D. Odstrcil George Mason University, 4400 University Drive, Fairfax, VA 22030, USA and NASA/GSFC M/C 674, Greenbelt, MD 20771, USA
|
|
- Baldwin Webster
- 5 years ago
- Views:
Transcription
1 Different Techniques for for (and Measurement Some Success of BzIn) Measurement of Bs B.V. Jackson H.-S. Yu, P.P. Hick, A. Buffington, Center for Astrophysics and Space Sciences, University of California at San Diego, LaJolla, CA, USA M. Tokumaru, Ken ichi Fujiki Institute for Space-Earth Environmental Research (ISEE), Nagoya University, Furo-cho, Chikusa-ku, Nagoya , Japan D. Odstrcil George Mason University, 4400 University Drive, Fairfax, VA 22030, USA and NASA/GSFC M/C 674, Greenbelt, MD 20771, USA M.M. Bisi RAL Space, STFC Rutherford Appleton Laboratory, Harwell Campus, Oxfordshire, UK J. Kim, J Yun Korean Space Weather Center, National Radio Research Agency, 198-6, Gwideok-ro, Hallim-eup, Jeju-si, Jeju-do, South Korea Masayoshi
2 Different Techniques for Measurement of Bs Bz Introduction: Bs: Definition Geocentric Solar Magnetospheric (GSM) Bz: The reasons to determine Bz Concept studies: How we may be able to determine Bz 1) In CMEs. 2) In the background solar wind Some successes in determining Bz
3 Different Techniques for Measurement of Bs Bz Introduction: Bs: Definition Geocentric Solar Magnetospheric (GSM) Bz: The reasons to determine Bz Concept studies: How we may be able to determine Bz 1) In CMEs. 2) In the background solar wind Some successes in determining Bz
4 Different Techniques for Measurement of Bs Bz Introduction: Bs: Definition Geocentric Solar Magnetospheric (GSM) Bz: The reasons to determine Bz Concept studies: How we may be able to determine Bz 1) In CMEs. 2) In the background solar wind Some successes in determining Bz
5 Why Determine Bz? Geomagnetic Substorm Activity A brief (2-3 hour) disturbance in Earth s magnetosphere that releases energy from the tail of the magnetosphere causing particles to be injected into the high latitude ionosphere. Geomagnetic Storm Activity A series of substorms, or a strong or prolonged enhancement of the global magnetospheric electric field. Both cause radio communication difficulties, particle precipitation into the ionosphere, aurora, satellite damage, ground-based currents, etc., A southward IMF is a common factor in the occurrence of both storms and substorms.
6 Generally the largest storms and substorms are associated with CMEs Two factors in CMEs are important. 1) Southward Bz. 2) Dynamic pressure caused by high speed wind.
7 CMEs Fm N. Gopalswamy
8 Fm N. Gopalswamy CMEs
9 Fm N. Gopalswamy CMEs
10 Fm N. Gopalswamy CMEs
11 Fm N. Gopalswamy CMEs
12 Fm Ward (Chip) Manchester CMEs
13 Fm Ward (Chip) Manchester CMEs
14 Fm Ward (Chip) Manchester CMEs
15 Fm Ward (Chip) Manchester CMEs
16 Fm Ward (Chip) Manchester CMEs
17 Fm Ward (Chip) Manchester CMEs
18 Fm Ward (Chip) Manchester CMEs
19 M. L. Mays & A. Taktakishvili CMEs
20 M. L. Mays & A. Taktakishvili CMEs
21 M. L. Mays & A. Taktakishvili CMEs Timing and Field Amplitude sometimes good (state of the art)
22 Fm Dusan Odstrcil CMEs
23 Fm Dusan Odstrcil CMEs Simulated CME Events
24 Fm Dusan Odstrcil CMEs CME Event Boundary Conditions
25 Fm Dusan Odstrcil CMEs CME Event Boundary Conditions
26 Fm Dusan Odstrcil CMEs CME Event Boundary Changes
27 Fm Dusan Odstrcil CMEs CME Cone vs Spheromak
28 Fm Dusan Odstrcil CMEs CME Cone vs Spheromak density Cone Spheromak Cone Spheromak
29 Fm Dusan Odstrcil CMEs Density
30 Fm Dusan Odstrcil CMEs Velocity
31 Fm Dusan Odstrcil CMEs Magnetic Field B θ
32 Heliospheric Remote Sensing IPS Heliospheric Analyses ISEE (STELab) ISEE IPS array near Mt. Fuji ISEE IPS array systems
33 Heliospheric Remote Sensing IPS Heliospheric Analyses ISEE (STELab) IPS line-of-sight response ISEE IPS array systems
34 Heliospheric Remote Sensing IPS line-of-sight response Jackson, B.V., et al., 2008, Adv. in Geosciences, 21, Heliospheric C.A.T. analyses: example line-of-sight distribution for each sky location to form the source surface of the 3D reconstruction. ISEE IPS Sample outward motion over time
35 Heliospheric Remote Sensing Jackson, B.V., et al., 2011, Adv. in Geosciences, 30, or UCSD Prediction Analyses UCSD Web pages Web analysis runs automatically using Linux on a P.C.
36 Density Heliospheric Remote Sensing UCSD Prediction ( Today s 21 UT Analysis from ISEE Density (n/cm 3 ) Radial Magnetic Field (nt) Web analysis runs Masayoshi automatically using Linux on a P.C.
37 Heliospheric Remote Sensing 2017/09/17 11:47 UT Backside halo CME sequence
38 More Details Magnetic Field
39 Heliospheric Remote Sensing (Zhao, X. P. and Hoeksema, J. T., 1995, J. Geophys. Res., 100 (A1), 19.) CSSS model Dunn et al., 2005, Solar Physics 227: Source surface B r field component sample 1. Inner region: the CSSS model calculates the magnetic field using photospheric measurements and a horizontal current model. 2. Middle region: the CSSS model opens the field lines. In the outer region. 3. Outer region: the UCSD tomography convects the magnetic field along velocity flow lines.
40 Heliospheric Remote Sensing
41 (Jackson, B.V., et al., 2015, ApJL, 803:L1. 1-5, doi: / /803/1/l1.) CSSS model Closed field Extrapolated B n closed B rt field field component for CR for 2056 CR 2056 About 1/50 th of the static flux r fall-off
42 Heliospheric Remote Sensing Φ = λ 2 n e B ds v 3-D reconstructions of Carrington rotation (CR) 2121 showing a CME of interest from 07 March 2012 launched around 01:00UT.
43 Heliospheric Remote Sensing Φ = λ 2 n e B ds v The same period extracted from CR2121 comparing IPS g-level fisheye sky map (left) with that of reconstructed RM from ambient magnetic fields (right) perturbed by the CME.
44 Oberoi and Lonsdale, 2012, Radio Science, 47, RS0K08, doi: /2012rs Faraday rotation signals at low frequency Φ = λ 2 n e B ds Heliospheric Remote Sensing From Oberoi and Lonsdale Heliospheric Signal
45 현재이이미지를표시할수없습니다. 현재이이미지를표시할수없습니다. Fm Mario Bisi Heliospheric Remote Sensing High-Band Tiles 110 to ~250 MHz. LOFAR Low-Band Dipoles ~10 to 90 MHz RAL Space
46 Fm Mario Bisi 2017 RAL Space Heliospheric FR Observation s
47 2017 RAL Space Heliospheric Remote Sensing Fm Mario Bisi Heliospheric FR Observations (3) Using simple dimensional-analysis calculations: RM = x ne[cm -3 ] x B[nT] x L[AU] m -2, where L is the contributing integration length along the LOS, we get a maximum expected RM value: RM = x 669 x 150 x 0.25 = 50.2 m -2 (or rad m -2 ); perhaps high but is very much in line with the LOFAR preliminary heliospheric RM values.
48 Interstellar Medium Variations Fm Richard Fallows Observed RM (red) and ionospheric contribution (blue) Plot courtesy Charlotte Sobey, CSIRO Heliospheric Remote Sensing Raw rotation measures (red) plus estimated ionospheric contributions (blue) After subtraction of ionosphere 800 days Day of interest Ionospheric contribution estimated using Total Electron Content (TEC) maps produced from GPS satellite data.
49 Fm Richard Fallows Heliospheric Remote Sensing RM Calculations Current Estimates Measured RM (ISM subtracted) Calculated Ionospheric RM RM difference Modelling and number checking efforts underway indicate that the resulting difference in RM, assumed to be due to the heliosphere, is in the ballpark for that expected from the passage of this CME.
50 In the meantime Choi et al., JGR, 122, 4921, doi: /2016JA for substorms of weak to medium even the weakly (in terms of either intensity or duration) southward IMF Bz should be considered significant Magnetic Field Russell - McPherron Effect Daily Implementation
51 GSM RTN coordinates (Russell, C. T., and McPherron, R. L., 1973, J. Geophys. Res., 78 (1), 92.) Sun
52 GSM RTN coordinates (Russell, C. T., and McPherron, R. L., 1973, J. Geophys. Res., 78 (1), 92.) Sun
53 (see: UCSD Prediction Analyses Last March Analyses from ISEE: Day -4 Bz (GSM) Four Days In Future From here Web analysis runs automatically using Linux on a P.C.
54 (see: UCSD Prediction Analyses Last March Analyses from ISEE: Day -3 Bz (GSM) Three Days In Future From here Web analysis runs automatically using Linux on a P.C.
55 (see: UCSD Prediction Analyses Last March Analyses from ISEE: Day -2 Two Days In Future Bz (GSM) From here Web analysis runs automatically using Linux on a P.C.
56 (see: UCSD Prediction Analyses Last March Analyses from ISEE: Day -1 One Day In Future Bz (GSM) From here Web analysis runs automatically using Linux on a P.C.
57 (see: UCSD Prediction Analyses Last March Analyses from ISEE: Day -1 No Days In Future Bz (GSM) Web analysis runs automatically using Linux on a P.C.
58 (see: UCSD Predictions Magnetic Field Analysis No Days In Future NOAA Bz (GSM) Kp Web analysis runs automatically using Linux on a P.C.
59 ACE and IPS-derived Bz Pearson s R Correlation per Carrington Rotation in GSM Coordinates over Ten Years Positive Correlations (over 10 years)
60 (Russell, C. T., and McPherron, R. L., 1973, J. Geophys. Res., 78 (1), 92.) 10 years of ACE data Bz Amplitude in GSM coordinates 10 years of GONG data IPS extrapolation
61 UCSD Prediction Analyses Study Dst vs GSM Bz (CR 2074) Kp vs GSM Bz R = 0.64 R = 0.67 ACE Dst Kp ACE Bz R = 0.52 IPS ACE Bz R = 0.35 IPS-derived Bz IPS-derived Bz
62 UCSD Prediction Analyses Study Dst vs GSM Bz (CR 2083) Kp vs GSM Bz R = 0.39 R = 0.67 ACE Dst ACE Bz IPS ACE Bz Dst Kp Kp R = 0.52 R = 0.38 IPS-derived Bz IPS-derived Bz
63 Can t possibly be right - a good NOAA colleague GSM Bz Largest min -Bz -17nT 09 UT 03/27 (Perhaps)
64 GSM Bz UCSD current prediction Maybe Maybe
65 Conclusions: Geocentric Solar Magnetospheric (GSM) Bz: The reasons to determine Bz Concept studies: How we may be able to determine Bz 1) In CMEs. 2) In the background solar wind Now there are some successes in determining Bz
CHAPTER 1 INTRODUCTION
CHAPTER 1 INTRODUCTION The dependence of society to technology increased in recent years as the technology has enhanced. increased. Moreover, in addition to technology, the dependence of society to nature
More informationREPORT DOCUMENTATION PAGE. IPS Space Weather Research. Mr. Jung Hoon Kim N/A AOARD UNIT APO AP AFRL/AFOSR/IOA(AOARD)
REPORT DOCUMENTATION PAGE Form Approved OMB No. 0704-0188 The public reporting burden for this collection of information is estimated to average 1 hour per response, including the time for reviewing instructions,
More informationScientific 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
More informationStudy of the Ionosphere Irregularities Caused by Space Weather Activity on the Base of GNSS Measurements
Study of the Ionosphere Irregularities Caused by Space Weather Activity on the Base of GNSS Measurements Iu. Cherniak 1, I. Zakharenkova 1,2, A. Krankowski 1 1 Space Radio Research Center,, University
More informationSUNHAK HONG, KICHANG YOON, SUNGWON PARK, YUNG-KYU KIM, Seung-man Choi
SUNHAK HONG, KICHANG YOON, SUNGWON PARK, YUNG-KYU KIM, Seung-man Choi SWx Operations operational work flow Observation Ionosondes (x2) & TEC (x5) Mag (x3) Products 1639 Subscribers (Dec. 31, 2013) Satellite
More informationRegional 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
More informationStudy 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
More informationMonitoring 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
More information[titlelscientific Studies of the High-Latitude Ionosphere with the Ionosphere Dynamics and Electrodynamics-Data Assimilation (IDED-DA) Model
[titlelscientific Studies of the High-Latitude Ionosphere with the Ionosphere Dynamics and Electrodynamics-Data Assimilation (IDED-DA) Model [awardnumberl]n00014-13-l-0267 [awardnumber2] [awardnumbermore]
More informationThe 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
More informationESS 7 Lectures 15 and 16 November 3 and 5, The Atmosphere and Ionosphere
ESS 7 Lectures 15 and 16 November 3 and 5, 2008 The Atmosphere and Ionosphere The Earth s Atmosphere The Earth s upper atmosphere is important for groundbased and satellite radio communication and navigation.
More informationSPACE 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
More informationThe low latitude ionospheric effects of the April 2000 magnetic storm near the longitude 120 E
Earth Planets Space, 56, 67 612, 24 The low latitude ionospheric effects of the April 2 magnetic storm near the longitude 12 E Libo Liu 1, Weixing Wan 1,C.C.Lee 2, Baiqi Ning 1, and J. Y. Liu 2 1 Institute
More informationInfluence of Major Geomagnetic Storms Occurred in the Year 2011 On TEC Over Bangalore Station In India
International Journal of Electronics and Communication Engineering. ISSN 0974-2166 Volume 6, Number 1 (2013), pp. 105-110 International Research Publication House http://www.irphouse.com Influence of Major
More information2 nd ICAO/UNOOSA Symposium, March 2016, Abu Dhabi, UAE. Space Weather. Sharafat Gadimova Office for Outer Space Affairs
2 nd ICAO/UNOOSA Symposium, 15 17 March 2016, Abu Dhabi, UAE Space Weather Sharafat Gadimova Office for Outer Space Affairs Science, Capacity Building and Outreach 2004: Session of the Committee on the
More informationDate(2002) proton flux Dst (pfu) 11-Jan nt 23-May nt 17-Jul nt 22-Aug nt 7-Sep nt 10-Nov nt 21-Apr nt
3.1 Solar energetic particles effect on the Earth/ionosphere in quiet geomagnetic condition Paul J Marchese, Donald E. Cotten *, and Tak David Cheung City University of New York Queensborough Community
More informationMulti-instrument observations of atmospheric gravity waves/traveling ionospheric disturbances associated with enhanced auroral activity
Multi-instrument observations of atmospheric gravity waves/traveling ionospheric disturbances associated with enhanced auroral activity Zama Katamzi-Joseph *, Anasuya Aruliah, Kjellmar Oksavik, John Bosco
More informationIonospheric 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,
More informationThe Earth s Atmosphere
ESS 7 Lectures 15 and 16 May 5 and 7, 2010 The Atmosphere and Ionosphere The Earth s Atmosphere The Earth s upper atmosphere is important for groundbased and satellite radio communication and navigation.
More informationThe 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
More informationWhat is Space Weather? THE ACTIVE SUN
Aardvark Roost AOC Space Weather in Southern Africa Hannes Coetzee 1 What is Space Weather? THE ACTIVE SUN 2 The Violant Sun 3 What is Space Weather? Solar eruptive events (solar flares, coronal Mass Space
More informationESS 7. Lectures 18, 19 and 20 November 14, 17 and 19. Technology and Space Weather
ESS 7 Lectures 18, 19 and 20 November 14, 17 and 19 Technology and Space Weather Space Weather Effects on Satellite Lifetimes: Atmospheric Drag A satellite would orbit forever if gravity was the only force
More informationIonospheric response to the space weather event of 18 November An investigation
Indian Journal of Radio & Space Physics Vol. 39, October 2010, pp. 290-295 Ionospheric response to the space weather event of 18 November 2003 - An investigation Pankaj Kumar 1,$, Wahab Uddin 1, Alok Taori
More informationModeling of Ionospheric Refraction of UHF Radar Signals at High Latitudes
Modeling of Ionospheric Refraction of UHF Radar Signals at High Latitudes Brenton Watkins Geophysical Institute University of Alaska Fairbanks USA watkins@gi.alaska.edu Sergei Maurits and Anton Kulchitsky
More informationUsing 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
More informationThe ionosphere weather service SWACI and its capability for estimating propagation effects of transionospheric radio signals
The ionosphere weather service SWACI and its capability or estimating propagation eects o transionospheric radio signals Norbert Jakowski Institute o Communications und Navigation German Aerospace Center
More informationCHARGED: An NSF-Funded Initiative to Understand the Physics of Extreme GICs Michael W. Liemohn
CHARGED: An NSF-Funded Initiative to Understand the Physics of Extreme GICs Michael W. Liemohn Department of Climate and Space Sciences and Engineering University of Michigan, Ann Arbor, MI Dan Welling,
More informationAnalysis of Ionospheric Anomalies due to Space Weather Conditions by using GPS-TEC Variations
Presented at the FIG Congress 2018, May 6-11, 2018 in Istanbul, Turkey Analysis of Ionospheric Anomalies due to Space Weather Conditions by using GPS-TEC Variations Asst. Prof. Dr. Mustafa ULUKAVAK 1,
More informationAnna Belehaki, Ioanna Tsagouri (NOA, Greece) Ivan Kutiev, Pencho Marinov (BAS, Bulgaria)
Characteristics of Large Scale Travelling Ionospheric Disturbances Exploiting Ground-Based Ionograms, GPS-TEC and 3D Electron Density Distribution Maps Anna Belehaki, Ioanna Tsagouri (NOA, Greece) Ivan
More informationROTI 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,
More informationand 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.
More informationarxiv: v1 [astro-ph.im] 16 Aug 2016
Separating Nightside Interplanetary and Ionospheric Scintillation with LOFAR arxiv:1608.04504v1 [astro-ph.im] 16 Aug 2016 R.A. Fallows ASTRON - the Netherlands Institute for Radio Astronomy, Postbus 2,
More informationUsing the Radio Spectrum to Understand Space Weather
Using the Radio Spectrum to Understand Space Weather Ray Greenwald Virginia Tech Topics to be Covered What is Space Weather? Origins and impacts Analogies with terrestrial weather Monitoring Space Weather
More informationVariability in the response time of the high-latitude ionosphere to IMF and solar-wind variations
Variability in the response time of the high-latitude ionosphere to IMF and solar-wind variations Murray L. Parkinson 1, Mike Pinnock 2, and Peter L. Dyson 1 (1) Department of Physics, La Trobe University,
More informationStorms 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
More informationSolar 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
More information100-year GIC event scenarios. Antti Pulkkinen and Chigomezyo Ngwira The Catholic University of America & NASA Goddard Space Flight Center
100-year GIC event scenarios Antti Pulkkinen and Chigomezyo Ngwira The Catholic University of America & NASA Goddard Space Flight Center 1 Contents Objectives. Approach. Identification of four key factors
More informationIonospheric and cosmic ray monitoring: Recent developments at the RMI
Solar Terrestrial Centre of Excellence Ionospheric and cosmic ray monitoring: Recent developments at the RMI Danislav Sapundjiev, Stan Stankov, Tobias Verhulst, Jean-Claude Jodogne Royal (RMI) Ringlaan
More informationPulsar polarimetry. with. Charlotte Sobey. Dr. Aris Noutsos & Prof. Michael Kramer
Pulsar polarimetry with Dr. Aris Noutsos & Prof. Michael Kramer Outline Introduction Observations Ionosphere Outline Pulsars as objects Pulsars as probes of the ISM Faraday rotation using RM synthesis
More informationIntroduction to ILWS. George Withbroe. Office of Space Science Sun Earth Connection Division NASA Headquarters
Introduction to ILWS George Withbroe Office of Space Science Sun Earth Connection Division NASA Headquarters GOAL: Stimulate and strengthen research in solar-terrestrial physics to improve understanding
More informationNational Radio Research Agency
Feb 22. 2012 Korean Space Weather Center National Radio Research Agency Ⅰ. Korean Space Weather Center Ⅱ. Space Weather in Korea Ⅲ. Vision & Goal in 24 th Solar Cycle [1] Forecasting & Warning Service
More informationDaily 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
More informationThe frequency variation of Pc5 ULF waves during a magnetic storm
Earth Planets Space, 57, 619 625, 2005 The frequency variation of Pc5 ULF waves during a magnetic storm A. Du 1,2,W.Sun 2,W.Xu 1, and X. Gao 3 1 Institute of Geology and Geophysics, Chinese Academy of
More informationRadio Astronomy and the Ionosphere
Radio Astronomy and the Ionosphere John A Kennewell, Mike Terkildsen CAASTRO EoR Global Signal Workshop November 2012 THE IONOSPHERE UPPER ATMOSPHERIC PLASMA - The ionosphere is a weak (1%) variable plasma
More informationThe 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?
More informationJames M Anderson. in collaboration with Jan Noordam and Oleg Smirnov. MPIfR, Bonn, 2006 Dec 07
Ionospheric Calibration for Long-Baseline, Low-Frequency Interferometry in collaboration with Jan Noordam and Oleg Smirnov Page 1/36 Outline The challenge for radioastronomy Introduction to the ionosphere
More informationKiChang Yoon, Sunhak Hong, Yongki Kwon, Gwan-sik Wi
53th COPUOS Scientific and Technical Subcommittee Space Weather Expert Group 15-17 February 2016 KiChang Yoon, Sunhak Hong, Yongki Kwon, Gwan-sik Wi Contents 1. SWx Operations 2. Tailored Services 3. National
More informationSpace weather: A research grand challenge. Professor Jøran Moen (GCI-Cusp project scientist)
Space weather: A research grand challenge Professor Jøran Moen (GCI-Cusp project scientist) Birkeland Space Weather Symposium 15 JUNE 2017 Outline: Space weather phenomena in cusp Research Grand Challenges
More informationActivities of the JPL Ionosphere Group
Activities of the JPL Ionosphere Group On-going GIM wor Submit rapid and final GIM TEC maps for IGS combined ionosphere products FAA WAAS & SBAS analysis Error bounds for Brazilian sector, increasing availability
More informationMWA Ionospheric Science Opportunities Space Weather Storms & Irregularities (location location location) John Foster MIT Haystack Observatory
MWA Ionospheric Science Opportunities Space Weather Storms & Irregularities (location location location) John Foster MIT Haystack Observatory Storm Enhanced Density: Longitude-specific Ionospheric Redistribution
More informationA dynamic system to forecast ionospheric storm disturbances based on solar wind conditions
ANNALS OF GEOPHYSICS, VOL. 48, N. 3, June 2005 A dynamic system to forecast ionospheric storm disturbances based on solar wind conditions Ioanna Tsagouri ( 1 ), Anna Belehaki ( 1 ) and Ljiljana R. Cander
More informationMay 2012 Solar Activity ~ Radio and Geomagnetic Effects Whitham D. Reeve ( 2012 W. Reeve)
May 2012 Solar Activity ~ Radio and Geomagnetic Effects Whitham D. Reeve ( 2012 W. Reeve) Abbreviations in this article: ACE: Advanced Composition Explorer AGC: Automatic Gain Control CME: Coronal Mass
More informationEffects of the solar wind electric field and ionospheric conductance on the cross polar cap potential: Results of global MHD modeling
GEOPHYSICAL RESEARCH LETTERS, VOL. 30, NO. 23, 2180, doi:10.1029/2003gl017903, 2003 Effects of the solar wind electric field and ionospheric conductance on the cross polar cap potential: Results of global
More informationConvection Development in the Inner Magnetosphere-Ionosphere Coupling System
Convection Development in the Inner Magnetosphere-Ionosphere Coupling System Hashimoto,K.K. Alfven layer Tanaka Department of Environmental Risk Management, School of Policy Management, Kibi International
More informationElectrodynamics in the Mid-Latitudes. Anthea Coster, MIT Haystack Observatory
Electrodynamics in the Mid-Latitudes Anthea Coster, MIT Haystack Observatory References Kelley, M. C. 1989; 2009. The Earth's ionosphere: Plasma physics and electrodynamics. International Geophysics Series,
More informationIES 2015, May 12-14, Old Town Alexandria. Geomagnetic Laboratory, Natural Resources Canada 2. Geodetic Survey, Natural Resources Canada
Analyses of the geomagnetic variations and GPS scintillation over the Canadian auroral zone Lidia Nikitina 1, D.W. Danskin 1, R. Ghoddousi-Fard 2, P. Prikryl 1 1 Geomagnetic Laboratory, Natural Resources
More informationSpace 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
More informationIonospheric Propagation
Ionospheric Nick Massey VA7NRM 1 Electromagnetic Spectrum Radio Waves are a form of Electromagnetic Radiation Visible Light is also a form of Electromagnetic Radiation Radio Waves behave a lot like light
More informationanalysis of GPS total electron content Empirical orthogonal function (EOF) storm response 2016 NEROC Symposium M. Ruohoniemi (3)
Empirical orthogonal function (EOF) analysis of GPS total electron content storm response E. G. Thomas (1), A. J. Coster (2), S.-R. Zhang (2), R. M. McGranaghan (1), S. G. Shepherd (1), J. B. H. Baker
More informationModeling and Subionospheric VLF perturbations caused by direct and indirect effects of lightning
Modeling and Subionospheric VLF perturbations caused by direct and indirect effects of lightning Prepared by Benjamin Cotts Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global
More informationIonospheric Storm Effects in GPS Total Electron Content
Ionospheric Storm Effects in GPS Total Electron Content Evan G. Thomas 1, Joseph B. H. Baker 1, J. Michael Ruohoniemi 1, Anthea J. Coster 2 (1) Space@VT, Virginia Tech, Blacksburg, VA, USA (2) MIT Haystack
More informationOperational 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.
More informationThe Effect of Geomagnetic Storm in the Ionosphere using N-h Profiles.
The Effect of Geomagnetic Storm in the Ionosphere using N-h Profiles. J.C. Morka * ; D.N. Nwachuku; and D.A. Ogwu. Physics Department, College of Education, Agbor, Nigeria E-mail: johnmorka84@gmail.com
More informationMEETING 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
More informationThe ICG, Multifunction GNSS Signals and How To Protect Them. Space Weather Studies Using GNSS and Space Science Outreach activities at Sangli
4 th EUROPEAN SPACE SOLUTIONS The ICG, Multifunction GNSS Signals and How To Protect Them Space Weather Studies Using GNSS and Space Science Outreach activities at Sangli D. J. SHETTI DEPARTMENT OF PHYSICS,
More informationThe importance of ground magnetic data in specifying the state of magnetosphere ionosphere coupling: a personal view
DOI 10.1186/s40562-016-0042-7 REVIEW Open Access The importance of ground magnetic data in specifying the state of magnetosphere ionosphere coupling: a personal view Y. Kamide 1,2* and Nanan Balan 3 Abstract
More informationSpace 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
More informationSNIPE mission for Space Weather Research. CubeSat Developers Workshop 2017 Jaejin Lee (KASI)
SNIPE mission for Space Weather Research CubeSat Developers Workshop 2017 Jaejin Lee (KASI) New Challenge with Nanosatellites In observing small-scale plasma structures, single satellite inherently suffers
More informationGeomagnetic Disturbances. IEEE PES Chicago Chapter Technical Presentation March 12, Alan Engelmann Transmission Planning ComEd.
Geomagnetic Disturbances IEEE PES Chicago Chapter Technical Presentation March 12, 2014 Alan Engelmann Transmission Planning ComEd GMD Background Solar Disturbances Impacts Monitoring Events 2 Solar Disturbances
More informationGeomagnetic observations and ionospheric response during storm on 14 April 2006
Indian Journal of Radio & Space Physics Vol 39, April 2010, pp 71-79 Geomagnetic observations and ionospheric response during storm on 14 April 2006 N O Bakare $,*, V U Chukwuma & B J Adekoya Department
More informationDetecting 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
More informationGround 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
More information4/29/2012. General Class Element 3 Course Presentation. Radio Wave Propagation. Radio Wave Propagation. Radio Wave Propagation.
General Class Element 3 Course Presentation ti ELEMENT 3 SUB ELEMENTS General Licensing Class Subelement G3 3 Exam Questions, 3 Groups G1 Commission s Rules G2 Operating Procedures G3 G4 Amateur Radio
More informationMeasuring Total Electron Content. Investigation of Two Different Techniques
Measuring Total Electron Content with GNSS: Investigation of Two Different Techniques Benoît Bidaine 1 F.R.S. FNRS B.Bidaine@ulg.ac.be Prof. René Warnant 1,2 R.Warnant@oma.be 1 University of Liège (Unit
More informationIonospheric 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,
More informationNON-TYPICAL SERIES OF QUASI-PERIODIC VLF EMISSIONS
NON-TYPICAL SERIES OF QUASI-PERIODIC VLF EMISSIONS J. Manninen 1, N. Kleimenova 2, O. Kozyreva 2 1 Sodankylä Geophysical Observatory, Finland, e-mail: jyrki.manninen@sgo.fi; 2 Institute of Physics of the
More informationModeling the ionospheric response to the 28 October 2003 solar flare due to coupling with the thermosphere
RADIO SCIENCE, VOL. 44,, doi:10.1029/2008rs004081, 2009 Modeling the ionospheric response to the 28 October 2003 solar flare due to coupling with the thermosphere David J. Pawlowski 1 and Aaron J. Ridley
More informationEFFECTS 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
More informationRecent results of EMIC/ELF/VLF wave measurements at Athabasca (L=4.2), Canada. Kazuo Shiokawa (ISEE, Nagoya Univ.) Martin Connors (Athabasca Univ.
Recent results of EMIC/ELF/VLF wave measurements at Athabasca (L=4.2), Canada Kazuo Shiokawa (ISEE, Nagoya Univ.) Martin Connors (Athabasca Univ.) Athabasca (September 3, 2005-) all-sky imager meridian-scanning
More informationSatellite 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
More informationPropagation Tool.
Propagation Propagation Tool http://www.hamqsl.com/solar.html The Ionosphere is made up of several layers at varying heights above the ground: The lowest level is the D Layer (37 to 56 miles), which
More informationEarthquake Analysis over the Equatorial
Earthquake Analysis over the Equatorial Region by Using the Critical Frequency Data and Geomagnetic Index Earthquake Analysis over the Equatorial Region by Using the Critical Frequency Data and Geomagnetic
More informationEvaluating Transformer Heating due to Geomagnetic Disturbances
Evaluating Transformer Heating due to Geomagnetic Disturbances Presented by: Brian Penny, American Transmission Company 53 rd Annual Minnesota Power Systems Conference November 7, 2017 atcllc.com Presentation
More informationIntroduction to International Space Weather Initiative (ISWI) and China's Participation (Meridian Project)
Introduction to International Space Weather Initiative (ISWI) and China's Participation (Meridian Project) Chi Wang National Space Science Center, CAS Nov. 7, 2012 Outline What is Space Weather? International
More informationNear Earth space monitoring with LOFAR PL610 station in Borówiec
Near Earth space monitoring with LOFAR PL610 station in Borówiec Hanna Rothkaehl 1, Mariusz Pożoga 1, Marek Morawski 1, Barbara Matyjasiak 1, Dorota Przepiórka 1, Marcin Grzesiak 1 and Roman Wronowski
More informationA generic description of planetary aurora
A generic description of planetary aurora J. De Keyser, R. Maggiolo, and L. Maes Belgian Institute for Space Aeronomy, Brussels, Belgium Johan.DeKeyser@aeronomie.be Context We consider a rotating planetary
More informationPersonal Space Weather Station
Personal Space Weather Station Nathaniel A. Frissell, W2NAF 1 1 New Jersey Institute of Technology, K2MFF Introduction Space Weather is a common interest of hams, scientists, and engineers. By studying
More informationGeneral Classs Chapter 7
General Classs Chapter 7 Radio Wave Propagation Bob KA9BHD Eric K9VIC Learning Objectives Teach you enough to get all the propagation questions right during the VE Session Learn a few things from you about
More information1. Introduction. 2. Materials and Methods
A Study On The Detection Of Solar Flares And Its Effects On The Daytime Fluctuation Of VLF Amplitude And Geomagnetic Variation Using A Signal Of 22.10 KHz Transmitted From England And Received At Kiel
More informationLEO GPS Measurements to Study the Topside Ionospheric Irregularities
LEO GPS Measurements to Study the Topside Ionospheric Irregularities Irina Zakharenkova and Elvira Astafyeva 1 Institut de Physique du Globe de Paris, Paris Sorbonne Cité, Univ. Paris Diderot, UMR CNRS
More informationRadioastronomy in Space with Cubesats
Radioastronomy in Space with Cubesats Baptiste Cecconi (1), Philippe Zarka (1), Marc Klein Wolt (2), Jan Bergman (3), Boris Segret (1) (1) LESIA, CNRS-Observatoire de Paris, France (2) Radboud University
More informationAWESOME for educational and research use
SuperSID - a small-version AWESOME for educational and research use By Deborah Scherrer Tim Huynh Stanford University Solar Center 1 What I am going to talk about What is this project? What can the instrument
More informationNVIS PROPAGATION THEORY AND PRACTICE
NVIS PROPAGATION THEORY AND PRACTICE Introduction Near-Vertical Incident Skywave (NVIS) propagation is a mode of HF operation that utilizes a high angle reflection off the ionosphere to fill in the gap
More informationA Beginner s Guide to Space Weather and GPS Updated February 21, 2008 Professor Paul M. Kintner, Jr. with acknowledgements to
A Beginner s Guide to Space Weather and GPS Updated February 1, 008 Professor Paul M. Kintner, Jr. with acknowledgements to M. Psiaki, T. Humphreys, A. Cerruti, B. Ledvina, A. Mannucci, D. Gary, E. de
More informationChapter 2 Analysis of Polar Ionospheric Scintillation Characteristics Based on GPS Data
Chapter 2 Analysis of Polar Ionospheric Scintillation Characteristics Based on GPS Data Lijing Pan and Ping Yin Abstract Ionospheric scintillation is one of the important factors that affect the performance
More informationMagnetosphere Ionosphere Coupling and Substorms
Chapter 10 Magnetosphere Ionosphere Coupling and Substorms 10.1 Magnetosphere-Ionosphere Coupling 10.1.1 Currents and Convection in the Ionosphere The coupling between the magnetosphere and the ionosphere
More informationThe impact of geomagnetic substorms on GPS receiver performance
LETTER Earth Planets Space, 52, 1067 1071, 2000 The impact of geomagnetic substorms on GPS receiver performance S. Skone and M. de Jong Department of Geomatics Engineering, University of Calgary, 2500
More informationHAARP Generated ELF/VLF Waves for Magnetospheric Probing. Mark Gołkowski
HAARP Generated ELF/VLF Waves for Magnetospheric Probing Mark Gołkowski University of Colorado Denver M.B. Cohen, U. S. Inan, D. Piddyachiy Stanford University RF Ionospheric Workshop 20 April 2010 Outline
More informationTo Estimate The Regional Ionospheric TEC From GEONET Observation
To Estimate The Regional Ionospheric TEC From GEONET Observation Jinsong Ping(Email: jsping@miz.nao.ac.jp) 1,2, Nobuyuki Kawano 2,3, Mamoru Sekido 4 1. Dept. Astronomy, Beijing Normal University, Haidian,
More informationBeamforming for IPS and Pulsar Observations
Beamforming for IPS and Pulsar Observations Divya Oberoi MIT Haystack Observatory Sunrise at Mileura P. Walsh Function, Inputs and Outputs Function - combine the voltage signal from each of the 512 tiles
More information