Real time reconstruction of 3-D electron density distribution over Europe with TaD profiler Ivan Kutiev 1,2, Pencho Marinov 1, Anna Belehaki 2 1 Bulgarian.

Slides:



Advertisements
Similar presentations
Modelling complexity in the upper atmosphere using GPS data Chris Budd, Cathryn Mitchell, Paul Spencer Bath Institute for Complex Systems, University of.
Advertisements

Near real time assessment of the Space Weather effect on navigation based on the DGPS technique S.Lejeune, R.Warnant, A. Barré, M. Bavier Royal Observatory.
In the frame of the SIDC Space Weather Pilot Project, the Royal Observatory of Belgium, the Royal Meteorological Institute of Belgium and the Geophysical.
HF management communication system and link optimization Bruno Zolesi. Istituto Nazionale di Geofisica e Vulcanologia.
Introduction to the Ionosphere
European Digital Upper Atmosphere Server DIAS A project co-funded by the eContent programme of the European Commission.
B. Nava, S.M. Radicella, R. Leitinger and P.Coïsson The Abdus Salam ICTP, Trieste, Italy IGAM, Graz, Austria XXVIII General Assembly of International Union.
URSIGA, New Delhi, Oct 2005 Coordinated Observations of Ionospheric Scintillations, Density Profiles and Total Electron Content on a Common Magnetic.
Using a DPS as a Coherent Scatter HF Radar Lindsay Magnus Lee-Anne McKinnell Hermanus Magnetic Observatory Hermanus, South Africa.
I. U. Observatorio del Ebro, Universitat Ramon Llull Center for Atmospheric Research, University of Massachusets Lowell IRI/COST 296 WORKSHOP; July.
Comparative Study of the Global Ionospheric Behavior During Solar Cycles and Minima Eduardo A. Araujo-Pradere 1,2, Dominic Fuller-Rowell 1,3,
Anna Belehaki National Observatory of Athens, Greece Fifth European Space Weather Week, Brussels, November 2008.
Further development of modeling of spatial distribution of energetic electron fluxes near Europa M. V. Podzolko 1, I. V. Getselev 1, Yu. I. Gubar 1, I.
Status of GNSS ionospheric Study in Korea
PROBABILISTIC ASSESSMENT OF THE QSAR APPLICATION DOMAIN Nina Jeliazkova 1, Joanna Jaworska 2 (1) IPP, Bulgarian Academy of Sciences, Sofia, Bulgaria (2)
DIAS home page Second European Space Weather Week, ESTEC, Noordwijk, The Netherlands, November 2005 European Digital.
University of Wisconsin-Milwaukee Geographic Information Science Geography 625 Intermediate Geographic Information Science Instructor: Changshan Wu Department.
Abstract Since the ionosphere is the interface between the Earth and space environments and impacts radio, television and satellite communication, it is.
DCABES 2009 China University Of Geosciences 1 The Parallel Models of Coronal Polarization Brightness Calculation Jiang Wenqian.
IRI Model Introduction NCU, Institute of Space Science.
Mesoscale ionospheric tomography over Finland Juha-Pekka Luntama Finnish Meteorological Institute Cathryn Mitchell, Paul Spencer University of Bath 4th.
1 Institute of High Energy Physics 13/09/2010 Comparison and Study in Measurement Accuracy of Height Difference between Laser Tracker and Level Men LingLing.
Abstract has 6 upper air stations for GPS S SR2K2 Modemwith Radiosonde M2K2_DC, 6 Upper Air stations of RDF Radiotidolite RT20A ( Vaisala ) and three Upper.
Sandro M. Radicella Head, Aeronomy and radiopropagation Laboratory Ionospheric Research at the Abdus Salam ICTP Aeronomy and Radiopropagation Laboratory.
Ionospheric Services The Australian Bureau of Meteorology, Space Weather Services setion (formerly the Ionospheric Prediction Service, IPS) provides a.
Effects of ionospheric small- scale structures on GNSS G. WAUTELET Royal Meteorological Institute of Belgium Ionospheric Radio Systems & Techniques (IRST)
EGU General Assembly 2013, 7 – 12 April 2013, Vienna, Austria This study: is pioneer in modeling the upper atmosphere, using space geodetic techniques,
Altitude (km) January Global AverageTemperature (K) Pressure (hPa) With O( 3 P) Cooling WACCM-X The Whole Atmosphere Community Climate Model – eXtended.
5 th European Space Weather Week, November 2008, Brussels Operational implementation of the SWIF model in DIAS system Tsagouri Ioanna Koutroumbas.
Ground-based ionospheric networks in Europe Ljiljana R. Cander.
P. Wielgosz and A. Krankowski IGS AC Workshop Miami Beach, June 2-6, 2008 University of Warmia and Mazury in Olsztyn, Poland
Joint International GRACE Science Team Meeting and DFG SPP 1257 Symposium, Oct. 2007, GFZ Potsdam Folie 1 Retrieval of electron density profiles.
ROSA – ROSSA Validation results R. Notarpietro, G. Perona, M. Cucca
GALOCAD GAlileo LOcal Component for nowcasting and forecasting Atmospheric Disturbances R. Warnant*, G. Wautelet*, S. Lejeune*, H. Brenot*, J. Spits*,
Data Assimilation for the Space Environment Ludger Scherliess Center for Atmospheric and Space Sciences Utah State University Logan, Utah GEM.
VARIABILITY OF TOTAL ELECTRON CONTENT AT EUROPEAN LATITUDES A. Krankowski(1), L. W. Baran(1), W. Kosek (2), I. I. Shagimuratov(3), M. Kalarus (2) (1) Institute.
Comparison of the electron density profiles measured with the Incoherent Scatter Radar, Digisonde DPS-4 and Chirp-Ionosonde Ratovsky K.G., Shpynev* B.G.,
Michael Pezzopane et al. Assimilation of autoscaled data and regional and local ionospheric models as input source for a real-time 3-D IRI modeling: additional.
Ionospheric Assimilation Model for Space Weather Monitoring and Forecasting I. T. Lee 1 W. H. Chen 2, T. Matsuo 3,4, C. H. Chang 2,
Abstract/INTRODUCTION Electron density (ED) data returned by the ARIEL 3 and ARIEL 4 Satellites have been separated into seasonal, diurnal, longitudinal.
Electron density profile retrieval from RO data Xin’an Yue, Bill Schreiner  Abel inversion error of Ne  Data Assimilation test.
Data Assimilation Retrieval of Electron Density Profiles from Radio Occultation Measurements Xin’an Yue, W. S. Schreiner, Jason Lin, C. Rocken, Y-H. Kuo.
COSMIC Ionospheric measurements Jiuhou Lei NCAR ASP/HAO Research review, Boulder, March 8, 2007.
© Copyright QinetiQ limited 2006 On the application of meteorological data assimilation techniques to radio occultation measurements of.
Swedish Institute of Space Physics, Kiruna M. Yamauchi 1 Different Sun-Earth energy coupling between different solar cycles Acknowledgement:
GALOCAD GAlileo LOcal Component for nowcasting and forecasting Atmospheric Disturbances R. Warnant, G. Wautelet, S. Lejeune, H. Brenot, J. Spits, S. Stankov.
Thermospheric density variations due to space weather Tiera Laitinen, Juho Iipponen, Ilja Honkonen, Max van de Kamp, Ari Viljanen, Pekka Janhunen Finnish.
Michael Pezzopane et al.SIF 2015 – 24 September 2015 Importance of a real-time monitoring of the Earth's ionosphere M. Pezzopane, J.A. Baskaradas, C. Bianchi,
Tsagouri I. 1, A. Belehaki 1, N. Bergeot 2,3, C. Cid 4, V. Delouille 2,3 T. Egorova 5, N. Jakowski 6, I. Kutiev 7, A. Mikhailov 8, M. Nunez 9, M. Pietrella.
A revised formulation of the COSMO surface-to-atmosphere transfer scheme Matthias Raschendorfer COSMO Offenbach 2009 Matthias Raschendorfer.
Interminimum Changes in Global Total Electron Content and Neutral Mass Density John Emmert, Sarah McDonald Space Science Division, Naval Research Lab Anthony.
S. Datta-Barua, Illinois Institute of Technology G. S. Bust, JHUAPL
Status of GNSS ionospheric Study in Korea
Atmosphere-Ionosphere Wave Coupling as Revealed in Swarm Plasma Densities and Drifts Jeffrey M. Forbes Department of Aerospace Engineering Sciences, University.
D. E. Shemansky† , J. A. Kammer ‡ , X. Zhang ‡ & Y. L. Yung‡
The Space Weather and Navigation Systems (SWANS) project
Recent progress of WDC for Geophysics, Beijing
HF radio sounding the horizontally inhomogeneous ionosphere
Ionospheric Models Levan Lomidze Center for Atmospheric and Space Sciences Utah State University CEDAR-GEM Student Workshop, June.
Center for Atmospheric & Space Sciences
Joe Comberiate Larry Paxton JHU/APL June 28, 2007
Prospects for real-time physics-based thermosphere ionosphere models for neutral density specification and forecast Tim Fuller-Rowell, Mariangel Fedrizzi,
“Consolidation of the Surface-to-Atmosphere Transfer-scheme: ConSAT
Mid-latitude Electron Density Variations Under Magnetospheric Substorm Conditions As Determined From Istanbul Dynasonde Observations Aysegul Ceren MORAL,
Lessons Learned in Developing the USU Kalman GAIM J. J. Sojka, R. W
R. Warnant*, G. Wautelet*, S. Lejeune*, H. Brenot*,
Earth’s Ionosphere Lecture 13
Ionosphere References: Prolss: Chap. 4, P (main)
Exploring the ionosphere of Mars
Evaluation of IRI-2012 by comparison with JASON-1 TEC and incoherent scatter radar observations during the solar minimum period Eun-Young Ji,
Presentation transcript:

Real time reconstruction of 3-D electron density distribution over Europe with TaD profiler Ivan Kutiev 1,2, Pencho Marinov 1, Anna Belehaki 2 1 Bulgarian Academy of Sciences 2 National Observatory of Athens

The core Topside Sounder Model (TSM) and TSM profiler (TSMP) TSM (Topside Sounder Model) provids - topside scale height H T, - upper (O + -H + ) transition height h T, - (scale height)/(transition height) ratio R T TSMP (Topside Sounder Model Profiler) provides the shape of the vertical electron density (Ne) profile in topside ionosphere and plasmasphere as a sum of O + and H + individual profiles. When the density and height of the F layer peak are specified, TSMP defines the Ne profile. Hp HTHT

TSMP-assisted Digisonde profiler (TaD) In the topside: TSMP provides the shape of Ne profile At F layer peak: Digisonde provides NmF2, and hmF2 The new coupled profiler is named TSMP-assisted Digisonde (TaD) profiler. TaD now provides electron density profiles in topside ionosphere and plasmasphere at the time of Digisonde sounding, e.g. in real time.

Digisonde and TaD topside profiles Digisonde topside profile is expressed by the α-Chapman formula. At higher altitudes the profile decreases with a scale height 2Hm (Hm is the neutral scale height). The O + scale height H T, provided by TaD is approximately 1.25 times larger than Hm.

Further improvement of TaD Modeling the He + profile around transition height h T Modeling the Hp/H T ratio as a function of geomagnetic latitude, month, local time, and O + density at transition height h T (using ISIS-1 topside sounder Ne profiles) Profile parameters Hp and h T are presented by their ratios with H T, so the shape of the whole TaD profile is made dependent on H T only. Adjustment of the integral of TaD profile with measured GNSS- TEC.

Using TaD profiler in reconstruction of 3-D electron density distribution (EDD) over Europe Concept: Produce TaD Ne profiles over the Digisonde stations of the DIAS ionosonde network, adjusted by TEC values extracted from the ROB GNSS-TEC maps. For the same mapping area calculate the profile parameters: NmF2, hmF2, H T, h T, and Hp at all grid nodes (1˚x1˚) by using the Polyweight spatial interpolation procedure. Produce TaD profiles at grid nodes. Develop a procedure calculating electron density at any point of the 3-D space by interpolating between the proper profile values at grid nodes.

DIAS ionosonde network European DIAS (Digital Upper Atmosphere Server) network consists of 8 Digisonde stations. They provide foF2, hmF2, and bottomside Ne profile every 15 min. ( Mapping area is confined to (-10˚,25˚)E and (35˚,60˚)N to comply with the GNSS-TEC maps provided by Royal Observatory of Belgium (ROB)

Maps of TaD profile parameters Maps are produced by Polyweight interpolation procedure, after the TaD profiles were calculated and adjusted with GNSS-TEC values at each grid node (1˚x1˚) geographic coordinates.

Electron density maps at fixed altitudes Ne distribution at fixed heights is produced by using TaD profiles at the grid nodes. Ne profiles below hmF2 are provided by Digisonde software. Level ranges are different for the different heights.

Vertical slices from the 3-D EDD

Vertical Ne profiles at -10˚E, 35˚N

Vertical Ne profiles at 25˚E, 60˚N

Ne profile along the raypath (-10˚,35˚) and (25˚,60˚)

Ne profile along the raypath (25˚,35˚) and (-10˚,60˚)

Conclusion On the basis of TaD profiling technique, a new method is developed for reconstruction of the 3-D electron density distribution (EDD) over Europe in real time. Respective software allows obtaining the EDD along arbitrary raypaths within the mapping area. The software is planned to be implemented in DIAS system and consequently to be used to upgrade the products streaming from DIAS to the ESA Space Situational Awareness Space Weather Services.

Thank you