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Space Weather Effects on GPS Thomas J. Bogdan, Director Space Weather Prediction Center NCEP/NWS/NOAA 325 Broadway, DSRC Room 2C109 Boulder, CO 80305,

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Presentation on theme: "Space Weather Effects on GPS Thomas J. Bogdan, Director Space Weather Prediction Center NCEP/NWS/NOAA 325 Broadway, DSRC Room 2C109 Boulder, CO 80305,"— Presentation transcript:

1 Space Weather Effects on GPS Thomas J. Bogdan, Director Space Weather Prediction Center NCEP/NWS/NOAA 325 Broadway, DSRC Room 2C109 Boulder, CO 80305, USA

2 For Official Use Only 2 How GPS works Triangulation from known satellite positions Distance calculated based on radio signal travel time Must correct for delays due to propagation through the atmosphere

3 For Official Use Only 3 GPS Error Sources Typical Error in Meters Standard GPSDifferential GPS (per satellites) Satellite Clocks1.5 0 Orbit Errors2.5 0 Ionosphere5.0 0.4 Troposphere0.5 0.2 Receiver Noise0.3 0.3 Multipath0.6 0.6 The ionosphere is the largest source of error for Standard GPS and second largest for Differential GPS http://www.trimble.com/gps/howgps-error2.shtml#3

4 For Official Use Only 4 Ionosphere Effects on GPS The ionosphere is defined as the region of the upper atmosphere where radio signal propagation is affected by charged particles.

5 For Official Use Only 5 Scintillation Effects SATCOM MESSAGE ERRORS -12 -9 -7 -3 0 3 6 9 12 15 00:21:0000:22:0000:23:00 Universal Time (hh:mm:ss) Relative Signal Strength (dB) Ascension Island 6 April 1997 Average Signal Level Receiver Fade Margin 064. THE QUICK BROWN FOX JUMPS OVER THE LAZY DOGS BACK 01234567<9"TI ?65.( VHE UUicK vROWN$GOX JUMPS OVER†THE!McZY(f~d¸z.9g?_f_}_ j›sSL 33 s %E QUICK$BROWN(FOX JUM‘S OVER THE0L—ZY ?OGS ‚—CK 0123456789 TIÌU¤M ?67. (THE QUKcK BROWN GOY"JUMPS _V˜Z ™‰.O ÁOx'??.9 :c™l???0SsQJ.ª:.$~ $ U ¶S?IcK0 SˆN …? MUM“Û!_VGS* THE LAZY DOGS BACK 01=3456789 TIMES 069. THE QUICK BROWN FOX JUMPS OVER THE LAZY DOGS BACK 0123456789 TIM SATCOM Message S. Basu, private communication

6 For Official Use Only 6 October 29 th, 2003 “walls” of TEC challenge provision of integrity with differential GPS TEC “walls”: 130 TEC units over 50 km 20 m of GPS delay; walls move 100 to 500 m/s SED? “wall” Courtesy: Tom Dehel, FAA Ionosphere Challenges

7 For Official Use Only 7 Mannucci et al., 2005 Anomaly crests 1 TECU = 10 16 electrons m -2

8 For Official Use Only 8 Space Weather Effects on WAAS July 1, 2003 – March 1, 2005 % CONUS at 95% Availability Magnetic Storm Index (Nov 8, 2004) 15 hour loss on 10/29; 11.3 hour loss on 10/30, shorter losses on 11/20/2003

9 For Official Use Only 9 Ionosphere Corrections Need to model the ionosphere to compute corrections Empirical climatological models: Klobuchar Coefficients Physics based numerical models: CTIPe, TIE-GCM Data assimilation schemes: WAAS, US-TEC, GAIM Models can provide specification and forecast The ionosphere is highly variable in space and time

10 For Official Use Only 10 US-TEC Product Current NOAA capability for characterizing the total number of free electrons (TEC) in the ionosphere, with parallel input data streams for reliability Since 2004, a product characterizing the ionospheric TEC over the continental US (CONUS) has been running in real-time at NOAA’s Space Environment Center (SEC) The ionospheric data assimilation model uses a Kalman filter and ingests ground-based GPS data to produce 2-D maps of total electron content over the CONUS Product evolved from a collaboration between SEC and NOAA’s National Geodetic Survey (NGS), National Geophysical Data Center (NGDC), and Forecast Systems Laboratory (FSL) Primary Product: Real-time ionospheric maps of total electron content every 15 minutes. Currently uses about 100 real-time GPS stations from the CORS network http://www.sec.noaa.gov/ustec

11 For Official Use Only 11 Applications: Ionospheric correction for single frequency GPS; NDGPS positioning; dual-frequency integer ambiguity resolution for rapid centimeter accuracy positioning (OPUS). (OPUS)OPUS) Sat. 1 Sat. 5 Sat. 14 Sat. 29 …. etc A A A AB B B B C C C C Slant-Path TEC Maps

12 For Official Use Only 12 US-TEC Validation Summary Differential TEC: Slant = 2.4 TEC units Vertical = 1.7 TEC units “Absolute” FORTE ray tracing: Slant = 2.7 TEC units Vertical = 1.9 TEC units Estimated US-TEC slant path total electron content uncertainty < 3 TEC units (equivalent to about 45 cm of signal delay at L1 frequencies) Estimate US-TEC vertical total electron content uncertainty < 2 TEC units (equivalent to about 30 cm of signal delay at L1 frequencies)

13 For Official Use Only 13 SWPC Ionosphere Goals Produce global real-time specification and forecast Web display of GAIM output from AFWA Assimilation schemes using numerical models: CTIPe, IDEA Improve US-TEC CONUS: Specification with 10 minute latency US-TEC slant path total electron content uncertainty < 2 TECU US-TEC vertical electron content uncertainty < 1 TECU CONUS: Provide Forecast 1 hour forecast as good as specification 3 hour forecast: uncertainty < 3 TEC units 6-12 hour forecasts

14 For Official Use Only 14 Conclusions Solar Maximum is on the way (2012?) Ionosphere Services is a fast growing area in Space Weather SWPC is committed to offer improved products and tools SWPC is ready to collaborate on: Data Models and model results Research Services


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