Apr 27-30, 2010Boulder, CO2010 Space Weather Workshop Follow-On Radio Occultation Constellations for Meteorology, Ionosphere and Climate: Overview of Currently.

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Presentation transcript:

Apr 27-30, 2010Boulder, CO2010 Space Weather Workshop Follow-On Radio Occultation Constellations for Meteorology, Ionosphere and Climate: Overview of Currently Planned Missions, Data Quality and Coverage, and Potential Science Applications Bill Schreiner, C. Rocken, X. Yue, B. Kuo COSMIC Program Office, UCAR, Boulder CO P. Wilczynski, D. Ector, R. Fulton NOAA/NESDIS Office of Systems Development, Silver Springs, MD

Apr 27-30, 2010Boulder, CO2010 Space Weather Workshop Outline COSMIC and RO Overview Future RO Missions Summary

Apr 27-30, 2010Boulder, CO2010 Space Weather Workshop COSMIC (Constellation Observing System for Meteorology, Ionosphere and Climate) Joint Taiwan and US project NSF is U.S. lead agency –NOAA, NASA, Air Force, Navy 6 Satellites launched April 14, 2006 GPS Radio Occultation Receiver -Refractivity -Pressure, Temperature, Humidity -Absolute Total Electron Content (TEC) -Electron Density Profiles (EDP) -Ionospheric Scintillation (S4 amplitude) Tiny Ionospheric Photometer (TIP) – UV Radiances CERTO Tri-Band Beacon Transmitter Complete global and diurnal sampling Demonstrated forecast value of GPS radio occultation soundings in near-real time Total cost ~$100M; Taiwan paid for 80% of costs Mission on time, within budget, and exceeding expectations

Apr 27-30, 2010Boulder, CO2010 Space Weather Workshop CDAAC CDAAC NESDISNESDIS GTS NCEP ECMWF CWB UKMO Canada Met. JMA WMO BUFR Files per day with Latency ~ 75-90min Getting COSMIC Results to Weather Centers JCSDA Meteo France COSMIC Operational Processing Science & Archive TACC AFWA Input Data - COSMIC data - GPS ground data - GPS NDM Bits - GFS Forecast - IGS/IGU ORB/CLK - Bernese Config files Research Community SFTP UCAR/Unidata’s LDM WGET RTSs: Alaska Norway Antarctica/McMurdo Providing data to > 1,250 registered users from 54 countries

Apr 27-30, 2010Boulder, CO2010 Space Weather Workshop GPS Antennas on COSMIC Satellites Nadir 2 POD Antennas - TEC, EDP and S4 (1 Hz) - clock reference data (50 Hz) V LEO COSMIC S/C 2 Occultation Antennas - atmospheric profiling (50 Hz) GPS receiver developed by JPL and built by Broad Reach Eng. Antennas built by Haigh-Farr Upto 9 GPS Upto 4 GPS Future Side-viewing Antennas?

Apr 27-30, 2010Boulder, CO2010 Space Weather Workshop GPS Absolute TEC COSMIC trans- ionospheric radio links for a 100-min period, June 29, 2007 Absolute TEC good to ~ 3 TECU Relative TEC ~ TECU Actual COSMIC reference link data ~ TECU at 1-Hz ( )

Apr 27-30, 2010Boulder, CO2010 Space Weather Workshop COSMIC GPS Radio Occultation GPS SatelliteCOSMIC LEO Satellite  TEC = solid - dashed [Schreiner et al., 1999] Inverted via onion-peeling approach to obtain electron density N(r) Assumption of spherical symmetry

Apr 27-30, 2010Boulder, CO2010 Space Weather Workshop EDP Precision from Collocated Soundings [Schreiner et al., 2007]

Apr 27-30, 2010Boulder, CO2010 Space Weather Workshop 110 km altitude COSMIC EDP Retrieval Errors Unit: 1×10 11 /m 3 COSMIC Observations Abel retrieval Error from Simulation 220 km altitude COSMIC EDP retrieval assumes spherical symmetry (Abel inversion) Simulation Performed by UCAR/COSMIC : -small errors at F-layer and above -Larger errors below F-layer (shown below for real obs and error simulation) EDP Retrieval improvements are under investigation at UCAR [Yue et al., 2010]

Apr 27-30, 2010Boulder, CO2010 Space Weather Workshop GPS L-band Scintillation E layer F layer Where is the source region of the scintillation? Localize irregularities: [see Sokolovskiy et al., 2002]

Apr 27-30, 2010Boulder, CO2010 Space Weather Workshop COSMIC EDPs used for verification of IRI and TIEGCM models (Lei et al., 2007) COSMIC EDPs used to estimate ionosphere High Transition Heights (HTH) and agree well with C/NOFS data (Yue et al., AGU, 2009) COSMIC EDP inversion errors quantified in E and F layers of ionosphere (Yue et al., 2010) COSMIC used to study ionospheric response to Sudden Stratospheric Warming event (Yue et al., 2010) By using COSMIC NmF2 and hmF2, HAO/NCAR reported that the Weddell Sea Anomaly phenomena can be explained by conjugate effects (Burns et al., 2009) Mid-latitude summer nighttime anomaly (MSNA) of the ionosphere observed by COSMIC EDPs (Lin et al., 2009) Plasma depletion bays observed by COSMIC EDPs (Liu et al., 2009) COSMIC S4 Scintillation indices used in validation with C/NOFS data (Strauss, 2009) and to map irregularity regions (Gouthu et al., 2009) Sporadic E layer climatology produced with COSMIC data (Wang, 2009) COSMIC EDPs and TIP data used to study the ionosphere disturbance during 15 Dec 2006 geomagnetic storm and found a long lasting positive storm effect in ionosphere (Pedatella et al., 2009) TIP data used to map the post-sunset equatorial anomaly and F-region depletions (Coker et al., 2009) JPL did many observation system simulation experiments (OSSE) and found that COSMIC 2 can advance the assimilation performance because of much more GPS TEC observations than current COSMIC (Pi et al., 2009) Recent Ionosphere and Space Weather Studies Performed with COSMIC Data

Apr 27-30, 2010Boulder, CO2010 Space Weather Workshop GNSS Radio Occultation Follow-On Plans at NOAA NOAA Operational ROFollow-On mission funded in President’s FY2011 budget. NASA has funded JPL to develop advanced GNSS RO payload. UCAR working with NOAA and Taiwan on the planning of a COSMIC-II Mission. Preliminary design calls for 12 low Earth orbiting satellites, tracking GPS, GALILEO and possibly GLONASS. Will produce more than 8,000 soundings per day. Data Latency being studied Expected launch in NOAA also considering RO Data Purchase

Apr 27-30, 2010Boulder, CO2010 Space Weather Workshop Constellation Requirements Uniform RO global sampling Uniform RO local time sampling Minimize RO data latency Minimize deployment time Maximize GPS tracking data

Apr 27-30, 2010Boulder, CO2010 Space Weather Workshop

Apr 27-30, 2010Boulder, CO2010 Space Weather Workshop EDP Local Time Coverage in 4 hrs MidnightNoon 1 S/C GPS 4 hrs 12 S/C, GPS+Galileo 4 hrs

Apr 27-30, 2010Boulder, CO2010 Space Weather Workshop Occultation Density vs. Constellation Options IIA 8/72 & 4/24 IIB 12/72 IIC 6/72 & 6/24 IID 4/72 & 8/24 12 S/C with GPS+Galileo Add 8 MOOs with GPS (+ Missions of Opportunity)

Apr 27-30, 2010Boulder, CO2010 Space Weather Workshop Average Data Latency with Ground Stations Worst-Case:Current COSMIC 15 deg elevation cutoff Data to CDAAC = LOS + 4 min CDAAC processing time = 7.5 min Best-Case:Realistic COSMIC-II 5 deg elevation cutoff Data to CDAAC = AOS + 3 min CDAAC processing time = 5 min NetworkLEO Inclination (deg) Worst- Case Average Latency (min) Best-Case Average Latency (min) COSMIC (Fairbanks, Tromso) COSMIC+McMu rdo COSMIC+McMu rdo+TrollSat Stations Stations sites: Fairbanks, Tromso, McMurdo, TrollSat, Guam, Hawaii, Vandenberg, Colorado, NewHampshire, DiegoGarcia, England, Thule, Bangalore, Mauritius, Taiwan - Satellite-Satellite Comm (TDRSS, InmarSat) Option being considered: ~5-15 min latency

Apr 27-30, 2010Boulder, CO2010 Space Weather Workshop Summary COSMIC Space Weather Data Products – > 3 Million Absolute TEC data arcs – > 2.3 Million EDPs – Large amount of scintillation data – ~90% available within 3 hrs, ~50% in 1 hr, and ~10% in ½ hr – Positive impact on ionospheric and space weather studies NOAA moving ahead with GNSS RO Follow-On planning NOAA collaboration with Taiwan, 12 satellites launched ~ ~ 8,000 RO’s per day with near uniform geographic and LT sampling Data Latency TBD: Ground Stations (~ 30 min ave) vs Sat-Sat Comm (5-15 min) NOAA considering RO data purchase

Apr 27-30, 2010Boulder, CO2010 Space Weather Workshop Acknowledgments NSF Taiwan’s NSPO NASA/JPL, NOAA, USAF, ONR, NRL Broad Reach Engineering