Date post: | 04-Jan-2016 |
Category: |
Documents |
Upload: | jada-conner |
View: | 28 times |
Download: | 0 times |
Institute forMathematicsApplied toGeoscience
Geophysical Statistics Project - GSP
Data Assimilation Research Section - DAReS
Turbulence Numerics Team - TNT
Your typical ensemble
Ensemble mean = waste of time
GSP - statistically blending winds
QuikSCATLaunched June 1, 1999
~800 km altitude (~100 min orbit)1800 km-wide swath
about 400,000 measurements/day
graphics by JPL
QuickTime™ and aCinepak decompressor
are needed to see this picture.
GSP - Statistically Blending Winds
6144 ‘observations’ every 6 hours(unrealistically smooth)
~ 40,000 observations every 6 hours(dense, but ‘gappy’)
Resulting wind field with proper energy decay
Gradient (important to ocean circulation)
energy falls off too much
energy falls offperhaps not enough
GSP
The striping indicates the areas sampled by
the scatterometer.
Animation of E-W wind field created by synthesizing gridded winds and scatterometer (satellite) winds.
Technique remains faithful to the data.
Low standard deviation in data-
dense regions.
QuickTime™ and aPNG decompressor
are needed to see this picture.
Data Assimilation Research Section - DAReS
Our computational challenge is to run MANY (~100) instances of the numerical models (CAM, WRF, ...)
simultaneously.
Simply running one numerical weather prediction model has been driving supercomputer research.
Data assimilation exploits the information in observations to ‘steer’ a numerical model.
Put another way, it ‘confronts’ a numerical model with observations.
Our challenge is to run MANY of these.
QuickTime™ and aYUV420 codec decompressor
are needed to see this picture.
Our ‘MACHINE’
Data Assimilation Research Testbed : DART
* Many low-order models: Lorenz 63, L84, L96, etc.
* Global 2-level PE model (from NOAA/CDC)
* NCAR’s CAM 2.0 & 3.0 (global spectral model)
* NCAR’s WRF (regional)
* GFDL FMS B-Grid GCM (global grid point model)
Forward Operators and Datasets
Many linear, non-linear forward operators for low-models
U, V, T, Ps, Q, for realistic models
Radar reflectivity, GPS refractivity for realistic models
Observations from BUFR files (NCEP reanalysis flavor)
Can create synthetic (i.e perfect model) observations for all
Data Assimilation Research Section - DAReS
Turbulence is one of the last unsolved classical physics
problems.GASpAR
Geophysical-Astorphysical spectral element adpative refinement.
GASpAR
Flexible framework for accurate simulation of turbulence
Numerical methods that minimize dissipation.
Objects are structured to facilitate parallel computation.
Dynamic refinement gives a speedup of 5-10X over fixed grids with comparable accuracy.
Objected-oriented h-adapted code for simulating turbulent flows.
Hierarchical.
How does GASpAR do it?
Elements Fields Equation Solvers
Spectral Element Method
operators
GBLASBases
Mortar objects
Adaptive refinement based on error estimates
Mortar Objects
An unambiguous representation of the field at parent/child boundaries based on
interpolation.
Dynamically adaptive geophysicalfluid dynamics simulation
using GASpAR
Simulation of three vortices
Refinement done on a component of
velocity.
QuickTime™ and aH.264 decompressor
are needed to see this picture.