iasi on metop on-ground calibration of the fm2 instrument · itsc-14 – beijing, 25-31may. 2005 d....
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ITSC-14 – Beijing, 25-31May. 2005 1D. Blumstein – CNES DCT/PO/EV
Infrared Atmospheric Sounding Interferometer
IASI on METOPOn-Ground Calibration of the FM2 Instrument
International TOVS Study Conference25-31, May 2005
Beijing China
D. Blumstein1, B.Tournier2, T.Carlier1, T.Maciaszek1, T.Phulpin1, G.Chalon1, P.Astruc3, D.Miras3, D.Siméoni3
(1) Centre National d'Etudes Spatiales (CNES), Toulouse, France(2) NOVELTIS, Toulouse, France(3) ALCATEL SPACE, Cannes, France
ITSC-14 – Beijing, 25-31May. 2005 2D. Blumstein – CNES DCT/PO/EV
Outline
Key Performance specifications
On-ground characterization of IASI FM2First IASI instrument in flight (on METOP 2)
IASI Program Status
ITSC-14 – Beijing, 25-31May. 2005 3D. Blumstein – CNES DCT/PO/EV
Key performances specifications
Radiometric sensitivityApodized and non-apodized spectra
Radiometric accuracyAbsolute accuracyRelative accuracy (at a given time)
Between pixels, channels, viewing direction
Stability
Spectral & geometrySpectral calibrationSpectral response functionPoint Spread Function ( & interband registration)
ITSC-14 – Beijing, 25-31May. 2005 4D. Blumstein – CNES DCT/PO/EV
AVM result — IASI FM2 Noise Spectrum (NedT at 280 K) — Session SM0410060647 — CBS 91.7 K
0,0
0,1
0,2
0,3
0,4
0,5
0,6
0,7
0,8
0,9
1,0
64500 82500 100500 118500 136500 154500 172500 190500 208500 226500
Wavenumber (m^-1)
Ned
T at
280
K (K
)
Noise Spectrum in NedT at 280 K after drift correction - P4 - c10693_avm_SM0410060647Noise Spectrum in NedT at 280 K after drift correction - P1 - c10693_avm_SM0410060647Noise Spectrum in NedT at 280 K after drift correction - P3 - c10693_avm_SM0410060647NedT at 280 KNoise Spectrum in NedT at 280 K after drift correction - P2 - c10693_avm_SM0410060647NedT at 280 K
Measured radiometric sensitivity
IASI FM2 testing in vacuumDetectors temperature 91.7 KMeasured on blackbodyNo evolution of noise (ice cont.)
Loss of transmission : 1.5 % at 850 cm-1 over a period of 6 daysEquivalent to the absorption by a 40 nm thin film of water ice
non apodized (293 K scene)
measurements
B1 B3B2
Measurement SM0410111609 — Pixel 3Effect of scene temperature on B3 noise (scene at 240 & 280 K)
0,0
0,1
0,2
0,3
0,4
0,5
0,6
0,7
0,8
1900 1950 2000 2050 2100 2150 2200 2250 2300 2350 2400Wavenumber (cm-1)
NeD
T at
280
K (K
)
240 K 280 K spec
NeDT in K (at 280 K)
Mission radiometric performance in NeDT — T_CBS=91,7 K — (IASI FM2 OV Test)
0.0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1.0
645 845 1045 1245 1445 1645 1845 2045 2245Wavenumber (cm-1)
NeD
T at
280
K (K
)
Spécification FM2 (Delta-QR)
apodized + pseudo-noise
ITSC-14 – Beijing, 25-31May. 2005 5D. Blumstein – CNES DCT/PO/EV
- 0 .5
- 0 .4
- 0 .3
- 0 .2
- 0 .1
0
0 .1
0 .2
0 .3
0 .4
0 .5
6 4 5 0 0 1 1 4 5 0 0 1 6 4 5 0 0 2 1 4 5 0 0 2 6 4 5 0 0
W a v e N u m b e r ( m ^ - 1 )
Rad
iom
etric
Cal
ibra
tion
Erro
r in
Ned
T at
280
K (K
)
3 0 0 2 9 4 2 8 0 2 6 0 2 4 0
B B C c o a t in g e m is s iv it y lo s sH B B c o a t in g e m is s iv i t y lo s s
Measured radiometric accuracy (1/4)Session SM 06 22h59 — T_HBB about 299 K, no Non-Linearity correction
298,2
298,4
298,6
298,8
299,0
299,2
299,4
299,6
299,8
300,0
300,2
645 845 1045 1245 1445 1645 1845 2045 2245Wave numbers (cm-1)
Brig
thne
ss te
mpe
ratu
re (K
)
Pixel 1 Pixel 2 Pixel 3 Pixel 4
Session SM 06 22h59 — T_HBB around 299 K, Non-Linearity correction applied
298,2
298,4
298,6
298,8
299,0
299,2
299,4
299,6
299,8
300,0
300,2
645 845 1045 1245 1445 1645 1845 2045 2245Wave numbers (cm-1)
Brig
thne
ss te
mpe
ratu
re (K
)
Pixel 1 Pixel 2 Pixel 3 Pixel 4
IASI FM2 testing in vacuumNeed for NL correction in B1 bandDT < 0.25 KTarget in nadir position
Result valid for other incidencesPost-calibration done by Level 1 proc. to achieve "differential" requirements
Between pixels, scan views or channels
B1
NL (B1)corrected
-0 .5
-0 .4
-0 .3
-0 .2
-0 .1
0
0 .1
0 .2
0 .3
0 .4
0 .5
6 4 5 0 0 1 1 4 5 0 0 1 6 4 5 0 0 2 1 4 5 0 0 2 6 4 5 0 0
W a v e N u m b e r (m ^ -1 )
Rad
iom
etric
Cal
ibra
tion
Erro
r in
Ned
T at
280
K (K
)
3 0 0 K2 9 4 K2 8 0 K2 6 0 K
2 4 0 K2 2 0 K
H B B c o a tin g e m is s iv ity lo s s
B B C c o a t in g e m is s iv i ty lo s s
Tscene : 240 – 300 KPixel 1, Redundant Conf., Hot Case
Tscene : 220 – 300 KPixel 1, Nominal Conf., Cold Case
ITSC-14 – Beijing, 25-31May. 2005 6D. Blumstein – CNES DCT/PO/EV
Measured radiometric accuracy (2/4)
Raw measurements versus model comparison Pixel 1Nominal Conf.Cold Case
-0 .5
-0 .4
-0 .3
-0 .2
-0 .1
0
0 .1
0 .2
0 .3
0 .4
0 .5
6 4 5 0 0 1 1 4 5 0 0 1 6 4 5 0 0 2 1 4 5 0 0 2 6 4 5 0 0
W a v e N u m b e r (m ^ -1 )
Rad
iom
etric
Cal
ibra
tion
Erro
r in
Ned
T at
280
K (K
)
3 0 0 K2 9 4 K2 8 0 K2 6 0 K
2 4 0 K2 2 0 K
H B B c o a t in g e m is s iv ity lo s s
B B C c o a t in g e m is s iv ity lo s s
Radiometric Calibration Error Model — Nominal configuration, Cold CaseT_env HBB = 280 K, T_env BBC = 275 K, T_env CBB = 230 K
-0.5
-0.4
-0.3
-0.2
-0.1
0.0
0.1
0.2
0.3
0.4
0.5
645 1145 1645 2145 2645
Wave Number (cm-1)
DT
at 2
80 K
(Kel
vin)
220 K 240 K 260 K 280 K 294 K 300 K
ITSC-14 – Beijing, 25-31May. 2005 7D. Blumstein – CNES DCT/PO/EV
Measured radiometric accuracy (3/4)
- 0 .5
- 0 .4
- 0 .3
- 0 .2
- 0 .1
0
0 .1
0 .2
0 .3
0 .4
0 .5
6 4 5 0 0 1 1 4 5 0 0 1 6 4 5 0 0 2 1 4 5 0 0 2 6 4 5 0 0
W a v e N u m b e r ( m ^ - 1 )
Rad
iom
etric
Cal
ibra
tion
Erro
r in
Ned
T at
280
K (K
)
3 0 0 2 9 4 2 8 0 2 6 0 2 4 0
B B C c o a t in g e m is s iv i t y lo s sH B B c o a t in g e m is s iv i t y lo s s
Raw measurements versus model comparison Pixel 1Redundant ConfHot Case
Radiometric Calibration Error Model — Redundant configuration, Hot CaseT_env HBB = 295 K, T_env BBC = 285 K, T_env CBB = 230 K
-0.5
-0.4
-0.3
-0.2
-0.1
0.0
0.1
0.2
0.3
0.4
0.5
645 1145 1645 2145 2645
Wave Number (cm-1)
DT
at 2
80 K
(Kel
vin)
240 K 260 K 280 K 294 K 300 K
ITSC-14 – Beijing, 25-31May. 2005 8D. Blumstein – CNES DCT/PO/EV
Measured radiometric accuracy (4/4)
More in-depth verifications performed during the testScan angle effect verifiedInterpixel & interscan calibrationSensitivity to thermal drifts
Simulation of Entry/Exit of eclipse
Mission Objectives on radiometric calibration are expected to beachieved in orbit
Absolute Calibration Error : < 0.5 KIntercalibration error at a given time : < 0.2 K
All geophysical conditions4 pixels, all viewing directions, all channels
Intercalibration error over time : < 0.3 KShort term (orbital period)Long term
ITSC-14 – Beijing, 25-31May. 2005 9D. Blumstein – CNES DCT/PO/EV
Measured Spectral Response Function
IASI PFM testing in vacuum2 laser beams (B1:CO2, B3:HF/DF)
Field and Aperture illuminated
ISRF measured on +/- 16 cm-1 (+)Resolution (FWHM) compliant (w. margins)ISRF Model accuracy achievedISRF Model input are precisely measured
• Instrument Point Spread Function• Interferometric axis and shear• Corner Cube trajectory
B1 ISRF (944 cm-1)
B3 ISRF (2655 cm-1)
-1,0
-0,5
0,0
0,5
1,0
1,5
2,0
2,5
3,0
3,5
4,0
-16,00 -12,00 -8,00 -4,00 0,00 4,00 8,00 12,00 16,00Wave numbers (cm-1)
Nor
mal
ised
to S
urfa
ce
Measured P1 Model P1
-0,04
-0,03
-0,02
-0,01
0,00
0,01
0,02
0,03
-15,0 -14,5 -14,0 -13,5 -13,0
-0,5
0,0
0,5
1,0
1,5
2,0
2,5
3,0
-16,00 -12,00 -8,00 -4,00 0,00 4,00 8,00 12,00 16,00Wave numbers (cm-1)
Nor
mal
ised
to S
urfa
ce
Measured P1 Model P1
-0,20
-0,15
-0,10
-0,05
0,00
0,05
0,10
0,15
0,20
-4 -2 0 2 4
-0,025
-0,020
-0,015
-0,010
-0,005
0,000
0,005
0,010
-15,0 -14,5 -14,0 -13,5 -13,0
ITSC-14 – Beijing, 25-31May. 2005 10D. Blumstein – CNES DCT/PO/EV
Measured Spatial Response Function
Point Spread Function (IPSF) measured for the 3 IASI bandsInterband registration verified
Integrated absolute difference < 0.03
12 km FOV (at nadir)
ITSC-14 – Beijing, 25-31May. 2005 11D. Blumstein – CNES DCT/PO/EV
Spectral Performances (1/3)
First assessment done on few parametersDν/ν with respect to nominal instrumentSpectral resolution (Full Width at Half Maximum)
At 944 cm-1 (B1) and 2655 cm-1 (B3)
Shape error index Epsilon2 = variations of the ISRFAbsolute difference between average and instantaneous Summed over +/- 16 cm-1
Band 1 P1 P2 P3 P4 SpecificationDν/ν 2 10-4
FWHM cm-1 0.32 0.32 0.32 0.32 0.35cd0 0.014 0.014 0.010 0.011cd1 0.015 0.013 0.009 0.012
Band 3 P1 P2 P3 P4Dν/ν 2 10-4
FWHM cm-1 0.43 0.40 0.43 0.42 0.48cd0 0.020 0.025 0.015 0.019cd1 0.020 0.023 0.011 0.014
0.026
1 10-5
1 10-5
0.042
Epsilon2
Epsilon2
ITSC-14 – Beijing, 25-31May. 2005 12D. Blumstein – CNES DCT/PO/EV
Spectral Performances (2/3)
Spectral stability over 80 sec. Spec = 1.10-6
Standard deviation of the position of the quadratic barycentre of the ISRF
+ very good long term stability between measurement sessionsObserved Dν/ν (average of the 4 pixels) < 1.10-6
Hot Case / Cold Case
14 days between first and last measurements
Band 1 P1 P2 P3 P4cd0 8.27E-08 8.30E-08 7.70E-08 7.36E-08cd1 7.66E-08 7.46E-08 4.79E-08 8.08E-08
Band 3 P1 P2 P3 P4cd0 1.67E-08 2.29E-08 2.36E-08 1.66E-08cd1 1.58E-08 2.55E-08 2.09E-08 1.49E-08
ITSC-14 – Beijing, 25-31May. 2005 13D. Blumstein – CNES DCT/PO/EV
Spectral Performances (3/3)
Shape error index 1 Spec b1 < 0.02, Spec b3 < 0.05ISRF knowledge errors
Shape_index_1 = Σ( abs( Isrf_Model(n) – Isrf_Average(n) ) * dn )Ghost has to be removed from the averaged ISRF (computation on 13 cm-1)
Band 1 P1 P2 P3 P4cd0 0.025 0.023 0.023 0.023cd1 0.029 0.023 0.021 0.022cd0 0.034 0.031 0.026 0.027cd1 0.034 0.028 0.023 0.024
Band 3 P1 P2 P3 P4cd0 0.029 0.042 0.026 0.049cd1 0.032 0.046 0.019 0.050cd0 0.043 0.053 0.030 0.056cd1 0.039 0.056 0.021 0.053
+/- 13 cm
+/- 16 cm
+/- 13 cm
+/- 16 cm
ITSC-14 – Beijing, 25-31May. 2005 14D. Blumstein – CNES DCT/PO/EV
Summary
Excellent performances measured on 2nd IASI model (FM2)
The instrument ran flawlessly for the 3 weeks of test
Design modifications decided after PFM testing (ice contamination) successfully implemented on FM2 & FM3
• PFM model will be refurbished to benefit from these modifications
Big investment put into the on-ground calibration (human & financial)
Excellent stability of the instrument (spectral & radiometric)
Spectral Response Function of the instrument• Accurately measured at 2 wavenumbers (use of 2 laser beams for test)• Model accuracy verified at these 2 wavenumbers
ITSC-14 – Beijing, 25-31May. 2005 15D. Blumstein – CNES DCT/PO/EV
IASI Project Status : instruments (1/2)
FM2On-ground calibration completed (TVAC test in October 2004)Integration & tests on METOP 2 completedLaunch planned April 2006
FM3Subsystem Integration & Test completedThermal Vacuum Test planned in October 2005
PFMInstrument TVAC test in June 2003METOP Payload TVAC test in February 2004 Now dismounted from METOP 2Detectors refurbishment planned end of year 2005
ITSC-14 – Beijing, 25-31May. 2005 16D. Blumstein – CNES DCT/PO/EV
IASI Project Status : system (2/2)
OPS software (Level 1 processing) Delivered by CNES to EUMETSAT : Sept. 2004Now integrated & tested in CGSDelivered to METEO FRANCE for integration in direct readout software
TEC (IASI Technical Expertise Center) Acceptance test completed : Feb. 2005NRT terminal installed. First tests completedTEC ready for system level testing with EPS/CGS
Participation of IASI Instrument team to EPS system level tests with METOP 2 (SSVT4a, May 2005)
In-flight commissioning preparationInstrument on-orbit Verification Plan completedLevel 1 Cal/Val Plan completed (see poster B20), implementation on-going
ITSC-14 – Beijing, 25-31May. 2005 17D. Blumstein – CNES DCT/PO/EV
Aknowledgements
The authors would like to express their thanks to the many people involved in the development, integration and test of the IASI instruments either in the industry, in the space agencies or in the universities for their efforts which made IASI a reality.
A special thought goes to F.R.Cayla who has been so involved with IASI project since the beginning and is still very close from us in spite of his retirement four years ago.