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GERB STM, Exeter, Oct. 20061 SW Diurnal Errors in ERB monthly means: some studies from CERES and GERB LMD/IPSL M. Viollier and A. Ben Rehouma Ecole Polytechnique, Palaiseau, France
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GERB STM, Exeter, Oct. 20062 Comparison between the SW monthly means over two regions Reg#1 the whole area (45°S-45°N/60°W-60°E) Reg#2 (35°-10°S/10°W-10°E) with systematic diurnal cycle sharp diurnal errors SW standard deviation Month: August
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GERB STM, Exeter, Oct. 20063 SW Mean over Reg#1 Monthly Anomaly defined / all available years Scanners Nonscanner ISCCP-FD Negative trend See also, Wong et al (2006) Zhang et al (2004), for the tropical mean
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GERB STM, Exeter, Oct. 20064 Regional Anomaly (Reg # 2 – Reg # 1) Nonscanner ISCCP-FD +1.5 ± 3.0 +3.0 ± 0.8 Slope Wm -2 /decade ± taking autocorrelation into account, according to Weatherhead et al JGR (1998) More on our Friday presentation
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GERB STM, Exeter, Oct. 20065 Scanner Serie (Reg # 2 – Reg # 1) with Terra with Average of Terra and Aqua +5.0 ±1.5 +1.1 ± 2.0
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GERB STM, Exeter, Oct. 20066 Diurnal corrections for CERES-Terra, several approaches SRBAVG geo products ( about 2 years, 2000/03 2004/05) Combination (or average) of Terra and Aqua (ES4, about 4 years, 2002/07 2005/12) Examination of GERB ARG Ed1 products 5 months: 2006, 04 to 08)
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GERB STM, Exeter, Oct. 20067 Diurnal error, January 2003 Computed from differences between CERES SRBAVG GEO – NON GEO 1 x 1° Computed from differences between (Aqua+Terra) and Terra alone 2.5 x 2.5 °
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GERB STM, Exeter, Oct. 20068 Diurnal error, October 2003
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GERB STM, Exeter, Oct. 20069 SW Diurnal Errors, reg 2 (up), reg 1 (down) REG2 REG1
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10 Comparisons between contemporary T-(TA) and nonGeo-Geo / 2003 Agreement at least for these areas and their differences; the variations are higher for SRBAVG
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GERB STM, Exeter, Oct. 200611 Same for Albedo, 2003
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GERB STM, Exeter, Oct. 200612 GERB, 2006 July, 17-18 LW flux SW flux
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GERB STM, Exeter, Oct. 200613 Diurnal Cycle – August 2006 Area: 2.5x2.5° X 100
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GERB STM, Exeter, Oct. 200614 Albedo Diurnal Cycle – hourly means- off Angola Area: 2.5x2.5° May 2006April 2006 July 2006 Aug 2006
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GERB STM, Exeter, Oct. 200615 Albedo Diurnal Cycle – hourly means- Sahara Area: 2.5x2.5° May 2006April 2006 July 2006 Aug 2006
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GERB STM, Exeter, Oct. 200616 SW Monthly Means Computations with GERB Average the fluxes (2.5°x2.5°) and fill the 24x31 day-hour table Use ‘ERBE-type’ code, with Terra flux estimates (ES9- Ed1 - CV ) to compute monthly means Repeat using the GERB observed diurnal albedo variation shape in place of the ERBE modeled albedo
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GERB STM, Exeter, Oct. 200617 GERB April 2006 GERB2006
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GERB STM, Exeter, Oct. 200618 SRBAVG, TA and GERB April GERB2006 SRBAVG2003 SRBAVG2002 TA2003
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GERB STM, Exeter, Oct. 200619 SRBAVG, TA and GERB August SRBAVG 2001 GERB2006 SRBAVG2003 TA2003
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GERB STM, Exeter, Oct. 200620 Summary of Diurnal Errors Wm -2 Reg2 – Reg1JJANDJYear SRBAVG nonGeo-Geo 4.610.46.5 Terra- Ave( Terra,Aqua) 4.29.46.6 GERB correction applied to Terra 4.9-- Caution: Not the same years for each case
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GERB STM, Exeter, Oct. 200621 Conclusion We have looked for inter-regional differences in the evolution of the SW reflected flux (Reg1, Reg2) Reg 2 (South East Atlantic): diurnal errors are critical when using ES4-Terra (morning observation) Significant agreement between 3 independent evaluations of the relative diurnal errors (SRBAVG, Aqua, GERB); waiting for overlapping periods This is shown only for the studied regions and for their differences The 1985-2005 SW positive change (relatively to the average Reg1) observed with Terra seems slightly greater than the diurnal error
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22 Indo-French Megha-Tropiques satellite project - 2009 Saphir : microwave sounder for water vapour sounding : 6 channels in the WV absoption band at 183.31 GHz. (cross track, 10 km) MADRAS : microwave imager for precipitation : channels at 18, 23, 37, 89 and 157 GHz, H and V polarisations. (conical swath, <10 km to 40 km) ScaRaB
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GERB STM, Exeter, Oct. 200623 The three instruments of Megha-Tropiques ScaRaB : wide band instrument for inferring longwave and shortwage outgoing fluxes at the top of the atmosphere (cross track scanning, 40 km resolution at nadir) Saphir : microwave sounder for water vapour sounding : 6 channels in the WV absoption band at 183.31 GHz. (cross track, 10 km) MADRAS : microwave imager for precipitation : channels at 18, 23, 37, 89 and 157 GHz, H and V polarisations. (conical swath, <10 km to 40 km)
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