html5-img
1 / 31

Global Precipitation Measurement Mission An International Partnership &

GPM. Global Precipitation Measurement Mission An International Partnership & Precipitation Satellite Constellation for Research on Global Water & Energy Cycle. Scientific Agenda for GPM Mission’s Ground Validation Research Program. GPM L2 Ground Validation Preliminary Requirements Review

Download Presentation

Global Precipitation Measurement Mission An International Partnership &

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. GPM Global Precipitation Measurement Mission An International Partnership & Precipitation Satellite Constellation for Research on Global Water & Energy Cycle Scientific Agenda for GPM Mission’s Ground Validation Research Program • GPM L2 Ground Validation Preliminary Requirements Review • Eric A. Smith; NASA/Goddard Space Flight Center, Greenbelt, MD 20771 [tel: 301-286-5770;eric.a.smith@nasa.gov; fax: 301-286-1626;http://gpmscience.gsfc.nasa.gov] • 11 March 2004; NASA/Goddard Space Flight Center, Greenbelt, MD

  2. Why does GPM Mission need Ground Validation Research Program? • To scientifically verify credibility of satellite retrievals. • To establish uncertainties of retrievals. - - - - - - - - - - - - - - - - - - - - - - • To serve scientific clients who depend upon GV information in their research and applications.

  3. Who does GPM Mission’s GV Research Program Serve? • PMM Science Team members -- and scientists at large -- who are concerned with accuracy and precision of GPM precipitation retrievals, as well as other kinds of satellite-retrieved precipitation measurements -- in their research and applications programs and projects. Examples include: water cycle & climate diagnosticians, (2) weather climate & forecast modelers, (3) climatologists, (3) hydrometeorologists and hydrometeorological forecasters, and (4) air sea interaction specialists involved with fresh water flux problems. • GV scientists (both PMM and at large) who are involved with assessing and improving GV methodologies and measuring technologies. - - - - - - - - - - - - - - - - - - - - - - • Data assimilation specialists at experimental and operational forecast centers needing near-realtime error characterization of retrieved precipitation products as part of their forecast procedures. • Algorithm creators needing ongoing information concerning their algorithm’s performance (some 3-5 groups) to enable continued algorithm improvement.

  4. How do we plan to establish and accomplish effective GV Research Program? • Galvanize scientific working group within PMM Science Team and other similar international science teams to work cooperatively and under formal partnership arrangements using mission supported Measurement Infrastructure and Technical Support Groups. • Conduct GV operations at international network of GV Supersites (some 5-10) whose main responsibilities will be to provide: • routine and specialized GV data acquisition from suite of high quality measuring systems • computation, archive, and dissemination of standard and specialized GV products for GV research and applications ----------------------------------------------------------------------------------------------------------------------------------- • generation and dissemination of near-realtime, low bandwidth “error characterization” factors, consisting of: (1) bias, (2) bias uncertainty, and (3) error covariance matrices • detect and report to standard algorithm support groups, “instantaneous” and “significant” retrieval errors • Carry out effort within international framework -- much of this organization structure has been defined in preliminary fashion, but awaits final documents and signatures.

  5. GPM’s GV Strategy Requires SamplingSelection of Global Rainfall Regimes Tropical Oceanic Tropical Continental Extratropical Baroclinic & High Latitude Snow Regime Semi-arid Mediterranean Mid-latitude Continental & Mountain

  6. Actual and Potential GPM Ground Validation Sites Finland U.K. Germany Japan -- CRL-Northern Wakkanai Canada Austria Netherlands Switzerland South Korea U.S. -- NASA-Land DOE/ARM-SGP France China Italy Greece C Japan -- CRL-Southern Okinawa Spain Israel U.S. -- NASA-Gauge KSC Taiwan West Africa (AMMA) India U.S. -- NASA-Ocean Kawajalein/RMI Brazil South Africa Australia Regional Raingage Site Radar GV Site or GV Supersite Both

  7. Current Status of GPM Ground Validation Site Network Finland Germany U.K. Japan -- CRL-North Wakkanai Canada Austria Netherlands Switzerland South Korea U.S. -- NASA-Land DOE/ARM-SGP France Italy Greece China C Japan -- CRL-South Okinawa Spain-Catalunya Israel U.S. -- NASA-KSC Taiwan West Africa (AMMA) India U.S. -- NASA-Ocean Kawajalein/RMI Brazil South Africa Australia Existing or Potential Standard GV Site Existing or Potential GV Supersite

  8. What does GPM GV Supersite look like and what are error characteristics?

  9. Mid-Lat Continental Tropical Continental Tropical Oceanic Extratropical Baroclinic GPM Validation Strategy I. Basic Rainfall Validation  Raingauges/Radars new/existing gauge networks new/existing radar networks Research Quality Data Confidence sanity checks II. GPM Supersites  Basic Rainfall Validation hi-lo res gauge/disdrometer networks polarametric Radar system  Accurate Physical Validation scientists & technicians staff data acquisition & computer facility meteorological sensor system upfacing multifreq radiometer system Do/DSD variability/vertical structure convective/stratiform partitioning GPM Satellite Data Streams Continuous Synthesis  error variances  precip trends Calibration Algorithm Improvements Supersite Products III. GPM Field Campaigns  GPM Supersites cloud/ precip/radiation/dynamics processes  GPM Alg Problem/Bias Regions targeted to specific problems FC Data Research  cloud macrophysics  cloud microphysics  cloud-radiation modeling High Latitude Snow

  10. Supersite Template Legend Data Acquisition & Analysis Facility (SSC) Focused Field Campaigns S/X-band Multiparameter Radars GPM Core Satellite Radar/Radiometer Prototype Instruments • Uplk Mtchd Radiom/Radar & • Dual-Frequency Doppler Profiler • Meteorological Tower & • Atmospheric Sounding System Piloted Site Scientists Engineers & Technicians UAVs Retrieval Error Detection DELIVERY Meteorology-Microphysics Aircraft Algorithm Improvement Guidance Error Characterization 150 km  Multi-Gage Hi-Res Domain Site center-displaced with  Uplooking Matched Radiom/Radar [10.7,19,22,37 GHz/14,35 GHz] Upwarddual-freqDoppler Radar Profilers 150 km 5 km Triple Gage Site Multiple-Gage Lo-Res Domain Site centered on main Multiparmeter Radar Single Disdrometer/Triple Gage Site

  11. Error Characterization (Accuracy) Bias (B) & Bias Uncertainty (DB) At Supersite B(RRi)tk = ∑ j = -NT/2,+NT/2 [1/(NT+1)] [ RRiSR(tj,RRi)RRiPEM(tj,RRi] B(RRi)tk end-to-end uncertainties in PEM {for i = 1 , L rainrate intervals (~5) and time period tk} Based on Physical Error Model based on:  physical error model ( passive-active RTE model )  matched satellite radiometer/radar instrument on ground with continuous calibration (eyeball) independent measurements of observational inputs needed for error model (DSD profile, T-q profile, surface R) All retrievals from constellation radiometers & other satellite instruments are bias- adjusted according to bias estimate from reference algorithm for core satellite.

  12. Error Characterization (Precision) J(x) = (xb – x)TF-1 (xb – x) + ( yo – H(x))T ( O + P )-1 ( yo – H(x)) F, O, & P are error covariance matrices associated with forecast model, observations, & forward model (precip parameterization), where yo , H, & x are observation, forward model, & control variable. Space-Time Observational Error Covariance (O) At Supersite (regional expansion rule based on DPR) O(rrj,j,tj)tk = ∑ rj = 0,100 ∑ ri = 0,100.∑ j = 0,360 ∑ i = 0,360 ∑ j = -NT/2,+NT/2 ∑ i = -NT/2,+NT/2 [1/NT]  [ SR(rrj,j,tj)  GV(rMOD(ri+rj,100),MOD(i+j,360),ti+j) ]2 {given polar coordinates (r,) for r out to 100 km and time period tk} Space-Time Autocorrelation Structure Given By  volume scanning ground radars ( dual-polarization enables DPR calibration cross-checks )  research-quality, uniformly distributed, dense, & hi-frequency sampled raingage networks

  13. Where are NASA’s Supersites going to be located? Oceanic: Kwajalein Atoll, RMI Continental: DOE ARM-CART Site, Lamont, OK

  14. Have we quantified our scientific goals vis-à-vis GV measurements themselves? YES -- through Level 2 GV Requirements Document

  15. Do we have evidence that our requirements are rationale and achievable? YES -- through current and ongoing analysis of TRMM and other GV analyses

  16. Kwajalein Monthly Mean Rain Rates

  17. Kwajalein Total Rain Rate PDFs and CDFs

  18. Kwajalein Summary Statistics

  19. Melbourne Monthly Mean Rain Rates Melbourne Total PDFs & CDFs

  20. Melbourne Bias & Precision Summaries by Month OCN LND

  21. Comparison between GSFC & U-WASH GV Retrievals at Kwajalein

  22. Comparison between GSFC & U-WASH GV Retrievals at Kwajalein

  23. Comparison between GSFC & UWASH GV Retrievals at Kwajalein[Jul-Dec 1999 period (6 mo): 103,927 monthly accumulations for 2 x 2 km grids] Statistic GSFC UWASH mean 211 198 stn-dev 101 87 median 198 186 min 10 10.5 max 667 601

  24. What are our problems, what are we missing -- and what are we doing about it? • Some Degree of Institutional and Science Team Resistance to Paradigm Shift • Lack of Physical Error Model

  25. Proposed Physical Error Model (PEM) (E.A. Smith & K-S. Kuo, 2003) • Use Ground Eyeball Radar-Radiometer Z-TB measurements in conjunction with matched Core Satellite DPR-GMI measurements to observe both ends of reflectance-radiance tube between satellite and eyeball instruments. • Use dual-frequency ground Doppler Radar Profiler measurements (either VHF-UHF or UHF-SBand) to provide initial guess DSD profile to Radiative Transfer Model (RTE model), variationally adjusting DSD profile to within standard error of estimates to optimally match observed Z-TB observations, in which residual mismatch objectively defines bias uncertainty. • Take time-average of realization differences vis-à-vis satellite rainrate algorithm estimates with modeled estimates (diagnosed from resultant model-adjusted DSD profiles) to define conditional bias errors. Based on TRMM analyses, monthly zonally-averaged accuracies are expected to be approximately 5%.

  26. Application to GV Error Characterization Matching two-point measurements with radiative transfer simulation by perturbing hydrometeor profile and physical parameters in RTE model. • Use hydrometeor profile retrieved from 2-frequency ground-based Doppler profiler (radar) as starting input to RTE model. • Perturb model hydrometeor input, to within standard error of measurement, until there is optimal match between simulated reflectances-radiances and those from spaceborne and ground radar-radiometer measurements. • Hydrometeor profile determined from best agreement between observed and simulated reflectances-radiances -- result taken as truth for purpose of accuracy assessment of spacecraft retrievals. Note: Effects of small perturbations can be efficiently calculated without running time-consuming model again by first solving adjoint form of RTE (Box et al., 1988, 1989; Polonski and Box, 2002).

  27. Formulation for Single Scattering Properties • Graupel and aggregate hydrometeors are assumed to be clusters of multi-layered spherical particles. • Single-scattering properties of multi-layered sphere is obtained using multi-layered Mie solution (Johnson, 1996) capable of ~7000 layers. One of six canonical configurations is assumed for each hydrometeor, whose single-scattering properties are calculated using consummate solution (interacting dipoles) for ensemble of spheres (Fuller and Kattawar, 1988a-b). Population of hydrometeors is assumed to be composed of such particles with various sizes in specified orientations (e.g., random or oriented). Bulk scattering properties of population are then derived accordingly.

  28. 3-DDeterministic Reverse MonteCarlo Plane-Parallel 3-Dimensional, Time-Dependent, Deterministic Radiative Transfer Model used to simulate multiple scattering within absorbing gaseous medium containing 3-dimensional heterogeneous mix of hydrometeors • Model Description: • 3-dimensional geometry with heterogeneous composition. • Deterministic solution, as opposed to reverse Monte Carlo solution. • Picard iterative solution, akin to successive-order-of-scattering solution. • Capable of simulating responses to time-dependent sources such as radar pulses. • Additional Notes: • Picard iteration is arguably most efficient 3-D deterministic RTE solution. • Time-dependent solution is obtained by succession of steady-state simulations under momentarily constant medium conditions.

More Related