A History of Vertical-Incidence Ionsphere Sounding at the National
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Planetary Challenges & Spiritual Evolution
Planetary Challenges & Spiritual Evolution – Citizen Summary Planetary Challenges & Spiritual Evolution Summary For Citizens of Planet Earth Written by Susan Joy Rennison, B. Sc Hons (Physics & Geophysics), June 2011 (Editorial Revision), Olten, Switzerland Copyright © 2011 Susan Joy Rennison Planetary Challenges & Spiritual Evolution – Citizen Summary Planetary Challenges & Spiritual Evolution Citizen Summary Table of Contents Table of Contents i Illustrations ii Foreword iv Introduction vii Our Sun, A Variable Star 1 The Extraordinary Quiet Solar Minimum of Solar Cycle 23 2 Space Weather & The Delivery of Evolutionary Energies 4 The Precession of the Equinoxes 5 Extreme Space Weather 6 The Gamma & Cosmic Ray Blitz From Across the Galaxy 8 The Global Warming Controversy 9 Atmospheric Change: New Electrical Manifestations 10 Extreme Physics right here on Earth 12 Asteroids, Comets & Meteors? “We’re living in a bowling alley” 13 Heavenly Phenomena: Strange Fireballs 16 The Geological Response 17 Strange Atmospheric Cloud Emissions 19 The ‘Orb’ Phenomena & ‘Diamond’ Rain 20 Earth’s Shadow Biosphere 21 The Planetary ‘Refresh’ 27 i Copyright Susan Joy Rennison Sunday, June 05, 2011 Planetary Challenges & Spiritual Evolution – Citizen Summary The ‘Upgrade’ of the Planetary Grid 31 Space Weather Drives Biological Changes 32 The Choice: Spiritual Evolution or Devolution? 33 Rapid Evolutionary Change 34 Conclusion 38 References 39 Illustrations The White House i Medieval Engraving of Gioacchino da Fiore (Joachim of Fiore) vi Space Weather Turns Into an International Problem vii The Sun −Earth Connection viii Aurora over Southern New Jersey (1989) ix Exploration of Near Earth Objects Workshop Poster x The Eventful Universe Workshop Poster xi Massive Coronal Mass Ejection Proceeding X45 Solar Flare. -
Ionospheric Radars Development
UNT Ionospheric radars development Enrico Zuccheretti, Umberto Sciacca [email protected] - [email protected] Istituto Nazionale di Geofisica e Vulcanologia - Rome, Italy The following slides were presented during the lectures of the course “Desarrollo de radares ionosféricos” held within the post graduate course on “Geofísica espacial” organised by the Universidad Nacional de Tucumán - Facultad de Ciencias Exactas y Tecnología - Departamento de Posgrado in Tucumán on 4 – 7 October 2010. UNT Module 1 Basics of radar theory and design elements Introduction UNT •Amongst the big variety of techniques used to study the geophysical environment, methods using electromagnetic waves occupy a very prominent position. •These techniques exploit radio waves modifications when they interact with the medium they pass through. •The ionosphere is no exception: the most common way to study its behaviour is to emit radio wave pulses into the ionosphere and to study the backscattered echo. •The echo signal contains information about the layers in which it may be refracted, reflected or absorbed. •Also signals coming from satellites (NNSS, GPS) or from terrestrial emitting station (VLF emitters) can be used. They do not exploit the radar technique but their properties are affected by the medium they pass through. Radio Frequencies Bands UNT ELF SLF ULF VLF LF MF HF VHF UHF SHF EHF 3 Hz 30 Hz 300 Hz 3 kHz 30 kHz 300 kHz 3 MHz 30 MHz 300 MHz 3 GHz 30 GHz 30 Hz 300 Hz 3 kHz 30 kHz 300 kHz 3 MHz 30 MHz 300 MHz 3 GHz 30 GHz 300 GHz The vertical sounding technique UNT •The measure technique is based on sending pulses of energy at different frequencies towards the ionosphere and in measuring the backscattered echo delay to properly evaluate the position of ionospheric layers. -
Chapter 8 Propagation
General License Class 1 General Class Chapter 8 Propagation 2 1 The Ionosphere Regions • Ionosphere. • The ionosphere is a portion of the atmosphere that extends from about 30 miles to about 300 miles above the surface of the Earth. • The ionosphere reaches its highest altitude when the sun is directly overhead. • Solar radiation causes atoms in the ionosphere to become ionized. 3 The Ionosphere Regions • Ionosphere. • The ionosphere organizes itself into regions or “layers”. • The layers vary with the strength of the ionization. • The D-region disappears at night. • The F-region splits into F1 & F2 regions during the day. 4 2 The Ionosphere Regions • D-Layer. • 30-60 miles altitude. • Rapidly disappears at sunset. • Rapidly re-forms at sunrise. • Absorbs long wavelength radio waves. • 160m, 80m, & 40m. 5 The Ionosphere Regions • E-Layer. • 60-70 miles altitude. • One hop up to 1200 miles. • Similar to the D-layer. • The E-layer lasts longer into the night than the D-layer. • The E-layer has less absorption than the D-layer. 6 3 The Ionosphere Regions • E-Layer. • The E-layer is where the following types of propagation occur: • Auroral propagation. • Sporadic-E skip. • 10m, 6m, & 2m. • Meteor Scatter. 7 The Ionosphere Regions • F-Layer. • 100-300 miles altitude. • One-hop up to 2500 miles. • During periods of high sunspot activity, the F-layer can remain ionized all night. 8 4 The Ionosphere Regions • F-Layer. • The F-layer splits into the F1- layer & the F2-layer during the day. • F1-layer = 100-140 miles. • F2-layer = 200-300 miles. -
Chapter 10 IONOSPHERICRADIO WAVE PROPAGATION Section 10.1 S
Chapter 10 IONOSPHERICRADIO WAVE PROPAGATION Section 10.1 S. Basu, J. Buchau, F.J. Rich and E.J. Weber Section 10.2 E.C. Field, J.L. Heckscher, P.A. Kossey, and E.A. Lewis Section 10.3 B.S. Dandekar Section 10.4 L.F. McNamara Section 10.5 E.W. Cliver Section 10.6 G.H. Millman Section 10.7 J. Aarons and S. Basu Section 10.8 J.A. Klobuchar Section 10.9 J.A. Klobuchar Section 10.10 S. Basu, M.F. Mendillo The series of reviews presented is an attempt to introduce in HF communications is leading to a rejuvenation of the ionospheric radio wave propagation of interest to system global ionosonde network. users. Although the attempt is made to summarize the field, the individuals writing each section have oriented the work 10.1.1.1 Ionogram. Ionospheric sounders or ionosondes in the direction judged to be most important. are, in principle, HF radars that record the time of flight or We cover areas such as HF and VLF propagation where travel of a transmitted HF signal as a measure of its ionos- the ionosphere is essentially a "black box", that is, a vital pheric reflection height. By sweeping in frequency, typically part of the system. We also cover areas where the ionosphere from 0.5 to 20 MHz, an ionosonde obtains a meas- is essentially a nuisance, such as the scintillations of trans- urement of the ionospheric reflection height as a function ionospheric radio signals. of frequency. A recording of this reflection height meas- Finally, we have included a summary of the main fea- urement as a function of frequency is called an ionogram. -
A Simplified Mathematical Model to Calculate the Maximum Usable Frequencies Over Iraqi Territory Khalid A
A Simplified Mathematical Model to Calculate the Maximum Usable Frequencies Over Iraqi Territory Khalid A. Hadi*, Loay E. Goerge** A Simplified Mathematical Model to Calculate the Maximum Usable Frequencies Over Iraqi Territory Khalid A. Hadi*, Loay E. Goerge** * Department of Astronomy & Space, College of Science, University of Baghdad ** Department of Computer Science, College of Science, University of Baghdad Receiving Date: 25-02-2011 - Accept Date: 13-06-2011 Abstract In this project, the spatial and temporal variation of maximum usable frequency (MUF) parameter is investigated and modeled. The values of MUF for Baghdad station links, with other stations distributed over Iraq territory, where determined using the international reference model (RECF533) for HF propagation. The determined MUF dataset reflected that the spatial distribution of this parameter for Baghdad station shows circular symmetry, which stimulated the possibility of using a two dimensional second order polynomial in order to describe MUF variation. The main feature of this adopted mathematical model is its low complexity. The results of conducted analysis indicated that the spatial variation of MUF is simple while its temporal variation is more complicated and needs more sophisticated mathematical description than the polynomial description. The test results showed that the accuracy of proposed simple model lies within the tolerance of REC533 reference model. Key words: Ionosphere, HF communication prediction, MUF Vol 7 No: 4, October 2011 1 20 ISSN: 2222-8373 A Simplified Mathematical Model to Calculate the Maximum Usable Frequencies Over Iraqi Territory 1. INTRODUCTION The Maximum Usable Frequency, denoted by MUF, is an important ionospheric parameter. It is defined as the highest frequency that allows reliable long-range high frequency (HF) radio communication between two points due to ion-ospheric refraction. -
Vhf-Uhf Digest E-Zine Version
The Worldwide TV-FM DX Association Serving the VHF-UHF Enthusiast VHF-UHF DIGEST E-ZINE VERSION MARCH 2002 The VHF-UHF Digest is the official publication of the Worldwide TV-FM DX Association dedicated to the observation and study of the propagation of long distance television and FM broadcasting signals at VHF and UHF. The WTFDA is governed by a board of directors: TOM BRYANT, GREG CONIGLIO, BRUCE HALL, DAVE JANOWIAK AND MIKE BUGAJ. WHEN IS YOUR MEMBERSHIP UP? CONTENTS In order to keep your VUD arriving at your Page Two home without interruption, look for your name Mailbox on this list. Your membership ends on the last FM News. ..Greg Coniglio day of the month shown. Renew early! TV News...Doug Smith Western TV DX...Victor Frank March Eastern TV DX…Matt Sittel Edward Cotton Aaron Mitterling Bill Draeb Gerard Hart Southern FM DX…John Zondlo Bill Dvorak Thomas Leu Photo News…Jeff Kruszka Pat Dyer Jim Pizzi TV Statistics…Fred Nordquist Carlon Howington Joseph Smith Jr Northern FM DX…Keith McGinnis Scott Steenhusen Richard Steinberger Satellite News…George Jensen Phil Sullivan Peter V. Taylor Mid-Latitude SpE Part III…Mike Hawk David Cox Allan Dunn CA Highway Patrol Freqs Frank Drobny Dave Nieman Sign-up/Renewal Form and addresses Ryan Grabow William Hepburn Paul Crego Luis Franceschi Joseph Kureth Jr. Alex Cruz This month we continue with Mike Hawk’s April article on Sporadic E. We also provide a list for Eric Fader John Hourigan those of you interested in 42mhz skip of CHP Dan Oetting William Thompson frequencies that includes each office’s ID Larry Weisberg James Ivil number. -
Using High Frequency Propagation to Calculate Basic Maximum Usable Frequency
Using High Frequency Propagation to Calculate Basic Maximum Usable Frequency Israa Abdualqassim Mohammed Ali* * University of Baghdad, College of Science, Baghdad, Iraq Received: XX 20XX / Accepted: XX 20XX / Published online: ABSTRACT A comparison between observed (obs.) digital ionospheric sounding data and predicted (pre.) using International Reference Ionosphere (IRI) model for critical frequency (foF2) and Basic Maximum Usable Frequency (BMUF) of ionospheric F2-Layer has been made. A mid-latitude region selected for this research work by using data from station Wakkanai (45.38o N, 141.66o E). This study included 12 monthly median data from year (2001, R12=111) selected for high Sunspot number (SSN) and years for low SSN (2004, R12=44) and (2005, R12=29). Frequency parameters foF2 reveals that there is a good correlation between observed and predicted except for January of years 2001 and 2004, and BMUF revealed that there is a good correlation between observed and predicted for years of low SSN and all months except in month 1, 9 and 12 of year 2004, for year 2001 of high SSN there is a bad correlation. A correction factor as a function of time used from fitting technique to correct the predicted value with observed value of BMUF for year 2001. Keywords: Ionosphere; foF2; M3000F2; BMUF Author Correspondence, e-mail: [email protected] 1. INTRODUCTION The maximum usable frequency (MUF) is important ionospheric parameter for radio users because of its role in radio frequency management and for providing a good communication 1 link between two locations (Athieno et al., 2015; Suparta et al., 2018). -
Radio Wave Propagation References
RADIO WAVE PROPAGATION REFERENCES “Almost Everything You Need to Know…”: Chapter 7: 53-68 “RAC Basic Study Guide 6th Ed:” 6.2, 6.3, 6.4, 6.5, 6.6, 6.8, 6.9, 6.10 “RAC Operating Manual 2nd Ed:” “The ARRL Handbook For Radio Amateurs 2001,78thEd:” Chapter 21: 1-37 "Radio Propagation" Wikipedia, The Free Encyclopedia. 6 Nov 2007 http://en.wikipedia.org/ “Chelmsford Amateur Radio Society” Intermediate Course (5) Antennas and Feeders TOC: •INTRO •RADIO WAVES •POLARIZATION •LINE OF SIGHT, GROUND & SKY WAVES •IONOSPHERE REGIONS •IONOSPHERIC LAYERS •PROPAGATION, HOPS, SKIPS ZONES •ABSORPTION AND FADING •SOLAR ACTIVITY AND SUN SPOTS •MF, HF CRITICAL FREQUENCIES •UHF, VHF, SPORADIC E, AURORAS, DUCTING •SCATTER, HF, VHF,UHF Major General Urquhart: “My communications are completely broken down. Do you •BEACONS really believe any of that can be helped by a cup of tea?” •SAMPLE QUESTIONS Corporal Hancock: “Couldn't hurt, sir” -Arnhem 1944 PROPAGATION - INTRO Propagation: How radio waves travel from point A to point B; and the events occurring in the transmission path that affect the communications between the points, stations, or operators. When the electrons in a conductor, (antenna wire) are made to oscillate back and forth, Electromagnetic Waves (EM waves) are produced. These waves radiate outwards from the source at the speed of light, 300 million meters per second. Light waves (waves we see) and radio waves (waves we hear)are both EM waves, differing only in frequency and wavelength. PROPAGATION – INTRO CONT’D EM waves travel in straight lines, unless acted upon by some outside force. They travel faster through a vacuum than through any other medium. -
Introductionto the Ionoshpereand Geomagnetism
N6517513 INTRODUCTION TO THE IONOSHPERE AND GEOMAGNETISM OCT 1964 SEL-64-111 INTRODUCTION TO THE IONOSPHERE AND GEOMAGNETISM by H. Rishbeth and O. K. Garriott October 1964 Reproduction in whole or in part is permitted for any purpose of the United States Government. Technical Report No. 8 Prepared under National Aeronautics and Space Administration Grant NsG 30-60 Radioscience Laboratory Stanford Electronics Laboratories Stanford University Stanford, California CONTENTS -=_:_!-_¸ Paze I. THE NEUTRAL ATMOSPHERE .................. 1 I. Atmospheric Nomenclature ............... 1 2. Evolution of the Earth's Atmosphere ......... 5 3. Structure of the Atmosphere ............. 7 4. Dissociation and Diffusive Separation ........ 12 5. Thermal Balance ................... 16 6. The Exosphere .................... 2O __J, 7. Experimental Techniques ............... 21 II. MEASUREMENT OF IONOSPHERIC PARAMETERS .......... 27 I. Introduction ..................... 27 2. Determination of Electron Density by Sounding .... 27 3, Propagation Methods ................. 36 4. Direct Measurements ................. 44 z, 5. Incoherent Scatter .................. 46 III. PROCESSES IN THE IONOSPHERE ............... 50 I. The Balance of Ionization .............. 50 2. Chapman's Theory ................... 53 3. Production and Loss ................. 63 4. The D, E and F1 Photochemical Regime ....... 69 5. Plasma Diffusion ................... 81 6. Solving the Continuity Equation ........... 88 IV. MORPHOLOGY OF THE IONOSPHERE 94 1. D Region .................... 94 2. -
Radio Transmission and the Ionosphere
Ih S. DEPARTMENT OF COMMERCE NATIONAL BUREAU OF STANDARDS WASHINGTON / » ruT O v / Letter Circular LC-614 RADIO TRANSMISSION AND THE IONOSPHERE October 23, 19^0 6 . s TKD :ANK U. 3. DEPARTMENT OF COMMERCE Letter 1-6 NATIONAL BUREAU OF STANDARDS Circular Washington LC-6l4 ( Supersedes LC-E75) October 23 , 19^0 RADIO TRANSMISSION' AND THE IONOSPHERE Radio transmission over great distances is made possible by . reflection of the radio waves from ionized (electrically conduct- ing) layers in the ionosphere, the upper region of the earth* atmosphere. How far the radio waves go, and what frequencies may be used, are determined by the heights and the degree of ionization of the ionized layers, which are located between about BO kilometers (30 miles) and 400 kilometers (250 miles) above the earth's surface. Because of variations in the ionized layers, the conditions of radio wave transmission vary with time of day, with season, and from year to year. For the efficient maintenance of radio services it is important to have a constant supply of information on these changes. To this end an ionosphere observing, reporting, and predicting service is provided by the National Bureau of Standards. It is analogous to the weather reporting service, though quite independent of it-; the factors producing or affecting weather exist at much lower levels of the atmosphere than the ionosphere. The results of the Bureau * work on the ionosphere arid -radio transmission are made available to the public by a Science Service Urslgram and radio broadcast each week, and regular publication each month and each quarter, as well as through special papers (see References at end hereof) published from time to time on particular phases of the subject. -
Radio Communications
RADIO COMMUNICATIONS An Amateur Radio Technician and General Class License Study Guide Prepared by John Nordlund – AD5FU and Edited by Lynette Dowdy - KD5QMD Based on the Element 2 Technician Exam Question Pool Valid from 7/1/06 until 7/1/2010 and the Element 3 General Exam Question Pool Valid 7/1/2007 until 7/1/2011 Page 1 of 78 Acknowledgment: My greatest thanks to Lynette – KD5QMD, for her understanding and assistance, without which this book would be filled with countless typographical and grammatical errors and an overload of confusing jargon and bewildering techno-babble. | | This publication is the intellectual property of the author, and may not be reproduced for commercial gain for any purpose without the express permission of the author. | | However, Share the Fun. | | This publication may be freely distributed for the educational benefit of any who would care to obtain or upgrade their amateur radio license. | | | If you love the hobby you have a duty of honor to pass it along to the next generation. | | | 73 de AD5FU Page 2 of 78 How to use this study guide. Contained within the next 73 pages is a text derived from the official exam question pools for Element 2 Technician and Element 3 General class exams. It is the expressed opinion of the author and editor of this study guide that studying the full question pool text is counterproductive in attempting to obtain your Amateur Radio License. We therefore do not recommend downloading the actual exam question pool texts. This study guide is divided into sections of related information. -
Midlatitude D Region Variations Measured from Broadband Radio Atmospherics
MIDLATITUDE D REGION VARIATIONS MEASURED FROM BROADBAND RADIO ATMOSPHERICS by Feng Han Department of Electrical and Computer Engineering Duke University Date: Approved: Steven A. Cummer, Advisor David R. Smith Qing H. Liu William T. Joines Thomas P. Witelski Dissertation submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in the Department of Electrical and Computer Engineering in the Graduate School of Duke University 2011 Abstract (Electrical and Computer Engineering) MIDLATITUDE D REGION VARIATIONS MEASURED FROM BROADBAND RADIO ATMOSPHERICS by Feng Han Department of Electrical and Computer Engineering Duke University Date: Approved: Steven A. Cummer, Advisor David R. Smith Qing H. Liu William T. Joines Thomas P. Witelski An abstract of a dissertation submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in the Department of Electrical and Computer Engineering in the Graduate School of Duke University 2011 Copyright c 2011 by Feng Han All rights reserved except the rights granted by the Creative Commons Attribution-Noncommercial Licence Abstract The high power, broadband very low frequency (VLF, 3{30 kHz) and extremely low frequency (ELF, 3{3000 Hz) electromagnetic waves generated by lightning dis- charges and propagating in the Earth-ionosphere waveguide can be used to measure the average electron density profile of the lower ionosphere (D region) across the wave propagation path due to several reflections by the upper boundary (lower iono- sphere) of the waveguide. This capability makes it possible to frequently and even continuously monitor the D region electron density profile variations over geograph- ically large regions, which are measurements that are essentially impossible by other means.