RADIOTOMOGRAPHIC IMAGING OF THE ARTIFICIALLY DISTURBED MIDLATITUDE IONOSPHERE WITH CASSIOPE AND PARUS SATELLITES
|
|
|
- Edward Allen
- 6 years ago
- Views:
Transcription
1 RADIOTOMOGRAPHIC IMAGING OF THE ARTIFICIALLY DISTURBED MIDLATITUDE IONOSPHERE WITH CASSIOPE AND PARUS SATELLITES Vyacheslav E. Kunitsyn, Elena S. Andreeva, Artem M. Padokhin, Lomonosov Moscow State University, Faculty of Physics Vladimir L. Frolov, Georgy P. Komrakov, Radio Physical Research Institute Paul Bernhardt, Carl Siefring Naval Research Laboratory IES 2015, Alexandria VA, USA, May 14, 2015
2 Motivation Since first theoretical works [Grigor ev, 1975 etc] the topic of artificial AGWs generation in the HF heating experemts was of great interest. Recent works report on the generation of AGW/TIDs in experiments at HAARP [Mishin et al., 2012; Pradipta et al, 2015, etc] and SURA [Burmaka et al., 2009; Chernogor et al., 2011] heaters. Still there is lack of the information of the spatial struture of such disturbances. Radiotomography technique is successfully applied during the past decades and provided information on many ionospheric structures such as the ionization troughs, equatorial anomaly, travelling ionospheric disturbances, equatorial plasma depletions, etc [Kunitsyn and Tereshchenko, 2003; Pryse, 2003; Bust and Mitchell, 2008] The aim of this work is to report the experimental results on the influence of the electron density perturbations caused by HF heating in the nightside midlatitude ionosphere on Parus/Transit and epop signals and present reconstructed parameters of heating-induced perturbations with the focus on artificial AGW/TIDs generation
3 Experimental equipment Sura Heater ( E; N), I=71 0 3x250kW transmitters 12x12 dipoles antenna array MHz pumping frequency range (O & X modes) ERP=80-280MW GNSS Receivers Multiconstellation (GPS/GLONASS/ GALLILEO/COMPASS/SBAS/QZSS) JAVAD SIGMA or DELTA receivers with up to 100 Hz sampling of L1/L2/L5... Beacon Receivers NWRA ITS30/33S, ADK4M working with 150/400MHz transmissions from PARUS (Russian LEO navigation system) satellites COSMOS 2407, and 150/400/1066MHz transmissions from epop/cer instrument onboard CASSIOPE
4 Description of the Experiment
![Results from Sura Heater Heating on 16 March 2009 [Frolov et al. 2010, Kunitsyn et al. 2011] 30 sec. heating 30 sec.](/docs-images/73/69353736/images/5-0.jpg "pause regime 6:15-7:51UT 5 min. heating 5 min. pause regime 7:51-8:26UT f=4.")
5 Results from Sura Heater Heating on 16 March 2009 [Frolov et al. 2010, Kunitsyn et al. 2011] 30 sec. heating 30 sec. pause regime 6:15-7:51UT 5 min. heating 5 min. pause regime 7:51-8:26UT f=4.3mhz O-mode ERP=40 Mw till 7:36 and 80 Mw later Low geomagnetic activity (Kp~1)
![Results from Sura Heater Heating on 15 March 2009 [Frolov et al. 2010, Kunitsyn et al. 2011] 5 min. heating 5 min.](/docs-images/73/69353736/images/6-2.jpg "pause regime 7:16-8:41UT f=4.3mhz O-mode ERP=80 Mw Moderate geomagnetic activity (Kp~3) f 0 F2<f for 7:50-8:12 UT")
6 Results from Sura Heater Heating on 15 March 2009 [Frolov et al. 2010, Kunitsyn et al. 2011] 5 min. heating 5 min. pause regime 7:16-8:41UT f=4.3mhz O-mode ERP=80 Mw Moderate geomagnetic activity (Kp~3) f 0 F2<f for 7:50-8:12 UT
![Low-orbital tomography and amplitude scintillations 2 φ+ ϕ N dl σ σ 2 ( z) f [ R ( z), αβ,, Ψ, p, Θ( z) ] dz 0 e χ N F Angle between line-of-sight](/docs-images/73/69353736/images/7-1.jpg "and magnetic field, H=300 km 57 56.5 Galibikha heating limit 56 55.5 55 20 15 5 peak 10 heating limit heating center 54.5 43.5 44 44.5 45 45.5 46 46.")
7 Low-orbital tomography and amplitude scintillations 2 φ+ ϕ N dl σ σ 2 ( z) f [ R ( z), αβ,, Ψ, p, Θ( z) ] dz 0 e χ N F Angle between line-of-sight and magnetic field, H=300 km Galibikha heating limit peak 10 heating limit heating center
![August,18 2011 [Kunitsyn et al., 2012].](/docs-images/73/69353736/images/8-3.jpg "IPP trajectories of LO beacon satellite IPP trajectories of")
8 Coordinated GNSS and LORT observations of the wavelike disturbances induced by HF-heating. August, [Kunitsyn et al., 2012]. IPP trajectories of LO beacon satellite IPP trajectories of GNSS satellites HF heating induced AGWs Observation sites with GNSS and beacon receivers 14:16-16:56 UT, 4785kHz 17:01-18:51 UT, 4785kHz ±10 min with ERP = 100MW f O F2 = 5.7 MHz Sura heater O-mode f =4.785MHz<f o F2 ERP ~ 50MW from 14:16 till 16:56 UT [10 min on,10 min pause] from 17:01 till 18:51 UT [10 min on,10 min pause] Note trough directivity pattern HF heating induced AGWs positive duct formation at high alt.
9 15:58 18:38 UT 5455kHz (lower than f O F2). [+10 min, -10 min], ERP ~100 MW 18:38 18:50 UT 5455kHz CW PARUS
10 15:58 17:13UT 8060kHz ±15 min; 17:28 18:43UT 4785kHz ±15 min ERP ~ 100MW 18:58 19:18UT 4785kHz CW ERP ~ 100MW epop
11 15:58 18:43UT 4785kHz ±15 min ERP ~ 100MW 18:58 19:18UT 4785kHz CW ERP ~ 100MW epop
![19:04 20:19 UT 4300 khz, [+ 15 min; 15 min], ERP = 55 MW.](/docs-images/73/69353736/images/12-1.jpg "20:34 20:54 UT 4300 khz, [+ 9 s; 1 s], ERP = 55 MW. f O F2 4.")
12 19:04 20:19 UT 4300 khz, [+ 15 min; 15 min], ERP = 55 MW. 20:34 20:54 UT 4300 khz, [+ 9 s; 1 s], ERP = 55 MW. f O F2 4.7 MHz at 20:30 UT. epop
13 18:59 20:14 UT 4300 khz, [+ 15 min; 15 min], ERP = 55 MW. f O F2 4.4 MHz at 20:15 UT. 20:29 20:30 UT 4300 khz, CW; 20:30 20:49 UT -[+ 9 s; 1 s], ERP = 55 MW epop
14 18:56 20:26 UT 4300 khz, [+ 10 min; 10 min], ERP = 55 MW. 20:26 20:46 UT 4300 khz, [+ 9 s; 1 s], ERP = 55 MW. f O F2 4.5 MHz at 19:50 UT. epop
15 epop-sura tomography experiment summary two campaigns (March, September 2014) 3 receiving sites with NWRA ITS30/33S beacon receivers (150/400/1066MHz) a) Galibikha( N, E) b) Sura( N, E) c) Sechenovo( N, E) Sura heater (all 3 transmitters) operating O-mode, square wave modulation of ERP at a frequency of the order of the Brunt-Vaisala frequency, f H f O F2, nighttime conditions Common features to benoted on the following RT reconstructions: wave-like structures, possibly artificial AGWs, diverging from the heated area narrow trough, corresponding to directivity pattern of Sura heater
16 LORT reconstructions of disturbed area using epop and COSMOS data
17 Penetration of the pumping wave up to the satellite heights :24 UT for COSOMOS 2414 pass Courtesy of Prof. A. Krukovsky
![18:59 20:14 UT 4300 khz, [+ 15 min; 15 min], ERP = 55 MW. f0f2 4.4 MHz at 20:15 UT.](/docs-images/73/69353736/images/18-2.jpg "20:29 20:30 UT 4300 khz, CW; 20:30 20:49 UT -[+ 9 s; 1 s], ERP = 55 MW Courtesy of Dr.")
18 18:59 20:14 UT 4300 khz, [+ 15 min; 15 min], ERP = 55 MW. f0f2 4.4 MHz at 20:15 UT. 20:29 20:30 UT 4300 khz, CW; 20:30 20:49 UT -[+ 9 s; 1 s], ERP = 55 MW Courtesy of Dr. Gordon James
19 Conclusions. We present the evedences for the generation of artificial AGW/TIDs in ionospheric heating experiments at Sura heater when the ERP is modulated with a square wave at a frequency lower than the Brunt- Vaisala frequency of the neutral atmosphere at the reflection height of the pump wave. A comprehensive model of HF-induced thermospheric perturbations has not yet been developed. More observational, theoretical and modeling efforts are required to understand the underlying generation processes. epop/cassiope instruments can contribute highly to this work. THANK YOU FOR YOUR ATTENETION
Radiotomographic imaging of the artificially disturbed midlatitude ionosphere with CASSIOPE and Parus satellites
Radiotomographic imaging of the artificially disturbed midlatitude ionosphere with CASSIOPE and Parus satellites Vyacheslav E. Kunitsyn 1, Elena S. Andreeva 1, Artem M. Padokhin 1, Vladimir L. Frolov 2,
Sounding of HF heating-induced artificial ionospheric disturbances by navigational satellites radio transmissions.
Sounding of HF heating-induced artificial ionospheric disturbances by navigational satellites radio transmissions. V.E. Kunitsyn 1, E.S. Andreeva 1, V.L. Frolov, G.P. Komrakov, M.O. Nazarenko 1, A.M. Padokhin
PUBLICATIONS. Radio Science. Radiotomography and HF ray tracing of the artificially disturbed ionosphere above the Sura heating facility
PUBLICATIONS RESEARCH ARTICLE Special Section: Ionospheric Effects Symposium 2015 Key Points: Radiotomographic imaging the artificially modified nighttime midlatitude ionosphere Spatial structure of the
First Results from the 2014 Coordinated Measurements Campaign with HAARP and CASSIOPE/ePOP
First Results from the 2014 Coordinated Measurements Campaign with HAARP and CASSIOPE/ePOP Carl L. Siefring, Paul A. Bernhardt, Stanley J. Briczinski, and Michael McCarrick Naval Research Laboratory Matthew
HAARP-induced Ionospheric Ducts
HAARP-induced Ionospheric Ducts Gennady Milikh, University of Maryland in collaboration with: Dennis Papadopoulos, Chia-Lee Chang, Hira Shroff, BAE systems Evgeny Mishin, AFRL/RVBXI, Hanscom AFB Michel
Radio-science experiments with the Enhanced Polar Outflow Probe satellite payload using its RRI, GAP and CERTO instruments
Radio-science experiments with the Enhanced Polar Outflow Probe satellite payload using its RRI, GAP and CERTO instruments H.G. James, CRC, Ottawa, Canada P.A. Bernhardt, NRL, Washington, U.S.A. R.B. Langley,
Artificial Ionospheric Perturbations Studied During НААRP May-June 2014 campaign
Artificial Ionospheric Perturbations Studied During НААRP May-June 2014 campaign E.N. Sergeev 1,2, A.V. Shindin 1, S.M. Grach 1, G.M. Milikh 3 1 Lobachevsky State University of Nizhni Novgorod, Gagarin
Artificial Ionospheric Perturbations Studied During НААRP May-June 2014 campaign
Artificial Ionospheric Perturbations Studied During НААRP May-June 2014 campaign E.N. Sergeev 1,2, A.V. Shindin 1, S.M. Grach 1, G.M. Milikh 3 1 Lobachevsky State University of Nizhni Novgorod, Gagarin
Whistler Wave Generation by Continuous HF Heating of the F-region Ionosphere
Whistler Wave Generation by Continuous HF Heating of the F-region Ionosphere Aram Vartanyan 1 G. M. Milikh 1, B. Eliasson 1,2, A. C. Najmi 1, M. Parrot 3, K. Papadopoulos 1 1 Departments of Physics and
The Largest Ionospheric Disturbances Produced by the HAARP HF Facility
The Largest Ionospheric Disturbances Produced by the HAARP HF Facility Paul A. Bernhardt 1, Carl L. Seifring 1, Stanley J. Briczinski 2, Elizabeth A. kendall 3, Brenton J. Watkins 4, William Bristow 4,
Daily and seasonal variations of TID parameters over the Antarctic Peninsula
Daily and seasonal variations of TID parameters over the Antarctic Peninsula A. Zalizovski 1, Y. Yampolski 1, V. Paznukhov 2, E. Mishin 3, A. Sopin 1 1. Institute of Radio Astronomy, National Academy of
Ground based measurements of ionospheric turbulence manifestations induced by the VLF transmitter ABSTRACT
Ground based measurements of ionospheric turbulence manifestations induced by the VLF transmitter Dmitry S. Kotik, 1 Fedor I. Vybornov, 1 Alexander V. Ryabov, 1 Alexander V. Pershin 1 and Vladimir A. Yashnov
New applications of the portable heater. Gennady Milikh, UMD-SPP group
New applications of the portable heater Gennady Milikh, UMD-SPP group 1 Stabilization of equatorial spread F (ESF) by ion injection 2 ESF characterizes spreading in the height of F-region backscatter return
Ionospheric Effects on Aviation
Ionospheric Effects on Aviation Recent experience in the observation and research of ionospheric irregularities, gradient anomalies, depletion walls, etc. in USA and Europe Stan Stankov, René Warnant,
Preliminary results from the Arecibo Heating EXperiment (HEX): From HF to GPS
Preliminary results from the Arecibo Heating EXperiment (HEX): From HF to GPS CEDAR Workshop 2017 Keystone, Co Dr Natasha Jackson-Booth 21 st June 2017 Collaborators and Acknowledgements QinetiQ Richard
Space-born system for on-line precursors monitoring of eathquakes,, natural and man-made made catastrophes
Space-born system for on-line precursors monitoring of eathquakes,, natural and man-made made catastrophes The main goal of the Project In my brief report, I would like to inform about the work on developing
Future of the HAARP Facility. Bob McCoy Director, Geophysical Institute University of Alaska Fairbanks
Future of the HAARP Facility Bob McCoy Director, Geophysical Institute University of Alaska Fairbanks rpmccoy@alaska.edu 1 US Chairmanship 2015-2017 Future Space Research in Alaska: Integrated networks
INTRODUCTION. 1.1 Background. Chapter -1
Chapter -1 INTRODUCTION 1.1 Background Beacon experiments onboard satellites have been contributing to atmospheric research since the eighties. According to Oxford dictionary, Beacon specifies a single
Chapter 1: Telecommunication Fundamentals
Chapter 1: Telecommunication Fundamentals Block Diagram of a communication system Noise n(t) m(t) Information (base-band signal) Signal Processing Carrier Circuits s(t) Transmission Medium r(t) Signal
Page 1 of 8 Search Contact NRL Personnel Locator Human Resources Public Affairs Office Visitor Info Planning a Visit Directions Maps Weather & Traffic Field Sites Stennis Monterey VXS-1 Chesapeake Bay
Solar Radar Experiments
Solar Radar Experiments Paul Rodriguez Plasma Physics Division Naval Research Laboratory Washington, DC 20375 phone: (202) 767-3329 fax: (202) 767-3553 e-mail: paul.rodriguez@nrl.navy.mil Award # N0001498WX30228
The First Results from the Scintillation and Ionospheric TEC Receiver in Space (CITRIS) Instrument on STPSat1
The First Results from the Scintillation and Ionospheric TEC Receiver in Space (CITRIS) Instrument on STPSat1 Carl L. Siefring and Paul A. Bernhardt Plasma Physics Division, Naval Research Laboratory Washington,
SEMEP. Search for ElectroMagnetic Earthquake Precursors
Page: 1 of 11 SEMEP Search for ElectroMagnetic Earthquake Precursors Identification of ionospheric perturbations connected to seismicity from the analysis VLF/LF signals on the DEMETER satellite Deliverable
Paul Bernhardt 1, Carl Siefring 1, Andrew Yau 2, H. Gordon James 3. Naval Research Laboratory, Washington, DC. University of Calgary, Alberta, Canada
Space Based Instrumentation for Future Detection of Artificial ULF/ELF/VLF waves and Their Effects using the Canadian Sponsored Enhanced Polar Outflow Project (epop) Satellite Paul Bernhardt 1, Carl Siefring
Storms in Earth s ionosphere
Storms in Earth s ionosphere Archana Bhattacharyya Indian Institute of Geomagnetism IISF 2017, WSE Conclave; Anna University, Chennai Earth s Ionosphere Ionosphere is the region of the atmosphere in which
The Largest Ionospheric Disturbances Produced by the HAARP HF Facility
The Largest Ionospheric Disturbances Produced by the HAARP HF Facility Paul A. Bernhardt, Carl L. Siefring, Stanley J. Briczinski Plasma Physics Division and Naval Center for Spacecraft Technology Naval
Frequency Dependence of VLF Wave Generation at Gakona, Alaska
Frequency Dependence of VLF Wave Generation at Gakona, Alaska Spencer P. Kuo 1, Maurice Rubinraut 1, Yen-Liang Wu 1, R. Pradipta 2, J.A. Cohen 2, M.C. Lee 2,3 1 Dept of Electrical & Computer Engineering,
Study of small scale plasma irregularities. Đorđe Stevanović
Study of small scale plasma irregularities in the ionosphere Đorđe Stevanović Overview 1. Global Navigation Satellite Systems 2. Space weather 3. Ionosphere and its effects 4. Case study a. Instruments
Model for artificial ionospheric duct formation due to HF heating
Click Here for Full Article GEOPHYSICAL RESEARCH LETTERS, VOL. 37,, doi:10.1029/2010gl042684, 2010 Model for artificial ionospheric duct formation due to HF heating G. M. Milikh, 1 A. G. Demekhov, 2 K.
Testing Plasma Physics in the Ionosphere
Testing Plasma Physics in the Ionosphere Dennis Papadopoulos University of Maryland College Park, MD 20742 X. Shao, G. Milikh - UMCP C. Chang, T. Wallace, M. McCarrick, I Doxas BAE Systems-AT U. Inan,
On the Viability and Requirements of a Barge Based ELF System
On the Viability and Requirements of a Barge Based ELF System Presentation to Dr. Bobby Junker ONR Code 31 Dennis Papadopoulos University of Maryland December 21,2010 Outline The Physics and Experimental
Monitoring the polar cap/ auroral ionosphere: Industrial applications. P. T. Jayachandran Physics Department University of New Brunswick Fredericton
Monitoring the polar cap/ auroral ionosphere: Industrial applications P. T. Jayachandran Physics Department University of New Brunswick Fredericton Outline Ionosphere and its effects on modern and old
Assimilation Ionosphere Model
Assimilation Ionosphere Model Robert W. Schunk Space Environment Corporation 399 North Main, Suite 325 Logan, UT 84321 phone: (435) 752-6567 fax: (435) 752-6687 email: schunk@spacenv.com Award #: N00014-98-C-0085
C4: Collaborative Work on Novel Approaches to ELF/VLF Generation
C4: Collaborative Work on Novel Approaches to ELF/VLF Generation Mark Golkowski University of Colorado Denver Robb Moore, Umran Inan, Morris Cohen, Ray Ingram, Tom Lee, Ed Kennedy, Paul Kossey C4: Collaborative
The EISCAT Heating Facility
The EISCAT Heating Facility Michael Rietveld EISCAT Tromsø, Norway EISCAT radar school, 30 Aug-4 Sept, 2010, Sodankylä 1 Outline Description of the hardware Antenna beams Practical details- power levels
Ionospheric Monitoring in China. Zhen Weimin, Ou Ming
ICG-5 WG-B, Turino Ionospheric Monitoring in China Zhen Weimin, Ou Ming October 20 th, 2010, Turino, Italy Outline 1.Introduction 2.Ionosphere monitoring in China 3.Summary 1. Introduction GNSS performance
Modification of the high latitude ionosphere F region by X-mode powerful HF radio waves: Experimental results from multiinstrument
Modification of the high latitude ionosphere F region by X-mode powerful HF radio waves: Experimental results from multiinstrument diagnostics N. F. Blagoveshchenskaya 1, T. D. Borisova 1, T. K. Yeoman
(CSES) Introduction for China Seismo- Electromagnetic Satellite
Introduction for China Seismo- Electromagnetic Satellite (CSES) Wang Lanwei Working Group of China Earthquake-related related Satellites Mission China Earthquake Administration Outline Project Objectives
Operational Products of the Space Weather Application Center Ionosphere (SWACI) and capabilities of their use
Operational Products of the Space Weather Application Center Ionosphere (SWACI) and capabilities of their use N. Jakowski, C. Borries, V. Wilken, K.D. Missling, H. Barkmann, M. M. Hoque, M. Tegler, C.
Ionospheric Imprint to LOFAR
Ionospheric Imprint to LOFAR Norbert Jakowski Institute of Communications und Navigation German Aerospace Center Kalkhorstweg 53, D-17235 Neustrelitz, Germany LOFAR Workshop, 8/9 November 2010, Potsdam,
Geoff Crowley, Chad Fish, Charles Swenson, Gary Bust, Aroh Barjatya, Miguel Larsen, and USU Student Team
Geoff Crowley, Chad Fish, Charles Swenson, Gary Bust, Aroh Barjatya, Miguel Larsen, and USU Student Team NSF-Funded Dual-satellite Space Weather Mission Project Funded October 2009 (6 months ago) 1 2 11
Space weather Application Center Ionosphere A Near-Real-Time Service Based on NTRIP Technology
Space weather Application Center Ionosphere A Near-Real-Time Service Based on NTRIP Technology N. Jakowski, S. M. Stankov, D. Klaehn, C. Becker German Aerospace Center (DLR), Institute of Communications
The USU-GAIM Data Assimilation Models for Ionospheric Specifications and Forecasts
The USU-GAIM Data Assimilation Models for Ionospheric Specifications and Forecasts L. Scherliess, R. W. Schunk, L. C. Gardner, L. Zhu, J.V. Eccles and J.J Sojka Center for Atmospheric and Space Sciences
VLF REMOTE SENSING OF THE LOWER IONOSPHERE AND REAL TIME SIGNAL PROCESSING
VLF REMOTE SENSING OF THE LOWER IONOSPHERE AND REAL TIME SIGNAL PROCESSING VLADIMIR SREĆKOVIĆ 1, DARKO JEVREMOVIĆ 2, V. VUJČIĆ 2 1 INSTITUTE OF PHYSICS, P.O.BOX 57,UNIVERSITY OF BELGRADE 2 ASTRONOMICAL
ALTITUDE PROFILES OF ELECTRON DENSITY DURING LEP EVENTS FROM VLF MONITORING OF THE LOWER IONOSPHERE
The Sharjah-Stanford AWESOME VLF Workshop Sharjah, UAE, Feb 22-24, 2010. ALTITUDE PROFILES OF ELECTRON DENSITY DURING LEP EVENTS FROM VLF MONITORING OF THE LOWER IONOSPHERE Desanka Šulić 1 and Vladimir
CDAAC Ionospheric Products
CDAAC Ionospheric Products Stig Syndergaard COSMIC Project Office COSMIC retreat, Oct 13 14, 5 COSMIC Ionospheric Measurements GPS receiver: { Total Electron Content (TEC) to all GPS satellites in view
GPS interfrequency biases and total electron content errors in ionospheric imaging over Europe
RADIO SCIENCE, VOL. 41,, doi:10.1029/2005rs003269, 2006 GPS interfrequency biases and total electron content errors in ionospheric imaging over Europe Richard M. Dear 1 and Cathryn N. Mitchell 1 Received
GPS=GLONASS-based TEC measurements as a contributor for space weather forecast
Journal of Atmospheric and Solar-Terrestrial Physics 64 (2002) 729 735 www.elsevier.com/locate/jastp GPS=GLONASS-based TEC measurements as a contributor for space weather forecast N. Jakowski, S. Heise,
The Significance of GNSS for Radio Science
Space Weather Effects on the Wide Area Augmentation System (WAAS) The Significance of GNSS for Radio Science Patricia H. Doherty Vice Chair, Commission G International Union of Radio Science www.ursi.org
Effects of magnetic storms on GPS signals
Effects of magnetic storms on GPS signals Andreja Sušnik Supervisor: doc.dr. Biagio Forte Outline 1. Background - GPS system - Ionosphere 2. Ionospheric Scintillations 3. Experimental data 4. Conclusions
EFFECTS OF SCINTILLATIONS IN GNSS OPERATION
- - EFFECTS OF SCINTILLATIONS IN GNSS OPERATION Y. Béniguel, J-P Adam IEEA, Courbevoie, France - 2 -. Introduction At altitudes above about 8 km, molecular and atomic constituents of the Earth s atmosphere
Analysis of equatorial ionospheric irregularities based on a two high rate GNSS station setup
Analysis of equatorial ionospheric irregularities based on a two high rate GNSS station setup Jens Berdermann 1,Norbert Jakowski 1, Martin Kriegel 1, Hiroatsu Sato 1, Volker Wilken 1, Stefan Gewies 1,
Using GNSS Tracking Networks to Map Global Ionospheric Irregularities and Scintillation
Using GNSS Tracking Networks to Map Global Ionospheric Irregularities and Scintillation Xiaoqing Pi Anthony J. Mannucci Larry Romans Yaoz Bar-Sever Jet Propulsion Laboratory, California Institute of Technology
Satellite Navigation Science and Technology for Africa. 23 March - 9 April, The African Ionosphere
2025-28 Satellite Navigation Science and Technology for Africa 23 March - 9 April, 2009 The African Ionosphere Radicella Sandro Maria Abdus Salam Intern. Centre For Theoretical Physics Aeronomy and Radiopropagation
Scientific Studies of the High-Latitude Ionosphere with the Ionosphere Dynamics and ElectroDynamics - Data Assimilation (IDED-DA) Model
DISTRIBUTION STATEMENT A. Approved for public release; distribution is unlimited. Scientific Studies of the High-Latitude Ionosphere with the Ionosphere Dynamics and ElectroDynamics - Data Assimilation
Assimilation Ionosphere Model
Assimilation Ionosphere Model Robert W. Schunk Space Environment Corporation 221 North Spring Creek Parkway, Suite A Providence, UT 84332 phone: (435) 752-6567 fax: (435) 752-6687 email: schunk@spacenv.com
LITES and GROUP-C on the ISS
LITES and GROUP-C on the ISS Collaboration Opportunities with ICON and GOLD See also poster by Budzien et al. Andrew Stephan, Scott Budzien (NRL) Susanna Finn, Tim Cook, Supriya Chakrabarti (UMass Lowell)
PUBLICATIONS. Radio Science
PUBLICATIONS RESEARCH ARTICLE Special Section: Beacon Satellite Symposium 2013 Key Points: Radio beacon tomography HF ray tracing through the reconstructions Experimental verification Correspondence to:
How GNSS and Beacon receivers can be used to monitor auroral ionosphere and space weather?
How GNSS and Beacon receivers can be used to monitor auroral ionosphere and space weather? Kirsti Kauristie, Finnish Meteorological Institute Special Thanks: J. Norberg (FMI), A. Aikio and T. Nygren (University
Developing systems for ionospheric data assimilation
Developing systems for ionospheric data assimilation Making a quantitative comparison between observations and models A.C. Bushell, 5 th European Space Weather Week, Brussels, 20 th November 2008 Collaborators
Polar Ionospheric Imaging at Storm Time
Ms Ping Yin and Dr Cathryn Mitchell Department of Electronic and Electrical Engineering University of Bath BA2 7AY UNITED KINGDOM p.yin@bath.ac.uk / eescnm@bath.ac.uk Dr Gary Bust ARL University of Texas
Plasma effects on transionospheric propagation of radio waves II
Plasma effects on transionospheric propagation of radio waves II R. Leitinger General remarks Reminder on (transionospheric) wave propagation Reminder of propagation effects GPS as a data source Some electron
Experimental Observations of ELF/VLF Wave Generation Using Optimized Beam-Painting
Experimental Observations of ELF/VLF Wave Generation Using Optimized Beam-Painting R. C. Moore Department of Electrical and Computer Engineering University of Florida, Gainesville, FL 32611. Abstract Observations
Radio wave power distribution at HF frequencies as modelled for the Radio Receiver Instrument (RRI) on the epop satellite mission
Radio wave power distribution at HF frequencies as modelled for the Radio Receiver Instrument (RRI) on the epop satellite mission G. C. Hussey, R. G. Gillies, G. J. Sofko, and H. G. James SuperDARN Workshop
Satellite Navigation Science and Technology for Africa. 23 March - 9 April, Scintillation Impacts on GPS
2025-29 Satellite Navigation Science and Technology for Africa 23 March - 9 April, 2009 Scintillation Impacts on GPS Groves Keith Air Force Research Lab. Hanscom MA 01731 U.S.A. Scintillation Impacts on
IRI-Plas Optimization Based Ionospheric Tomography
IRI-Plas Optimization Based Ionospheric Tomography Onur Cilibas onurcilibas@gmail.com.tr Umut Sezen usezen@hacettepe.edu.tr Feza Arikan arikan@hacettepe.edu.tr Tamara Gulyaeva IZMIRAN 142190 Troitsk Moscow
Outline. GPS RO Overview. COSMIC Overview. COSMIC-2 Overview. Summary 9/29/16
Bill Schreiner and UCAR/COSMIC Team UCAR COSMIC Program Observation and Analysis Opportunities Collaborating with the ICON and GOLD Missions Sept 27, 216 GPS RO Overview Outline COSMIC Overview COSMIC-2
imaging of the ionosphere and its applications to radio propagation Fundamentals of tomographic Ionospheric Tomography I: Ionospheric Tomography I:
Ionospheric Tomography I: Ionospheric Tomography I: Fundamentals of tomographic imaging of the ionosphere and its applications to radio propagation Summary Introduction to tomography Introduction to tomography
The Ionosphere and its Impact on Communications and Navigation. Tim Fuller-Rowell NOAA Space Environment Center and CIRES, University of Colorado
The Ionosphere and its Impact on Communications and Navigation Tim Fuller-Rowell NOAA Space Environment Center and CIRES, University of Colorado Customers for Ionospheric Information High Frequency (HF)
Space Weather and the Ionosphere
Dynamic Positioning Conference October 17-18, 2000 Sensors Space Weather and the Ionosphere Grant Marshall Trimble Navigation, Inc. Note: Use the Page Down key to view this presentation correctly Space
On the Importance of Radio Occultation data for Ionosphere Modeling
On the Importance of Radio Occultation data for Ionosphere Modeling IROWG Workshop, Estes Park, March 30, 2012 ABSTRACT The availability of unprecedented amounts of Global Navigation Satellite Systems
CubeSat Communications Review and Concepts. Workshop, July 2, 2009
CubeSat Communications Review and Concepts CEDAR CubeSats Constellations and Communications Workshop, July 2, 29 Charles Swenson Presentation Outline Introduction slides for reference Link Budgets Data
Ionospheric Structure Imaging with ALOS PALSAR
The Second ALOS PI Symposium Rhodes, Greece November 3 7, 008 Ionospheric Structure Imaging with ALOS PALSAR PI Number: 37 JAXA-RA PI: Jong-Sen Lee, Thomas L. Ainsworth and Kun-Shan Chen CSRSR, National
Ionospheric Propagation
Ionospheric Propagation Page 1 Ionospheric Propagation The ionosphere exists between about 90 and 1000 km above the earth s surface. Radiation from the sun ionizes atoms and molecules here, liberating
The Precision Expandable Radar Calibration Sphere (PERCS) With Applications for Laser Imaging and Ranging
The Precision Expandable Radar Calibration Sphere (PERCS) With Applications for Laser Imaging and Ranging Paul A. Bernhardt 1, Andy Nicholas 2, Linda Thomas 3, Mark Davis 3 1 Plasma Physics Division, 2
MEETING OF THE METEOROLOGY PANEL (METP) METEOROLOGICAL INFORMATION AND SERVICE DEVELOPMENT WORKING GROUP (WG-MISD)
METP-WG/MISD/1-IP/09 12/11/15 MEETING OF THE METEOROLOGY PANEL (METP) METEOROLOGICAL INFORMATION AND SERVICE DEVELOPMENT WORKING GROUP (WG-MISD) FIRST MEETING Washington DC, United States, 16 to 19 November
VARIATIONS OF VLF SIGNALS RECEIVED ON DEMETER SATELLITE. IN ASSOCIATION WITH SEISMICITY A. Rozhnoi 1, M. Solovieva 1, Molchanov O.
VARIATIONS OF VLF SIGNALS RECEIVED ON DEMETER SATELLITE IN ASSOCIATION WITH SEISMICITY A. Rozhnoi 1, M. Solovieva 1, Molchanov O. 1 1 Institute of the Earth Physics, RAS, Bolshaya Gruzinskaya 10, Moscow,
and Atmosphere Model:
1st VarSITI General Symposium, Albena, Bulgaria, 2016 Canadian Ionosphere and Atmosphere Model: model status and applications Victor I. Fomichev 1, O. V. Martynenko 1, G. G. Shepherd 1, W. E. Ward 2, K.
Geomagnetic Conjugate Observations of Ionospheric Disturbances in. response to North Korea Underground Nuclear Explosion on 3
1 2 3 Geomagnetic Conjugate Observations of Ionospheric Disturbances in response to North Korea Underground Nuclear Explosion on 3 September 2017 4 5 6 7 Yi Liu, Chen Zhou *, Qiong Tang, Guanyi Chen, and
SATELLITE BEACON EXPERIMENTS FOR IONOSPHERIC STUDIES. 3.1 Introduction. Chapter -3
Chapter -3 SATELLITE BEACON EXPERIMENTS FOR IONOSPHERIC STUDIES This chapter gives an introduction to Earth s ionosphere, stating the importance of ionospheric studies using satellite beacon systems. Various
Regional ionospheric disturbances during magnetic storms. John Foster
Regional ionospheric disturbances during magnetic storms John Foster Regional Ionospheric Disturbances John Foster MIT Haystack Observatory Regional Disturbances Meso-Scale (1000s km) Storm Enhanced Density
CONTROLLED WAVE PARTICLE INTERACTION STUDIES IN THE RADIATION BELTS
CONTROLLED WAVE PARTICLE INTERACTION STUDIES IN THE RADIATION BELTS DENNIS PAPADOPOULOS UMCP ACKNOWLEDGE: C.L.CHANG, J.LEBINSKY AT BAE SYSTEMS XI SHAO, B.ELIASSON, S. SHARMA AND G. MILIKH AT UMCP SUPPORT:
Electron acceleration and ionization fronts induced by high frequency plasma turbulence
Eliasson, Bengt (2014) Electron acceleration and ionization fronts induced by high frequency plasma turbulence. In: 41st IOP Plasma Physics Conference, 2014-04-14-2014-04-17, Grand Connaught Rooms., This
Article in Proof. 2. Numerical Model of Formation of the Artificial 84 Ducts LXXXXX
Click Here for Full Article GEOPHYSICAL RESEARCH LETTERS, VOL. 37,, doi:10.1029/2010gl042684, 2010 1 Model for artificial ionospheric duct formation due to HF heating 2 G. M. Milikh, 1 A. G. Demekhov,
Radio tomography based on satellite beacon experiment and FORMOSAT- 3/COSMIC radio occultation
Radio tomography based on satellite beacon experiment and FORMOSAT- 3/COSMIC radio occultation Mamoru Yamamoto (1), Smitha V. Thampi (2), Charles Lin (3) (1) RISH, Kyoto University, Japan (2) Space Physics
Polar Ionospheric Imaging at Storm Time
UNCLASSIFIED/UNLIMITED Polar Ionospheric Imaging at Storm Time Ms Ping Yin and Dr Cathryn Mitchell Department of Electronic and Electrical Engineering University of Bath BA2 7AY UNITED KINGDOM p.yin@bath.ac.uk
Chapter 6 Propagation
Chapter 6 Propagation Al Penney VO1NO Objectives To become familiar with: Classification of waves wrt propagation; Factors that affect radio wave propagation; and Propagation characteristics of Amateur
Detecting Ionospheric TEC Perturbations Generated by Natural Hazards Using a Real-Time Network of GPS Receivers
Detecting Ionospheric TEC Perturbations Generated by Natural Hazards Using a Real-Time Network of GPS Receivers Attila Komjathy, Yu-Ming Yang, and Anthony J. Mannucci Jet Propulsion Laboratory California
The Ionosphere and Thermosphere: a Geospace Perspective
The Ionosphere and Thermosphere: a Geospace Perspective John Foster, MIT Haystack Observatory CEDAR Student Workshop June 24, 2018 North America Introduction My Geospace Background (Who is the Lecturer?
SPACE WEATHER SIGNATURES ON VLF RADIO WAVES RECORDED IN BELGRADE
Publ. Astron. Obs. Belgrade No. 80 (2006), 191-195 Contributed paper SPACE WEATHER SIGNATURES ON VLF RADIO WAVES RECORDED IN BELGRADE DESANKA ŠULIĆ1, VLADIMIR ČADEŽ2, DAVORKA GRUBOR 3 and VIDA ŽIGMAN4
ROTI Maps: a new IGS s ionospheric product characterizing the ionospheric irregularities occurrence
3-7 July 2017 ROTI Maps: a new IGS s ionospheric product characterizing the ionospheric irregularities occurrence Iurii Cherniak Andrzej Krankowski Irina Zakharenkova Space Radio-Diagnostic Research Center,
Tomographic reconstruction of the ionosphere using ground-based GPS data in the Australian region
Tomographic reconstruction of the ionosphere using ground-based GPS data in the Australian region Endawoe Yizengaw (1), Peter Dyson (2), and Elizabeth Essex () (1) Physics Department, La Trobe University,
APPLICATION OF SMALL SATELLITES FOR HIGH PRECISION MEASURING EFFECTS OF RADIO WAVE PROPAGATION
APPLICATION OF SMALL SATELLITES FOR HIGH PRECISION MEASURING EFFECTS OF RADIO WAVE PROPAGATION K. Igarashi 1, N.A. Armand 2, A.G. Pavelyev 2, Ch. Reigber 3, J. Wickert 3, K. Hocke 1, G. Beyerle 3, S.S.
A CubeSat Radio Beacon Experiment
A CubeSat Radio Beacon Experiment CUBEACON A Beacon Test of Designs for the Future Antenna? Michael Cousins SRI International Multifrequency? Size, Weight and Power? CubeSat Developers Workshop, April
Dependence of radio wave anomalous attenuation in the ionosphere on properties of spatial spectrum of irregularities
Dependence of radio wave anomalous attenuation in the ionosphere on properties of spatial spectrum of irregularities N.A. Zabotin, G.A. Zhbankov and E.S. Kovalenko ostov State University, ostov-on-don,
Significant of Earth s Magnetic Field and Ionospheric Horizontal Gradient to GPS Signals
Proceeding of the 2013 IEEE International Conference on Space Science and Communication (IconSpace), 1-3 July 2013, Melaka, Malaysia Significant of Earth s Magnetic Field and Ionospheric Horizontal Gradient
The Role of Ground-Based Observations in M-I I Coupling Research. John Foster MIT Haystack Observatory
The Role of Ground-Based Observations in M-I I Coupling Research John Foster MIT Haystack Observatory CEDAR/GEM Student Workshop Outline Some Definitions: Magnetosphere, etc. Space Weather Ionospheric
Form Approved REPORT DOCUMENTATION PAGE N Cornell University Day Hall Ithaca, NY 14853
REPORT DOCUMENTATION PAGE Form Approved OMB No. 0704-0188 The public reporting burden for this collection of information is estimated to average 1 hour par response, including the time for reviewing instructions,
Rec. ITU-R P RECOMMENDATION ITU-R P *
Rec. ITU-R P.682-1 1 RECOMMENDATION ITU-R P.682-1 * PROPAGATION DATA REQUIRED FOR THE DESIGN OF EARTH-SPACE AERONAUTICAL MOBILE TELECOMMUNICATION SYSTEMS (Question ITU-R 207/3) Rec. 682-1 (1990-1992) The
Radio Communication. Presentation created by: András Balogh
Radio Communication Presentation created by: András Balogh AM and FM The goal is to transmit a modulating signal S(t) via a wave sin(ωt). In case of AM, the product of the modulation is f(t)=(a+s(t))*sin(ωt);