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www.le.ac.uk Requirements Consolidation of the Near- Infrared Channel of the GMES-Sentinel-5 UVNS Instrument Scattering profile characterisation for SWIR Leif Vogel, Hartmut Boesch University Leicester

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Requirements Consolidation of the Near-Infrared Channel of the GMES-Sentinel-5 UVNS Instrument

Scattering profile characterisation for SWIR

Leif Vogel, Hartmut BoeschUniversity Leicester

Approach for Retrieval Simulations

• Spectra are simulated using the forward model of UoL FP retrieval algorithm for a range of geophysical scenarios

• Sensitivity tests for retrievals w.r.t. scattering profiles, i.e. the retrieval applies

• the same a priori trace gas profiles, temperature profile, surface albedo

• different setup for aerosol and cirrus a priori

• Maximal sensitivity to scattering induced errors

• Bias given by difference between true and retrieved XCH4

The UoL Retrieval Algorithm

• Measured radiance spectra are non-linear function of atmospheric parameters• retrieval is performed iteratively by

alternating calls to FW and IM

• Forward Model describes physics of measurement: • Multiple-scattering RT• Instrument Model• Solar Model

• Inverse Method estimates state: • Rodger’s optimal estimation

technique

• XCH4, XCO and its error is computed from retrieved state after iterative retrieval has converged

Names Quantity Notes

CO and CH4 1 Multiplier to a priori profile

H2O, HDO, CO2 1 Multiplier to a priori profile

Temperature 1 Additive offset to a priori profile

2 Aerosols AOD, height and width

Gauss profile

Cirrus clouds AOD, height and width

Gauss profile

Surface Albedo #bands x 2para Albedo at band centre and slope

Typical State Vector

Retrieved properties

Concept A        Bands NIR (685 – 773 nm)* SWIR 1 SWIR3

  NIR 1 NIR 2    

Wavelengths [nm] 685 - 700 750 – 773 1590 - 1675 2305 - 2385

Numbers of pixel 116 177 850 800

FWHM ISF 0.39 0.39 0.25 0.25

*) Simulated retrievals do not use full range due to strongly changing surface albedo

         Concept B        

Instrumental setup

Instrumental errors (ECHAM Scenarios)

• Aerosol profiles originating from ECHAM 5 model simulations (Stier et al 2005)

• Global coverage for one day (April 15th, 2015)

• Atmosphere: 18-level profile

• SZA: noon local time (27º- 87º)

• Total AOD given by MODIS measurements

• Surface albedo determined by MODIS and Sciamacy data

Geophysical scenario described in Butz et al. 2010, Butz et al. 2012

ECHAM Kahn et al. 2001

Mode Aerosols Base/Mixt. Aerosols

Nucleation SU Base SU land

Aitken SU, BC, POM Mix 5a SU, acc.DU, BC, Carb

Accumulation SU, BC, POM, SS, DU Mix 3a SU, SS, BC, Carb

Coarse SU, BC, POM, SS, DU Mix 4a SU, acc.DU, coarse DU, Carb

Aitken BC, POM Mix 3b BC, Carb, SU, SS

Accumulation DU Base Acc. DU

Coarse DU Base Coarse DU

Cirrus clouds

Calipso data, Gaussian profile, optical properties from Baum et al. (2005) for reff = 60µm

ECHAM Desaster

Simulated ECHAM scenarios

Sensitivity to radiometric accuracy

• Linear mapping of errors has been used to determine additive and multiplicative ARA errors – Additive gain: 3% of trop dark scenario in

respective band– Multiplicative gain: 3% for NIR1 and 2

• RSRA/ESRA errors determined by SWIR study

Simulated ECHAM scenarios

additive ARA

Error source

ECHAM Scenarios; Concept A

Instrumental

Std dev mean

ARA-additive

NIR 1 0.703 -0.207

NIR 2 1.072 0.881

NIR

1N

IR 2

Simulated ECHAM scenarios

multiplicative ARA

Error source

ECHAM Scenarios; Concept A

Instrumental

Std dev mean

ARA-multiplicative

NIR 1 0.750 -0.258

NIR 2 0.946 0.494

NIR

1N

IR 2

Simulated ECHAM scenarios

Sensitivity to ISRF

ISF  

nominal Gaussian function convolved with a box-car, fitted to the ESA supplied function

asy1pc

Independently scaling the width of the nominal function on either side of the peak. Asymmetry is introduced with a maximum impact of 1% of the peak value of the nominal function

homm Scene inhomogeneityGradient in along-slit illumination (10% of the mean illumination, direction of assumed gradient “…m” or “…p”)homp

idisp-1 Spectrally offset versions of the nominal slit function are added to the slit function itself; ISRF with the same centre of mass and FWHM as the original pattern. (error falls with then 1% enveloped of the requirement)

idisp1

idisp-2

idisp2

idisp-3

idisp3

wid1pc The effect of perturbing the width of the nominal function by 1%

• Linear mapping of errors has been used to determine sensitivity to ISRF

• 11 different slit functions are studied

asymmetry

Scene inhom

Spectral offset

width

Simulated ECHAM scenarios

Sensitivity to ISRF

R. Siddans

Simulated ECHAM scenarios

Sensitivity to ISRF

Sensitivity to ISRF

• Greatest CH4 error via idisp-3

• NIR 1 channel much less sensitive

• Allowing for the retrieval algorithm to spectrally shift and squeeze may mitigate (or mask) effects

ISFCH4 bias

NIR1 mean [%]

NIR1 std [%]

NIR2 mean [%]

NIR2 std [%]

Total mean [%]

Total std [%]

asy1pc -0.006 0.007 -0.007 0.024 0.010 0.025idisp-1 -0.003 0.084 0.163 0.298 0.163 0.309idisp1 -0.013 0.082 0.121 0.232 0.122 0.246idisp-2 0.005 0.096 0.207 0.358 0.207 0.371idisp2 -0.009 0.092 0.120 0.234 0.120 0.251idisp-3 0.014 0.107 0.236 0.402 0.237 0.416idisp3 -0.002 0.106 0.120 0.264 0.120 0.285wid1pc -0.018 0.099 0.172 0.342 0.173 0.356

Total range (asy1pc – idisp-3)

-0.006 – 0.14

0.007 – 0.107

-0.007 – 0.120

0.024 – 0.402

0.010 – 0.237

0.025 – 0.416

Simulated ECHAM scenarios

ISFCH4 bias

NIR1 mean [%]

NIR1 std [%]

NIR2 mean [%]

NIR2 std [%]

Total mean [%]

Total std [%]

homm0.035 0.071 -0.033 0.464

0.048

0.469

homp-0.035 0.071 0.034 0.465

0.048

0.470

             Scene Inhomogeneity

   

homm; homp0.035 0.071 0.034 0.465

0.048

0.469

Sensitivity to ISRF, Scene inhomogeniety

• NIR 1 channel much less sensitive

• Homm; homp slit function errors are not independent– Error of scene inhomogeneity is given as absolute mean

• Introduced bias is very low with 0.048%

• A greater variability in the NIR2 channel leads to total standard deviation of 0.469%.

Simulated ECHAM scenarios

Instrumental errors (ECHAM)

ConclusionsError source ECHAM Scenarios; Concept A

Instrumental Std dev mean

ARA-multiplicative 1)

NIR 1 0.750 -0.258

NIR 2 0.946 0.494

ARA-additive 2)NIR 1 0.703 -0.207

NIR 2 1.072 0.881

RSRA or ESRA 3) Done by SWIR study group

1 0

ISRF variations 4)

NIR 1 0.007 - 0.107 -0.006 - 0.014

NIR 2 0.024 - 0.402 -0.007 - 0.237

Scene inhomogeneity 5)

NIR 1 0.071 0.035

NIR 2 0.465 0.034

 Total Instrumental 6)

NIR1 and NIR2 2.0791 - 2.120 1.064 - 1.090

Only NIR 2 1.780 - 1.787 0.814 - 0.816

ARA requirements: Mean CH4 accuracy meets requirements, but standard deviation is rather high.

Reduction would be beneficial

Simulated MACC scenarios

Simulations with ECHAM 5 model simulations as described in Stier et al 2005, Butz et al 2010, Butz et al 2012

Description of atmospheric parameters and aerosol optical properties not directly transferable to the UoL algorithm.

Calculated aerosol optical properties are either dust or sulphate dominated

ECHAM 5 aerosols replaced with aerosols from MACC, ECWMF integrated forecasting system (IFS), 12h GMT April 14th 2010

Use atmospheric data from the previous scenarios in combination with ECMWF aerosols to increase number of successful retrievals

ECHAM Desaster

MACC vs. ECHAM Scenarios

Replace only aerosols All other scenario

information remains unchanged

Cirrus clouds, atmosphere, pressure levels, surface albedo, etc.

Different retrievals for MACC simulationsAerosol parameterization:

• Use two linear combination of aerosol types to approximate true type

• 2 generic Gaussian aerosol extinction profiles (altitude =2km agl, width = 1.5km, aod = 0.1)

• Cirrus (altitude 10km agl, width =1km, cod = 0.05

In total 8 global retrievals to study representation errors`

Representation errors(MACC scenarios)

Forwardsimulations

Retrieval

Without fluorescence With fluorescence

2 aerosols NIR1 and NIR2 Only NIR2 NIR1 and NIR2 Only NIR2

2 aerosls with zero level offset (fluorescence mitigation)

NIR1 and NIR2 Only NIR2 NIR1 and NIR2 Only NIR2

Simulation of fluorescene

• Fluorescence data supplied by L. Guanter

• FS Spectra added to simulated Spectra taking into account respective aerosol load and viewing direction

NIR 1&2 NIR 1&2NIR 2 NIR 2without fluorescence with fluorescence

with

out o

ffset

with

offs

etRepresentation errors

(MACC scenarios)

Some regional differences can be observed:• effect of fluorescence (without offset correction)• Indication that zero level offset may couple unfavourably with

cirrus clouds• Similar coverage of NIR 1&2 and NIR 2 only retrievals

CH4 bias [%]NIR 1&2 NIR 1&2NIR 2 NIR 2

without fluorescence with fluorescence

with

out o

ffset

with

offs

etRepresentation errors

(MACC scenarios)

Blue: converged retrievals over ice-free landGreen: a-posteriori filter is applied

NIR 1&2 NIR 1&2NIR 2 NIR 2without fluorescence with fluorescence

with

out o

ffset

with

offs

et

CH4 retrieval error [%]

Blue: converged retrievals over ice-free landGreen: a-posteriori filter is applied

Representation errors(MACC scenarios)

MACC scenarios

Converged MACC Scenarios

Error sourceNIR1 and NIR2(O2-A and O2-B band)

NIR2(O2-A band)

Error CH4 [%] std dev mean bias Mean precision

# retrievals 1) std dev mean bias Mean

precision# retrievals 1)

No FS, no offset 0.609 -0.067 0.127 1269 (65%) 0.864 -0.168 0.162 1419

(74%)

No FS, offset 0.838 -0.052 0.196 1429 (74%) 1.039 -0.116 0.224 1659

(86%)

FS, no offset 0.874 0.000 0.129 1069 (55%) 0.793 -0.108 0.162 1353

(70%)

FS, offset 0.831 -0.049 0.197 1395 (72%) 1.066 -0.129 0.226 1623

(84%)

1) Number of converged retrievals out of a total of 1933 simulated measurements over land and ice free surface.

All retrievals fulfill requirements• Less converged retrievals for NIR 1&2 than for only NIR2

<->Tighter boundary conditions due to O2-B band• Retrievals with NIR 1&2 show better performance in random and systematic errors

• Fluorescence leads to higher errors, but its effect can be mitigated• Indication that aerosol information in the O2-B band constrains the retrievals at cost

of lesser coverage <-> filtering effect

SummaryInstrumental errors from ECHAM ScenariosInstrumental Systematic 1) Pseudo random 2) Random 3)

ARA-multiplicativeNIR 1 -0.258 0.750  

NIR 2 0.494 0.946  

ARA-additiveNIR 1 -0.207 0.703  

NIR 2 0.881 1.072  

RSRA or ESRA 4) Done by SWIR study group

0 1  

ISRF variations 5)NIR 1 -0.006 - 0.014 0.007 - 0.107  

NIR 2 -0.007 - 0.237 0.024 - 0.402  

Sceneinhomogeneity

NIR 1 0.035 0.071  

NIR 2 0.034 0.465  

 Total Instrumental 6)NIR1 and NIR2 1.064 - 1.090 2.0791 - 2.120  

Only NIR 2 0.814 - 0.816 1.780 - 1.787  

Representation errors from MACC scenariosConverged but not filtered results

 Systematic 1) Pseudo random 2) Random 3)

Simulation with Fluorescence, retrieval with 2 aerosols and zero level offset

NIR1 and NIR2(1395, 72%)

0.049 0.831 0.197

Only NIR 2(1623, 84%)

0.129 1.066 0.226

         

Total error 9)

NIR1 and NIR2 1.065 - 1.091 2.239 - 2.277 0.197

Only NIR 2 0.824 - 0.826 2.075 - 2.081 0.2261) Systematic is described here by the mean bias2) Pseudo random is described as the standard deviation of the mean bias 3) Random is given by the mean of the retrieval error where applicable.4) 50% of user requirement5) Minimum and maximum values from the ILS variations. Min. variations are taken from asy1pc, max. values from idisp-36) The two values result from the assumed minimum and maximum error of the ILS

Conclusion:• Retrievals have been performed with two geophysical

Scenarios based on ECHAM and MACC aerosol distributions for instrumental and representation errors.

• Most error sources lead to results inline with the requirements. However, additive and multiplicative ARA induced errors are high. Reduction of these error sources is desirable.

• Representation errors meet the requirements. • Using a two NIR (O2-A & B) band retrieval increases

accuracy at the cost of slightly diminished coverage, and its use is beneficial to prevent erroneous results.

• The effect of fluorescence can be mitigated using a zero level offset.

• Further potential lies in improved aerosol representations (regional dependencies, climatology, improved optical properties), which may also lead to increased coverage.