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A NON-RAINING 1DVAR RETRIEVAL FOR GMI DAVID DUNCAN JCSDA COLLOQUIUM 7/30/15.

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Presentation on theme: "A NON-RAINING 1DVAR RETRIEVAL FOR GMI DAVID DUNCAN JCSDA COLLOQUIUM 7/30/15."— Presentation transcript:

1 A NON-RAINING 1DVAR RETRIEVAL FOR GMI DAVID DUNCAN JCSDA COLLOQUIUM 7/30/15

2  The GPM satellite is in a non- sun-synchronous LEO at 65° inclination  Together, GMI and the Dual- frequency Precipitation Radar provide an active-passive combination designed for measuring light to heavy precipitation, rain and snow  GMI is nearly identical to TMI (17 functional years—don’t change it!) but with additional high frequency channels  GMI is the calibration standard for the GPM constellation GPM MICROWAVE IMAGER (GMI)

3 NON-RAINING PARAMETERS AND GMI  Why develop a non-raining retrieval for GMI? Isn’t GPM tailor-made to sense rain and snow?  Other imager algorithms are sensitive to assumption of water vapor distribution—so I try to solve for it  Using GMI as an ‘ideal’ sensor to develop code and methods that can be applied to other sensors (AMSR2, SSMIS, etc.)  GMI is one of the best absolute-calibrated sensors in orbit (according to X-Cal), thus a good test bed for a new approach  ‘Non-raining parameters’ means total precipitable water (TPW), wind speed, and cloud liquid water path (LWP) over ocean—also called ‘Ocean Suite’

4 From Imaoka et al. (2010) Wind effect on Tb (RSS emissivity model) NON-RAINING PARAMETERS AND GMI

5 OPTIMAL ESTIMATION / 1DVAR  Through iteration, the cost function is minimized to find an optimal solution to the inversion, given the measurement vector (Tbs) and a priori knowledge of the environment and the measurement: Φ = (x-x a ) T S a -1 (x-x a ) + [y-f(x,b)] T S y -1 [y-f(x,b)].  Iterate to find state vector that minimizes the difference between observed Tbs and simulated Tbs  One huge advantage to 1DVAR is output error diagnostics (posteriori errors) that come out of the formalism: S x = (K T S y -1 K + S a -1 ) -1

6 To execute a 1DVAR retrieval, you need: 1.Prior knowledge of the environment 2.A good forward model—a method of modeling the atmosphere and surface to simulate what the satellite sees  Radiative transfer model  Surface emissivity model  Assumptions about the atmospheric profiles of water vapor, cloud water, etc. 3.Knowledge of channel errors and their covariances

7 1. PRIOR KNOWLEDGE OF THE ENVIRONMENT From analysis of ECMWF Interim Reanalysis 6-hourly data, LUTs consist of means/variances/covariances of  10m winds  EOFs of water vapor, broken up by SST. Mean 10m Wind Std Dev Wind

8 2. FORWARD MODEL  NOAA’s Community Radiative Transfer Model (CRTM v2.1.3)  Emission/absorption only—not a bad assumption in microwave unless rain or lots of ice present  User has option of FASTEM5 (or FASTEM4) or RSS ocean emissivity model  16 vertical layers defined by pressure  Liquid water cloud set at 850-750mb  Ice cloud may be added as well, and scattering turned on, but no skill in retrieving IWP currently  Reynolds OI SST used as base temperature, though retrieval shows some skill at retrieving SST if it’s allowed to vary  SST used as index for climatological mean water vapor profile from ERA-Int  10m wind, CLWP, SST and 3 EOFs of water vapor are retrieved parameters

9 3. CHANNEL ERRORS  Determining forward model error is an omnipresent issue for satellite retrievals  Most retrievals make up numbers, or at best assume a diagonal S y matrix in which there are no channel error covariances  S a determination is easier, since that can be taken from a model  S y is necessarily different for every sensor, every forward model used!  How to get a ‘real’ S y matrix? The approach: Run both the simplified forward model of the retrieval AND the fullest forward model possible, then analyze the difference: (Tb S, Simplified – Tb O ) - (Tb S, Full – Tb O ) = Tb S, Full – Tb S, Simplified

10 3. CHANNEL ERRORS Full Simplified

11 3. CHANNEL ERRORS  A good retrieval needs a good Jacobian (δT b /δx), which stems from S y  The approach takes into account all simplifying assumptions: no scattering, no ice, fewer levels, etc.  Attempted to screen out rain, sea ice, RFI-contaminated pixels  Even EC Full has trouble, especially at middle frequencies, though other channels in this analysis largely matched Xcal results  What about channel biases?  Success of retrieval depends heavily upon how S y is formed!

12 RESULTS GLOBAL IMAGES—NON-RAINING PARAMETERS LWP [mm] TPW [mm]Wind [m/s]


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