smos payload performance - earth.esa.intearth.esa.int/smos07/pres/05_pres.pdf · ideal g-matrix 1.-...
TRANSCRIPT
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1/337th SMOS Workshop, Frascati, 29-31 October 2007
SMOS Payload Performance
Manuel Martin-Neira, Michael Brown
SM-OS Project
European Space Agency
Josep Closa
EADS-CASA Espacio
and contributions from:
UPC and DEIMOS SMOS project teams
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2/337th SMOS Workshop, Frascati, 29-31 October 2007
Contents:
- Basic Equations
- Payload Performance Tests
- Performance over Temperature
- Image Validation
- Error Budget
- Future Work
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3/337th SMOS Workshop, Frascati, 29-31 October 2007
Basic Equations
Corbella Equation
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![Page 4: SMOS Payload Performance - earth.esa.intearth.esa.int/smos07/pres/05_pres.pdf · IDEAL G-Matrix 1.- same ... 6/33 7th SMOS Workshop, Frascati , 29-31 October 2007 Payload Performance](https://reader036.vdocuments.mx/reader036/viewer/2022062317/5a77dadf7f8b9aea3e8e591e/html5/thumbnails/4.jpg)
4/337th SMOS Workshop, Frascati, 29-31 October 2007
Basic Equations
Visibility Key Elements
kj
kj
jsysksys
kj MG
TTV
,,
=
NIR
PMS
Correlations
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5/337th SMOS Workshop, Frascati, 29-31 October 2007
Basic Equations
Imaging (Level-1 Processor)
kjV
IDEAL G-Matrix
1.- same antenna patterns
2.- no fringe-washing
2
221
n
rBF
TTT
!" ##$
#%
{ }VT IHFT=
BT
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6/337th SMOS Workshop, Frascati, 29-31 October 2007
Payload Performance Tests
The performance test plan of the SMOS payload included:
- Tests over temperature in the Large Space Simulator (LSS)
- Image validation in the Maxwell EMC chamber
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7/337th SMOS Workshop, Frascati, 29-31 October 2007
Payload Performance Tests
MIRAS in the Large Space Simulator
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8/337th SMOS Workshop, Frascati, 29-31 October 2007
Performance over Temperature
NIR and LICEF’s Temperature Profile
in the Large Space Simulator
hours
10 20 30 40 50 60
35 °C 35 °C
10 °C
22 °C
10 °C
0
T (°C)
10
20
30
–10
–20
nominal nominalredundant redundant
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9/337th SMOS Workshop, Frascati, 29-31 October 2007
Performance over Temperature
NIR Variation over Temperature
NIR Unit HOT WARM HOT WARM
AB H 0.15 0.22 0.11 0.18
AB V 0.02 0.09 0.02 0.04
BC H 0.02 0.02 0.02 0.09
BC V 0.07 0.09 0.02 0.07
CA H 0.07 0.11 0.04 0.11
CA V 0.07 0.09 0.02 0.04
Specification < 0.2 K/C ; 0.02 K/C with compensation
Temperature Drift for a 220 K Scene (K/C)
10 C --> 35 C 35 C --> 10 C
kj
kj
jsysksys
kj MG
TTV
,,
=
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10/337th SMOS Workshop, Frascati, 29-31 October 2007
Performance over Temperature
PMS Variation over Temperature
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11/337th SMOS Workshop, Frascati, 29-31 October 2007
Performance over Temperature
PMS Variation over Temperature
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12/337th SMOS Workshop, Frascati, 29-31 October 2007
Performance over Temperature
< 0.5 % (1-sigma)kj
kj
jsysksys
kj MG
TTV
,,
=
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13/337th SMOS Workshop, Frascati, 29-31 October 2007
Performance over Temperature
| Gkj | Variation over Temperature
kj
kj
jsysksys
kj MG
TTV
,,
=
| Gkj | < 0.3 % pp
(worst baseline)
LICEF temperatures
(same baseline)
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14/337th SMOS Workshop, Frascati, 29-31 October 2007
Performance over Temperature
Phase of Gkj and Mkj over Temperature
kj
kj
jsysksys
kj MG
TTV
,,
=
Arg {Gkj} = 16° pp
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15/337th SMOS Workshop, Frascati, 29-31 October 2007
Performance over Temperature
Peak-to-peak phase variation of Gkj (deg) over temperature
kj
kj
jsysksys
kj MG
TTV
,,
=
Peak-to-peak variations within segments are most of them below 0.5° (worst baseline is 1.5°)
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16/337th SMOS Workshop, Frascati, 29-31 October 2007
Performance over Temperature
LO phase variation tracking (in-orbit calibration)
- requires additional noise injection and Fourier or Spline interpolation;
- to minimise impact on coverage a new 4-epoch calibration sequence is introduced;
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17/337th SMOS Workshop, Frascati, 29-31 October 2007
Performance over Temperature
Frequency of noise injection to calibrate LO phase variations
- LSS: sampling !6 the main period is required (i.e. 7.6 min for 45 min period);
-Thermal model prediction for flight: orbital period dominant, thus 1 noise injection / 16 min;
- This frequency TBC during the commissioning phase;
- A reduction of the original short calibration to once a day would keep coverage loss < 1%
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18/337th SMOS Workshop, Frascati, 29-31 October 2007
Payload Performance Tests
MIRAS in the Maxwell EMC Chamber
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19/337th SMOS Workshop, Frascati, 29-31 October 2007
Image Validation
NIR sensitivity
Specification 0.25 0.25 0.55 0.55
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20/337th SMOS Workshop, Frascati, 29-31 October 2007
Image Validation
NIR Accuracy (using factory values)
NIR antenna temperature using factory values
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21/337th SMOS Workshop, Frascati, 29-31 October 2007
Image Validation
H-V Correlation Offset (Full-pol Mode)
Specification 1
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22/337th SMOS Workshop, Frascati, 29-31 October 2007
Image Validation
Correlation Offsets (1 cu = 10–4)
Specification
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23/337th SMOS Workshop, Frascati, 29-31 October 2007
Image Validation
Relative Phase Recovery
(H-pol)
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24/337th SMOS Workshop, Frascati, 29-31 October 2007
Image Validation
- PMS values are stable (gain variation < 0.2% over 12 h);
- Correlations are very stable (<0.5 cu over 12 h);
- Extremely marginal effects of X-band link (in practice, no effect);
- No effects from Star Tracker (with its shielding);
- All measurements show a high degree of consistency;
- All LICEFs are very similar -> highly separable in phase (FwF);
- Dynamic range is above 5 decades (8000 cu – 0.06 cu);
Other key results found in Maxwell:
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25/337th SMOS Workshop, Frascati, 29-31 October 2007
Image Validation
Imaging (Level-1 Processor)
kjV
IDEAL G-Matrix
1.- same antenna patterns
2.- no fringe-washing
2
221
n
rBF
TTT
!" ##$
#%
{ }VT IHFT=
BT
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26/337th SMOS Workshop, Frascati, 29-31 October 2007
Image Validation
{ }VT IHFT=
H-pol Modified Brightness Temperature
2
221
n
rBF
TTT
!" ##$
#%
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27/337th SMOS Workshop, Frascati, 29-31 October 2007
Image Validation
Amplification Factor
2
221
n
rBF
TTT
!" ##$
#%
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28/337th SMOS Workshop, Frascati, 29-31 October 2007
Image Validation
H-pol Brightness Temperature
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29/337th SMOS Workshop, Frascati, 29-31 October 2007
Image Validation
H-pol Brightness Temperature in AF-FoV
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30/337th SMOS Workshop, Frascati, 29-31 October 2007
Image Validation
H-pol Intermediate Radiometric Resolution
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31/337th SMOS Workshop, Frascati, 29-31 October 2007
Image Validation
H-pol Final Image Radiometric Resolution
"3 dB beam
boresight
2.3 K
4.6 K
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32/337th SMOS Workshop, Frascati, 29-31 October 2007
Error Budget
1.99 K RMS
3.26 K RMS
2.43 K RMS
3.98 K RMS
SAT-PDR
Actual Value
1.65 K RMS
3.31 K RMS
1.97 K RMS
3.94 K RMS
From IVT
(IDEAL reconstruction)
2.5 K RMS ( 00 )
4.1 K RMS ( 32 )
Level-1 OS
Radiometric Sensitivity
150 K
R-4.5.3-002-a,b
3.5 K RMS ( 00 )
5.8 K RMS ( 32 )
Level-1 SM
Radiometric Sensitivity
220 K
R-4.5.2-002-a,b
Specified ValueSystem ParameterSRD
Requirement
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33/337th SMOS Workshop, Frascati, 29-31 October 2007
Future Work
- Further detailed processing of LSS and IVT
- Validation of the LO calibration sequence
- Consolidation of the in-orbit calibration strategy
- Detailed validation of L1PP
- Empty chamber image of L1PP G-matrix
- Introduction of FTT+Gibbs/SDB Reduction in L1PP
- Performance analysis based on L1PP Maxwell images