4.2 Assimilation of surface sensitive infrared channels over

Assimilation of surface sensitive infrared
channels over land at Environment Canada
L. Garand, S.K. Dutta, and S. Heilliette
DAOS Meeting
Montreal, Qc
August 15-16, 2014
Outline
• Context & motivation
• Approach
• Assimilation results
________________________
• Also: Update on PCW mission
DRAFT – Page 2 – July 31, 2017
Context & motivation
Env. Can. moving to ensemble-variational system with:
•Flow-dependent background errors including surface skin
temperature correlations with other variables
•Analysis grid at 50 km, increments interpolated to model
25 km grid (15 km in 2015)
•~140 AIRS and IASI channels assimilated: many sensitive
to low level T, q, and Ts. RTM is RTTOV-10.
Favorable context to attempt assimilating surface-sensitive IR
channels over land and sea-ice vs earlier work with GOES (Garand et
al. JAM, 2004) with analysis grid at 150 km and no hyperspectral IR.
DRAFT – Page 3 – July 31, 2017
Ensemble spread of Ts (Feb-Mar 2011)
00 UTC
06 UTC
Maximum ~15h local
In SH (summer)
Maximum at night
Tibetan area (winter)
12 UTC
18 UTC
Ts background error
over land in 4Dvar is
Constant: 3 K.
In EnVar, B is
0.5(BENKF+ BNMC)
DRAFT – Page 4 – July 31, 2017
Ensemble T(~964 hpa) spread
(Jan-Feb 2011)
00 UTC
06 UTC
Only minor
variations with
local time
Values < 0.5 K in SH
seem underestimated
12 UTC
18 UTC
DRAFT – Page 5 – July 31, 2017
Key factors to consider
•
•
•
•
•
Reliable cloud mask
Spectral emissivity definition (CERES, U-Wisconsin)
Highly variable topography
Radiance bias correction
Background and observation error definition
DRAFT – Page 6 – July 31, 2017
Approach guided by prudence
Assimilate under these restrictive conditions over land and sea ice:
•Estimate of cloud fraction < 0.01
•High surface emissivity (> 0.97)
•Relatively flat terrain (local height STD < 100 m)
•Diff between background Ts and retrieval
based on inverting RTE limited to 4K
Radiance bias correction approach:
•For channels flagged as being surface sensitive, use only ocean
data to update bias coefficients
DRAFT – Page 7 – July 31, 2017
Assigned observation error to radiances
Assigned = f std(O-P)
15.0mm
f typically in range 1.6-2.0
Desroziers = <(O-P)(O-A)>
4.13mm
15.3mm
DRAFT – Page 8 – July 31, 2017
4.50mm
Limitation linked to topography
Criterion used: local STD of topography < 50 m (on 3X3 ~50 km areas)
RED: accepted, white std > 100 m, blue 100>std>50 m
DRAFT – Page 9 – July 31, 2017
Limitation linked to surface emissivity
Surface emissivity
AIRS ch 787
Emissivity based on
CERES land types
(~15 km)
+ weighted average
for water/ice/snow
fraction.
Accept only emissivity > 0.97 ; Bare soil, open shrub regions excluded.
DRAFT – Page 10 – July 31, 2017
Examples of emissivity from CERES
10.7 micron
3.9 micron
water: 0.990
water: 0.977
A large portion of land masses have surface emissivity > 0.97
DRAFT – Page 11 – July 31, 2017
First attempt: negative impact in
region 60-90 N/S
00 hr
72hr
Possible cause: cloud contamination ?
DRAFT – Page 12 – July 31, 2017
Second attempt: added constraints
• Cut latitudes > 60 deg
• Local gradient of topography < 50 m (was 100 m)
Strong impact on (O-B) stats for surface channels
DRAFT – Page 13 – July 31, 2017
T std error diff. (CNTL-EXP)
NH-Extratropics 6 Feb to 31March 2011
vs ERA Interim
vs own analysis
Consistent positive impact vs ERA Interim and own
DRAFT – Page 14 – July 31, 2017
T std diff (CNTL-EXP) vs ERA-Interim
Tropics
SH Extratropics
DRAFT – Page 15 – July 31, 2017
Zonal T STD difference (CNTL-EXP)
vs ERA-Interim
72-h
120-h
DRAFT – Page 16 – July 31, 2017
Time series of T std diff at 850 hPa
(a)
NH extratropics
(b)
Tropics
EXP superior to CNTL 54-66 % of cases at days 3-5
DRAFT – Page 17 – July 31, 2017
CNTL
EXP
850 hPa TT anomaly cor.
NH extratropics
Tropics
DRAFT – Page 18 – July 31, 2017
CNTL
EXP
120-h N-Extr vs ERA-Interim
CNTL
EXP
U
HR
GZ
DRAFT – Page 19 – July 31, 2017
T
Validation vs raobs 120-h
Feb-Mar 2011 (59 days)
SH-extratropics
CNTL
EXP
NH-extratropics
U
V
U
GZ
T
GZ
DRAFT – Page 20 – July 31, 2017
V
T
Validation vs raobs 120-h
FEB-Mar 2011 (59 days)
North America
Europe
CNTL
EXP
U
V
U
V
GZ
T
GZ
T
DRAFT – Page 21 – July 31, 2017
Added yield: about 15%
(for surface sensitive channels)
CNTL
EXP
Number of radiances assimilated for surface channel AIRS 787
CNTL: ~1400/6h EXP: ~1600/6h
Region: world, EXP excludes surface-sensitive channels at latitudes > 60
Radiance thinning is at 150 km
DRAFT – Page 22 – July 31, 2017
Std/bias of (O-P) and (O-A), AIRS 787
CNTL EXP
O-P
O-A
No major impact on bias. Strong assimilation over land,
with std (O-P) DRAFT
of ~1.7
(O-A)
– PageK,
23 –std
July 31,
2017 of 0.40 K (not shown)
Conclusion
• Very encouraging results, especially in NH where most
of new data are assimilated
Next steps:
• Relax limitations on emissivity, use MODIS-derived atlas
• Run a summer cycle
• Seek operational implementation
Longer term
• Evaluate problems specific to high latitudes
DRAFT – Page 24 – July 31, 2017
Update on Polar Communications
and Weather (PCW) mission
Goal:
Fill communication and meteorological
observation gaps in the Arctic
Most likely configuration:
2 satellites in highly elliptical orbits
Status:
Seeking approval from Government
in early 2015. Could start
operating in 2021.
Meteorological instrument:
Similar to ABI or FCI
A possible 2-sat HEO system
DRAFT – Page 25 – July 31, 2017
Weather:
High-Level Requirements
Capabilities
• ‘GEO-like’ continuous imaging of Arctic circumpolar region
• ‘GEO-like’ spatial (1-3 km) and temporal (15 min) resolution
• ‘Next-generation’ meteorological imager (ABI, FCI, 16+
channels)
• Near-real time processing to L1c for delivery to Environment
Canada
• Compatibility with GEO imagers as part of WMO Global
Observing System.
DRAFT – Page 26 – July 31, 2017
Orbit Comparison
(2-sat Constellation)
Molniya (12-h)
Apogee: 39,800 km
TAP (16-h)
Apogee: 43,500 km
Tundra (24-h)
Apogee: 48,300 km
DRAFT – Page 27 – July 31, 2017
Science Studies: Uniqueness of HEO
System vs LEO
23 LEO satellites needed to get 15 min
Imagery at 60 N, versus 2 HEO
Trichchenko and Garand,
Can. J. Remote Sensing, 2012
Also, capability to get image triplets for AMV vastly superior to LEO
DRAFT – Page 28 – July 31, 2017
Science Studies:
Impact on NWP
OSSE showing significant impact of PCW
AMVs filling gap in polar areas
Garand et al., JAMC, 2013
Positive impact (blue) at 120-h
In both polar regions from 4 satellites
DRAFT – Page 29 – July 31, 2017
Example of PCW Geometry Matching
[16-hr TAP Orbit] for intercalibration
VIIRS/SNPP
GEO
DRAFT – Page 30 – July 31, 2017
Trishchenko and Garand, GSICS Newsletter, 2012