Chapter 10 IONOSPHERICRADIO WAVE PROPAGATION Section 10.1 S
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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. -
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. -
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. -
Of Airglow Associated with Medium-Scale Traveling Ionospheric Disturbance
PUBLICATIONS Journal of Geophysical Research: Space Physics RESEARCH ARTICLE Mesoscale field-aligned irregularity structures (FAIs) 10.1002/2014JA020944 of airglow associated with medium-scale traveling Key Points: ionospheric disturbances (MSTIDs) • An evolution of medium-scale traveling ionospheric disturbances Longchang Sun1,2, Jiyao Xu1, Wenbin Wang3, Xinan Yue4, Wei Yuan1, Baiqi Ning5, Donghe Zhang6, (MSTIDs) is presented 1 • Mesoscale field-aligned irregularity and F. C. de Meneses structures (FAIs) (~150 km) of airglow 1 are firstly presented State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, China, • We first find the mesoscale FAIs had a 2Graduate University of the Chinese Academy of Sciences, Beijing, China, 3High Altitude Observatory, National Center for northwestward relative velocity to Atmospheric Research, Boulder, Colorado, USA, 4COSMIC Program Office, University Corporation for Atmospheric Research, main-body MSTIDs Boulder, Colorado, USA, 5Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China, 6Department of Geophysics, Peking University, Beijing, China Correspondence to: fi L. Sun, Abstract In this paper, we report the evolution (generation, ampli cation, and dissipation) of optically [email protected] observed mesoscale field-aligned irregularity structures (FAIs) (~150 km) associated with a medium-scale traveling ionospheric disturbance (MSTID) event. There have not been observations of mesoscale FAIs of Citation: airglow before. The mesoscale FAIs were generated in an airglow-depleted front of southwestward propagating Sun, L., J. Xu, W. Wang, X. Yue, W. Yuan, MSTIDs that were simultaneously observed by an all-sky imager, a GPS monitor, and a digisonde around B. Ning, D. Zhang, and F. C. de Meneses Xinglong (40.4°N, 30.5° magnetic latitude), China, on 17/18 February 2012. -
INDIA JANUARY 2018 – June 2020
SPACE RESEARCH IN INDIA JANUARY 2018 – June 2020 Presented to 43rd COSPAR Scientific Assembly, Sydney, Australia | Jan 28–Feb 4, 2021 SPACE RESEARCH IN INDIA January 2018 – June 2020 A Report of the Indian National Committee for Space Research (INCOSPAR) Indian National Science Academy (INSA) Indian Space Research Organization (ISRO) For the 43rd COSPAR Scientific Assembly 28 January – 4 Febuary 2021 Sydney, Australia INDIAN SPACE RESEARCH ORGANISATION BENGALURU 2 Compiled and Edited by Mohammad Hasan Space Science Program Office ISRO HQ, Bengalure Enquiries to: Space Science Programme Office ISRO Headquarters Antariksh Bhavan, New BEL Road Bengaluru 560 231. Karnataka, India E-mail: [email protected] Cover Page Images: Upper: Colour composite picture of face-on spiral galaxy M 74 - from UVIT onboard AstroSat. Here blue colour represent image in far ultraviolet and green colour represent image in near ultraviolet.The spiral arms show the young stars that are copious emitters of ultraviolet light. Lower: Sarabhai crater as imaged by Terrain Mapping Camera-2 (TMC-2)onboard Chandrayaan-2 Orbiter.TMC-2 provides images (0.4μm to 0.85μm) at 5m spatial resolution 3 INDEX 4 FOREWORD PREFACE With great pleasure I introduce the report on Space Research in India, prepared for the 43rd COSPAR Scientific Assembly, 28 January – 4 February 2021, Sydney, Australia, by the Indian National Committee for Space Research (INCOSPAR), Indian National Science Academy (INSA), and Indian Space Research Organization (ISRO). The report gives an overview of the important accomplishments, achievements and research activities conducted in India in several areas of near- Earth space, Sun, Planetary science, and Astrophysics for the duration of two and half years (Jan 2018 – June 2020). -
General Disclaimer One Or More of the Following Statements May Affect
General Disclaimer One or more of the Following Statements may affect this Document This document has been reproduced from the best copy furnished by the organizational source. It is being released in the interest of making available as much information as possible. This document may contain data, which exceeds the sheet parameters. It was furnished in this condition by the organizational source and is the best copy available. This document may contain tone-on-tone or color graphs, charts and/or pictures, which have been reproduced in black and white. This document is paginated as submitted by the original source. Portions of this document are not fully legible due to the historical nature of some of the material. However, it is the best reproduction available from the original submission. Produced by the NASA Center for Aerospace Information (CASI) UNIVERSITY OF ILLINOIS URBANA AERONOMY REPfC".)IRT NO, 67 1 AN INVESTIGATION OF THE SOLAR ZENITH ANGLE VARIATION OF D-REGION IONIZATION (NASA-CF-143217) AN INVE'STIGATICN CF THE N75 -28597 SOIA; ZENITH ANGLE VAFIATICN CF C-FEGICN IONI2ATICN (I11incis Cniv.) 290 F HC iE.75 CSCL 044 U11C13s G3/4b 31113 by ^' x '^^ P. A. J. Ratnasiri o c n C. F. Scchrist, Jr. m y T April I, 1975 Library of Congress ISSN 0568-0581 Aeronomy Laboratory Supported by Department of Electrical Engineering National Science Foundation University of Illinois Grant GA 3691 IX Urbana, Illinois ii ABSTRACT A review of the D- region ionization measurements and its solar zenith angle variation reveals that a unified model of the D region, incorporating both thenetural chemistry and the ion chemistry, is required for a proper understanding of this region of the ionosphere. -
CC 149XX7 Next Generation Ionosonde (NEXION)
Next Generation Ionosonde (NEXION), (DPS 4-D). FAC: 1341 CATCODE: 149XX7 OPR: AFWA/A5/A8, MAJCOM/A3W OCR: MAJCOM/A6 1.1. Description. NEXION is an unmanned ionosonde facility that supports activities to sense and report ionospheric information for comprehensive and ongoing environmental analysis and mission impact assessment. NEXION is vertical incidence radar used to obtain information about the ionosphere directly overhead and consists of 30 systems worldwide and one test system. NEXION provides a 24/7 remote monitoring capability of the ionosphere by analyzing the signals reflected from the ionosphere and providing data to AFWA via the NIPRNet to be ingested into the new generation of Global Assimilation of Ionospheric Measurements (GAIM). 1.2. Requirements Determination. This facility supports activities and equipment to sense and report ionospheric information 24/7 to support and maintain battlespace awareness. Obtain further information through AFWA/A5/8 or MAJCOM/A3 weather staff. 1.3. Scope Determination. A NEXION site consists of a support building consisting of approximately 5 m2 (50 ft2), four receiving antennas placed in a triangular 60 degree configuration 60 m (197 ft) apart with #2 and #3 antennas aligned to magnetic north, and the #1 antenna centered between antennas #2 and #3 but physically located 34.64 m (114 ft) to the west of antenna #4. See Figure 1.2 for alignment and placement. Distance between the transmit tower and receiver antennas is 30 m (98.4 ft) minimum separation. The transmit antenna requires 15.24 m (50 ft) clearance between the transmit antenna and potential obstructions such as trees, shrubs, etc. -
Article E Layer
Geosci. Instrum. Method. Data Syst., 5, 53–64, 2016 www.geosci-instrum-method-data-syst.net/5/53/2016/ doi:10.5194/gi-5-53-2016 © Author(s) 2016. CC Attribution 3.0 License. Comparison between manual scaling and Autoscala automatic scaling applied to Sodankylä Geophysical Observatory ionograms Carl-Fredrik Enell1, Alexander Kozlovsky2, Tauno Turunen2,*, Thomas Ulich2, Sirkku Välitalo2, Carlo Scotto3, and Michael Pezzopane3 1EISCAT Scientific Association, Kiruna, Sweden 2Sodankylä Geophysical Observatory, University of Oulu, Sodankylä, Finland 3Istituto Nazionale di Geofisica e Vulcanologia (INGV), Rome, Italy *retired Correspondence to: Carl-Fredrik Enell ([email protected]) Received: 16 November 2015 – Published in Geosci. Instrum. Method. Data Syst. Discuss.: 21 December 2015 Revised: 14 March 2016 – Accepted: 14 March 2016 – Published: 23 March 2016 Abstract. This paper presents a comparison between stan- 1 Introduction dard ionospheric parameters manually and automatically scaled from ionograms recorded at the high-latitude So- dankylä Geophysical Observatory (SGO, ionosonde SO166, Ionosondes for studying the ionosphere were invented in the 64.1◦ geomagnetic latitude), located in the vicinity of the au- late 1920s, and their worldwide implementation started in the roral oval. The study is based on 2610 ionograms recorded 1940s as military shortwave communication became impor- during the period June–December 2013. The automatic scal- tant. An ionosonde is a radio echo instrument transmitting ra- ing was made by means of the Autoscala software. A few dio waves of alternating frequency, receiving reflections from typical examples are shown to outline the method, and statis- the ionosphere, and measuring the travel times of the waves tics are presented regarding the differences between manu- at different frequencies. -
Environmental Impact of High Power Density Microwave Beams on Different Atmospheric Layers
Environmental impact of high power density microwave beams on different atmospheric layers T. R. Robinson, T. K. Yeoman and R. S. Dhillon, Radio and Space Plasma Physics Group, Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, UK. ESA Contract number: 18156/04/NL/MV CONTRACT REPORT The work described in this report was done under ESA contract. Responsibility for the contents resides in the author or organisation that prepared it. Environmental impact of high power density microwave beams on different atmospheric layers T. R. Robinson, T. K. Yeoman and R. S. Dhillon, Radio and Space Plasma Physics Group, Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, UK. ESA Contract number: 18156/04/NL/MV Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, UK. Francesco Cattaneo Andres Galvez Leopold Summerer Radio and Space Plasma Physics Group Tech. Rep. 63, Leicester University, UK, 2004. September 2004 CONTRACT REPORT The work described in this report was done under ESA contract. Responsibility for the contents resides in the author or organisation that prepared it. i Environmental impact of high power microwave beams Abstract The mechanisms involved in the trans-ionospheric propagation of Solar Power Satellite microwave beams are considered in the context of both efficiency of the power transfer as well as of environmental impact. Processes involved include, linear effects such as collisional absorption, scintillation and scattering which lead to loss of energy from the beam, as well as the excitation of certain nonlinear effects, such as stimulated scattering and the thermal self-focussing instability. -
Handbook of Correlative Data
THE NATIONAL SPACE SCIENCE DATA CENTER Handbook of Correlative Data FEBRUARY 1971 J41516 cxa XA *NATIONAL SPACE SCIENCE DATA CENTER NATIONAL AERONAUTICS AND SPACE ADMINISTRATION GODDARD SPACE FLIGHT CENTER, GREENBELT, MD. NSSDC 71-05 The National Space Science Data Center HANDBOOK OF CORRELATIVE DATA Joseph H. King, Editor February 1971 FOREWORD In previous years, the National Space Science Data Center (NSSDC) has generated a Catalog of Correlative Data. This catalog listed and, to some extent, described the correlative data holdings of NSSDC. How- ever, it was felt desirable to have a document of a more general nature, which would point to correlative data available at any data center or in any readily accessible publication. This Handbook of Correlative Data was generated to fulfill this need. This Handbook can be used to acquaint the reader with many solar and geophysical phenomena, to point the reader to more detailed discus- sions of the phenomena, and to direct him to the data. It is antici- pated that many readers will require this Handbook for only the last one or two of these purposes. A second edition of this Handbook will be generated when warranted. Accordingly, I would appreciate receiving comments from the users of this Handbook. Any recommendations for improving its usefulness will be most helpful in the generation of a second edition. I want to thank the NSSDC personnel who served as authors of the individual sections; their names appear on the pages introducing each of the nine major parts. I would like to acknowledge the assistance of other NSSDC personnel, particularly Miss Mary Anne Beeler, who were involved in the various stages of the generation of this Handbook. -
A History of Vertical-Incidence Ionsphere Sounding at the National
TECH, aoaot Mii22 PB 151387 ^0.28 ^5oulder laboratories A HISTORY OF VERTICAL - INCIDENCE IONOSPHERE SOUNDING AT THE NATIONAL BUREAU OF STANDARDS BY SANFORD C. GLADDEN U. S. DEPARTMENT OF COMMERCE NATIONAL BUREAU OF STANDARDS IE NATIONAL BUREAU OF STANDARDS Functions and Activities The Functions of the National Bureau of Standards are set forth in the Act of Congress, March 3, 1901, as amended by Congress in Public Law 619, 1950. These include the development and maintenance of the national standards of measurement and the provision of means and methods for making measurements consistent with these standards: the determination of physical constants and properties of materials: the development of methods and instruments for testing materials, devices, and structures; advisory services to government agencies on scientific and technical problems; in- vention and development of devices to serve special needs of the Government; and the development of standard practices, codes, and specifications. The work includes basic and applied research, development, engineering, instrumentation, testing, evaluation, calibration services, and various consultation and information services. Research projects are also performed for other government agencies when the work relates to and supplements the basic program of the Bureau or when the Bureau's unique competence is required. The scope of activities is suggested by the listing of divisions and sections on the inside of the back cover. Publications The results of the Bureau's work take the form of either actual equipment and devices or pub- lished papers. These papers appear either in the Bureau's own series of publications or in the journals of professional and scientific societies.