maximum power transfer. Index Terms—RF Energy Harvesting; wireless sensor network; RF power transmission; industrial plants. or microwave energy [3]. In this paper, we explore a potential method to this challenges for recharging wireless sensor nodes I. INTRODUCTION by RF Power transmission and harvesting energy from RF ambient sources. The transmitted RF energy is captured by Many wireless sensor node architectures are adopted for use a receiver antenna, transformed into microwatts (µW) to low in a wireless access point, listen and control system.