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,

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Presentation transcript:

GERB STM, Exeter, Oct 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

GERB STM, Exeter, Oct 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

GERB STM, Exeter, Oct 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

GERB STM, Exeter, Oct Regional Anomaly (Reg # 2 – Reg # 1) Nonscanner ISCCP-FD +1.5 ± ± 0.8 Slope Wm -2 /decade ±  taking autocorrelation into account, according to Weatherhead et al JGR (1998) More on our Friday presentation

GERB STM, Exeter, Oct Scanner Serie (Reg # 2 – Reg # 1) with Terra with Average of Terra and Aqua +5.0 ± ± 2.0

GERB STM, Exeter, Oct 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)

GERB STM, Exeter, Oct 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 °

GERB STM, Exeter, Oct Diurnal error, October 2003

GERB STM, Exeter, Oct SW Diurnal Errors, reg 2 (up), reg 1 (down) REG2 REG1

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

GERB STM, Exeter, Oct Same for Albedo, 2003

GERB STM, Exeter, Oct GERB, 2006 July, LW flux SW flux

GERB STM, Exeter, Oct Diurnal Cycle – August 2006 Area: 2.5x2.5° X 100

GERB STM, Exeter, Oct Albedo Diurnal Cycle – hourly means- off Angola Area: 2.5x2.5° May 2006April 2006 July 2006 Aug 2006

GERB STM, Exeter, Oct Albedo Diurnal Cycle – hourly means- Sahara Area: 2.5x2.5° May 2006April 2006 July 2006 Aug 2006

GERB STM, Exeter, Oct 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

GERB STM, Exeter, Oct GERB April 2006 GERB2006

GERB STM, Exeter, Oct SRBAVG, TA and GERB April GERB2006 SRBAVG2003 SRBAVG2002 TA2003

GERB STM, Exeter, Oct SRBAVG, TA and GERB August SRBAVG 2001 GERB2006 SRBAVG2003 TA2003

GERB STM, Exeter, Oct Summary of Diurnal Errors Wm -2 Reg2 – Reg1JJANDJYear SRBAVG nonGeo-Geo Terra- Ave( Terra,Aqua) GERB correction applied to Terra Caution: Not the same years for each case

GERB STM, Exeter, Oct 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 SW positive change (relatively to the average Reg1) observed with Terra seems slightly greater than the diurnal error

22 Indo-French Megha-Tropiques satellite project Saphir : microwave sounder for water vapour sounding : 6 channels in the WV absoption band at 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

GERB STM, Exeter, Oct 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 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)