Intercomparison of IASI and CrIS spectra

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Presentation transcript:

Intercomparison of IASI and CrIS spectra Bertrand THEODORE and Dorothee COPPENS Hyperspectral L1 team, EUMETSAT

Operational monitoring of IASI products Comparison with AVHRR Comparison with HIRS Inter-comparison IASI-A/IASI-B: Direct, using grand averages Double differences Inter-comparison with CrIS: Direct, using SNOs IASI (AMSU-A) (MHS) HIRS/4 AVHRR/3

Difference IASI-AVHRR vs. AVHRR Channel 4 Ch 4 slope intercept M02 -5.52929 0.000977 M01 -2.50335 -0.00118 Radiance difference (10-5 W/m2.sr.cm-1) M02 M01 Channel 5 Ch 5 Slope intercept M02 -4.89576 0.001079 M01 4.1248 -0.003821 Radiance difference (10-5 W/m2.sr.cm-1) Radiance (W/m2.sr.cm-1) Radiance (W/m2.sr.cm-1)

IASI vs. HIRS <BT> M02 M01 s(BT)

Double-differences IASI-A/IASI-B Developped for the commisioning of Metop-B and now part of the monthly monitoring RTM: RTTOV 9.3 T, q and p from ECMWF forecasts standard profiles of trace gases Selection of scenes: night time (sunza >=120 deg.) No polar regions (abs(lat) <= 60 deg) Over sea clear sky (Plot by Chander et al, 2013)

Double-differences IASI-A/IASI-B On-ground update IASI-A and IASI-B On-board update IASI-B No update On-board update IASI-A On-ground update IASI-A and IASI-B Difference always lower than 0.1K NedT => good radiometric consistency

Intercomparison with CrIS: context Since 31st July 2012, Suomi NPP CrIS SDRs are distributed by EUMETSAT as “pass through”: Extract BUFR bulletins Repack BUFR bulletins Rename file to WMO GTS standard Since 12th March 2013, SDRs include cloud data from the VIIRS instrument i.e. as “pass through” including: Decode netCDF cloud EDRs Re-grid and merge with co-located CrIS Dissemination of 2670 CrIS products / day

Why Comparing CrIS and IASI ? CrIS data monitoring Identify problems in the operational environment related to the products Assess the quality of the operational products Global instruments inter-calibration: Feed-back on other products disseminated by EUMETSAT New intercalibration using IASI for the GSICS community Why using IASI ? IASI on Metop-A has proven to be good reference Commissioning of IASI-B has shown that it has a similar quality to IASI-A

IASI and CrIS CrIS: three bands with different spectral resolutions Range (cm-1) Nb of Chan. Spectral Resolution LW 650-1095 713 0.625 MW 1210-1750 433 1.25 SW 2155-2550 159 2.5 IASI: one band with a single spectral resolution Band Range (cm-1) Nb of Chan. Spectral Resolution - 645-2760 8461 0.25

Comparing IASI to CrIS: methodology

Comparing CrIS and IASI: 2 approaches SNOs Comparison of Simultaneous Nadir Observations of IASI and CrIS Selection: 2 minutes time difference and 6.5 km distance difference Occurrence: every 7 weeks at high latitude (+/- 70 deg) Double Differences Comparison of IASI with CrIS through synthetic spectra Use of ECMWF 3-hourly forecast files Examination of the double-difference of ECMWF bias: DD=(RADobs - RADcalc)IASI – (RADobs – RADcalc)CrIS =>Remove most inaccuracies in both RTM and ECMWF

IASI/CrIS SNOs: selection Pairs are defined with time and distance criteria: 2 minutes 6.5 km Similar satellite zenith angles: ABS(cos(a1)/coa(a2)-1) <=0.01 Homogeneous scenes: Cloud fraction < 1 % Or > 99 %

IASI/CrIS SNOs: results North Pole: 2397 pairs IASI-B/CrIS: 2619 pairs South Pole: 1210 pairs IASI-A/CrIS: 3607 pairs North Pole: 1528 pairs CrIS slightly warmer than IASI in band 1 But possibly non-linearity effects in band 1 Very good agreement in band 2 (BT diff. < 0.07 K) Difficult to conclude in band 3 South Pole: 1091 pairs

OBS-CALC Double Differences: methodology RTM: RTTOV 10.2 T, q and p from ECMWF forecasts standard profiles of trace gases Selection of scenes: close to nadir (satza < 10 deg.) night time (sunza >=120 deg.) No polar regions (abs(lat) <= 60 deg) Over sea clear sky (Cloud fraction in each product)

OBS-CALC : selection of clear cases BT11 >= 280K BT11 – Tsurf >= 0 K -3 K < BT11 - BT3.9 < 1.5 K (OBS-CALC)BT11 <= 1 K Same distribution of CrIS and IASI pixels

OBS-CALC : selection of clear cases Geographical distribution IASI-A: 9799 spectra CrIS: 18958 spectra IASI-B 10199 spectra

Double differences: results for IASI-A

Double differences: results for IASI-B

Conclusions Set-up of a tool to compare CrIS and IASI -> Daily operational monitoring of CrIS products (Obs-Calc) -> Direct comparison at SNOs for inter-calibration check Define a good and reliable criteria to select clear cases using channels differences, not specific to IASI or CrIS. Shows good radiometric consistency between IASI and CrIS: Difference at NedT (at 280K) < 0.1 K Inter-calibration issues: in band 1: non-linearity correction needed ? in band 3: to be investigated

Intercomparison of IASI and CrIS spectra Thank you for your attention !