workshop on hyperspectal meteorological science of uw-muri and beyond 14–15 may 2002, madison,...
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Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
Numerical Weather Prediction Numerical Weather Prediction Modeling for MURI/AtmosphericModeling for MURI/Atmospheric
Parameter RetrievalsParameter RetrievalsJohn R. Mecikalski, Derek J. PosseltJohn R. Mecikalski, Derek J. Posselt
CIMSS Co-InvestigatorsCIMSS Co-Investigators
1. Overview of NWP support2. GIFTS Simulated Data for Algorithm &
Product Development3. Computational Requirements4. Atmospheric Parameter Retrievals
O U T L I N E
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
NWP Infrastructure at CIMSSNWP Infrastructure at CIMSS
• PSU/NCAR MM5
• UW-Nonhydrostatic Modeling System (UW-NMS)
• Weather Research & Forecasting (WRF)
• Rapid Update Cycle-2 (RUC2)
The capabilities of numerically simulating the atmosphere overa wide range of meteorological scales, over large geographicaldomains, and for realtime numerical weather prediction (NWP)are rapidly increasing at CIMSS.
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
NWP support for Ongoing ProjectsNWP support for Ongoing Projects
• Cloud-Radiative modeling for instrument validation, radiance and retrieval algorithm development (MURI PI & Co-I’s)
• Generate “truth” atmosphere for satellite-based estimates of PBL stability, and convective initiation studies (MURI Co-I’s & MURI PM)
• Assessment of turbulence with NAST-I data (MURI PM)
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
The UW-NMS and PSU/NCAR MM5The UW-NMS and PSU/NCAR MM5
• A robust NWP system:– scaleable– explicit physics at 4 km-resolution– explicit microphysics for accurate clouds– variably-stepped topography
• Excellent model for “Cloud-Radiative” experiments: Independent of other NWP systems
• Developed for multi-processor, distributed memory computational environments (Fortran-90 with MPI).
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
NWP for Retrieval & SimulationNWP for Retrieval & Simulation
• NWP can provide atmospheric retrieval algorithms critical “first guess” information.
• NWP for direct GIFTS data and instrument simulation:– A numerically simulated atmosphere is
considered “nature” and is assumed to very accurately represent the true state.
– Requires a sophisticated numerical model and is therefore computationally very expensive(1 Gflops per data “cube”)
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
Improving Retrieval First GuessImproving Retrieval First GuessAERI (red) versus Radiosonde (black)AERI (red) versus Radiosonde (black)
First Guess
Temperature
Dew PointTemperature
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
Alt
itu
de
(k
m)
• April 1998-October 1999,463 AERI+Model/radiosonde profiles
• Differences are less than 1 deg K
• AERI+Model every 10minutes, sondes every3-12 hours
AERI
ETA MODEL
AERI/MODEL - RADIOSONDE (K)
NWP in Atmospheric Retrievals:NWP in Atmospheric Retrievals:AERI+Model/Radiosonde Temperature ComparisonAERI+Model/Radiosonde Temperature Comparison
NWPMODEL
GIFTS
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
Simulating GIFTS DataSimulating GIFTS Data
High-resolution numerical simulations are used to provide the following atmospheric parameters to the GIFTS radiative-transfer model:– Temperature– Water vapor mixing ratio– Mixing ratios and mean particle
diameters of cloud and ice liquid water– Liquid and ice water path– Cloud-top height with respect to both
liquid and ice cloud
Goal: To provide investigators with simulated (interferogram) data that accurately represents what will eventually come from the GIFTS instrument.
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
Numerical Model Output toSimulated Radiances
Simulated GIFTS Data Cube
Simulated GIFTS Brightness Temperatures
NWP Data Cube
Clouds from UW-NMS
ForwardModel:
Dave Tobin
ForwardModel:
Dave Tobin
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
Derived GIFTS DataDerived GIFTS Data
• Vertical Temperature Profiles• 1 sounding per 1 scene pixel • 128 x 128 = 16384 scene pixels• 4 km pixel spatial resolution (nadir)
“Regional Sounding” Product:• 100 vertical layers• Retrieved values/cube = 128x128x100• 1.6 million retrieved values/cube• 10 second dwell time
Longitude (deg)
Lat
itud
e (d
eg)
Tem
pera
ture
(K
)
GIFTS SIMULATED TEMPERATURE DATA CUBE950 MB LAYER TEMPERATURE
GIFTS SIMULATED VERTICAL TEMPERATURE PROFILE
Pre
ssu
re (
mb
)
Air Temperature (K)
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
Modeling Infrastructure for Large ScaleModeling Infrastructure for Large ScaleGIFTS-IOMI data processingGIFTS-IOMI data processing
• Need to simulate GIFTS data at 4 x 4 km resolution over large domain:– Distributed memory, massively parallel computer code
and computer system– Must be accomplished in a timely manner [O(few
days)]– Demands a sophisticated atmospheric model (UW-
NMS)
• Combination of UW-NMS and MM5 allows us to simulate “large” regional domains.
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
• Large-Scale Symmetric Multi-Processor (SMP)– Integrated unit with high-bandwidth backplane– Shared RAM, multiple CPU, single OS kernel– Communication: shared memory & semaphores– Examples: SGI Origin, IBM RS/6000
• Linux Cluster– Network of inexpensive COTS computers– Multiple RAM, multiple CPU, multiple OS kernel– Communication: TCP/IP, sockets & datagrams– Examples: Sandia ‘CPlant’, Forecast Systems Laboratory ‘Jet’
• 64-bit Linux
Necessary Computational Infrastructure Necessary Computational Infrastructure for MURI: for MURI: SMP & Cluster SystemsSMP & Cluster Systems
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
Hardware Diagram: Hardware Diagram: Linux Cluster
Network Switch
UPS
TapeArchive
FileserverComputer
DiskArray
Rack andCPUs
70% of the initial cost30% of the initial cost
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
Current Computational LimitsCurrent Computational Limits
3 x 3 Cube Domain:• 4 km resolution• Number of grid points:
400 x 400 x 40 = 6400000• Approximate memory use:
15-20 Gb of RAM• Total Cluster memory:
24 Gb of RAM
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
Near-Term LimitsNear-Term Limits
5 x 5 Cube Domain:• 4 km resolution• Number of grid points:
640 x 640 x 40 = 16384000• Anticipated memory use:
45-50 Gb of RAM• 16 more processors
(8 more nodes)• 32-bit limit for domain set-up
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
Future NeedsFuture Needs
25 x 25 Cube Domain:• 4 km resolution• Number of grid points:
3200 x 3200 x 40 = 4.1x108
• Approximate memory use:1170 Gb of RAM
• Doable?
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
Minimum Calculation Times forMinimum Calculation Times for3 by 3 Simulation (3 time steps)3 by 3 Simulation (3 time steps)
Processing Steps Time on 16 CPU Cluster
Numerical weather model calculations 10 days
Fast model coefficient generation 18.5 days *
Calculation of TOA radiances 5 days
FTS optics simulation 3 days
Detector array modeling and linear calibration 0.5 days
Total 37 days
* Not parallelized yet
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
Atmospheric Parameter RetrievalsAtmospheric Parameter Retrievals
Progress to Date: June 2002–May 2003• Temperature and Water Vapor
– Jun Li
• First Winds– Chris Velden, Gail Dengel
• Stability Indices– Wayne Feltz, John Mecikalski
• Atmospheric (PBL) Turbulence– John Mecikalski, Ryan Torn, Wayne Feltz
• Visibility: “GVision”– Derek Posselt, Wayne Feltz, John Mecikalski, Tom Rink
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
Atmospheric Temperature, Moisture, OzoneAtmospheric Temperature, Moisture, Ozone
1. The Physical retrieval model has been developed
2. Two fast ways for Jacobian calculation are developed
3. Contrast between surface skin temperature and surface air temperature on boundary layer moisture
4. Simulation studies using cube data from MM5
Clear Sky retrieval of T
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
First WindsFirst Winds
Issues for Winds …
Critical need for LARGE “cube” simulation data sets; without such large domains, useful wind sets from simulated GIFTS data are not possible
– First “GIFTS” winds have been produced.
– Issues of cube numbers when retrieving winds (2x2 or larger)
– Issues of concatenating cubes
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
Stability IndicesStability Indices“Truth” LCL Retrieved LCL
First Retrieval of StabilityExample: Lifted Condensation Level (LCL)LCL may be used as a measure of boundary layer depth, and/or thedepth of the inversion atop the boundary layer (e.g., marine inversion).
HigherStability
LowerStability
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
PBL TurbulencePBL Turbulence
Evaluating Turbulence from Hyperspectral MeasurementsExample: Shear-Driven Instabilities: AERI-derived Boundary
Layer Depths
CBL Waves & Rolls
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
PBL TurbulencePBL Turbulence
June 23, 2001 autocorrelation starting 320 minutes after sunrise
August 8, 2001 e autocorrelation starting 300 minutes after sunrise
Clear Day (no clouds)
Boundary Layer Cumulus
Preliminary Findings: We appear to have identified boundary layer “roll” turbulentfeatures that produce e variations at this AERI site at periodic intervals.Ongoing work will evaluate the horizontal scales of these roll structuresbased on bulk stability parameters (e.g., Ri).
Time Difference (min) Time Difference (min)
Cor
rela
tion
Cor
rela
tion
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
““GVision” –GVision” –A Tool for Coalescing GIFTS-IOMI DataA Tool for Coalescing GIFTS-IOMI Data
Purpose:– Draw together disparate data for viewing atmospheric parameters
– Capitalize on in-house expertise for visualizing GIFTS-IOMI data
– Test and validate all models using within UW-MURI (NWP, RTE, etc.)
– Develop 3rd-order fields (i.e. slantwise visibility)
“VisAD” Capabilities: Java-based application, developed at UW,that is designed for the optimal manipulation and displayof large meteorological data sets.
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
Goal for Indian Ocean METOC ImagerGoal for Indian Ocean METOC Imager
Point Weather Data• Marine Inversion• Aerosol & dust detection• Flight-level & directional
visibility• Flight-level turbulence• SST for engine efficiency• Surface characterization
IOMI-GIFTS 4 km “Cube”
Workshop on Hyperspectal Meteorological Science of UW-MURI and Beyond14–15 May 2002, Madison, Wisconsin
• We need to be thinking “Big”– NWP to support IOMI-GIFTS for large domains– IOMI-GIFTS data flow within an Modeling system
• NWP for next generation IOMI– IOMI-GIFTS validation experiments: NWP support – NWP to develop “turn-key” fleet-ready data system
• First Progress of Atmospheric Parameters– T, q, winds, stability, turbulence & – Continue from here ...
In Conclusion ...In Conclusion ...