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Progress of DCC Method in FY3A/MERSI and FY2
Chen Lin, Xiuqing Hu, Ling Sun CMA GPRC, National Satellite Meteorology Center
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OUTLINE Background DCC for Instrument Performance Monitoring of FY-3/MERSI DCC for Instrument Performance Monitoring of FY2D &FY2E Conclusions
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Background WHY DCC Advantage Disadvantage No need navigation;
Many targets; No sharp BRDF; Suitable for both GEO and LEO Easy to achieve …… Disadvantage Effect of stratosphere aerosols ; Rely on Thermal IR Too many data ……
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Radiative Transfer Model Simulation
SBDART model Surface: Sea water Background Tropospheric Aerosols : Oceanic 0.1; Background Stratospheric Aerosols: 0.02 Cloud Parameters: Ice cloud, Size 106um, Height 2-12km Ratio= The change of Reflectance with COD when COD>100, the ratio tend to 0
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Aerosols Effect Tropospheric Aerosols: Oceanic with AOD 0.1,0,2,0.5
Stratospheric Aerosols: Background 0.1 and 0.2 Fresh Volcano Ash 0.1 and 0.2
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effect the DCC Reflectance Angle Distribution Models
Angles Effect Different Angles will effect the DCC Reflectance Angle Distribution Models Should be Considered R, Anisotropic Factor Anisotropic Factor at SZA 15°(a)、25°(b)、35°(c)and 45°(d) over Ocean for Clear Sky of ice cloud with optical depth 50 ADMs based on CERES TRMM observations
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DCC as IPM for FY3/MERSI Methodology
DCC identification: Thermal IR TBB <205K; Latitude: 15°S to15°N; Longitude:0-360°; Surface: Ocean; Uniformity test: TBB in 3*3 grid box all less than 205K; STD of TBB in 3*3 grid box <1k STD of Ref in 3*3 grid box <1.5% Angles: Sun Zenith Angle<30°;View Zenith Angle<40° Statistics Bin: 10d or 30d Using the Pre-Launch Calibration table to calculate the nominal reflectance
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Spectral specification of MERSI bands
Center wl (mm) Width (mm) IFOV (m) NEDρ(%)/ NEDT (300K) Signal Dynamic Range 1 0.470 0.05 250 0.45 100% 2 0.550 0.4 3 0.650 4 0.865 5 11.25 2.5 0.54 K 330k 6 1.640 1000 0.08 90% 7 2.130 0.07 8 0.412 0.02 0.1 80% 9 0.443 10 0.490 11 0.520 12 0.565 13 14 0.685 15 0.765 16 17 0.905 0.10 18 0.940 19 0.980 20 1.030 4 channels IFOV 250m 2 shortwave IR channels (1640;2130) 4 channels central wavelength below 500nm(470nm 250m;412nm; 443nm;490nm) 3 water vapor channels
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Comparison 10d and 30d bin 10d disperse
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normalization 2σ 2σ :Double STD of DCC means to the fit curve
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Sensitivity of TBB Threshold
SZA and VZA Threshold is 40°, Ref bin=0.01 Mode:max(pdf) Mean: average Medium:mid-value SZA和VZA的阈值为40度,bin为0.01,考虑了ADMs校正,不同的红外TBB阈值判识的情况下,得到PDF的峰值随判识阈值变化。 Mode的值要大于平均值及中值,因为PDF的形态存在偏态分布,因此平均值和中值要小于mode值。平均值的稳定性最差,随TBB阈值变化较明显。中值最稳定。
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ADMs Effect Without ADMs With ADMs VZA 0-10;11-20;21-30,31-40
根据ADM分布图看出,对于角度在40°以内,是否经过ADMs有3~7%的差别。如果不经过校正,对于绝对辐射定标而言,就会引入3~7%的误差。虽然对于辐射定标跟踪来说影响应该不会很大,因为相当于是否都除以一个校正因子,但是对于其定标跟踪的稳定性也会起到一定的修正作用。 从经过ADMs校正前后,不同观测角度情况下的反射率PDF分布上来看,经过校正的反射PDF一致性要明显好于未校正,其PDF的形态和最大概率点都比较一致。具体数据见表格: 除了VZA在31-40°之间的mode值与别的角度下有差异,其余角度的mode值经过校正后就一致了。且无论Mode、Mean还是Medium不同角度的相对方差均表明经过ADMs校正后的值比未经过ADMs校正的方差均要小。说明ADMs的校正对于实现DCC的稳定性有一定的帮助。 VZA With ADMs Without ADMs Count Mode Mean Medium 0-10 0.760 0.704 0.666 0.831 0.772 0.706 30144 11-20 0.709 0.665 0.840 0.785 0.715 256436 21-30 0.779 564305 31-40 0.750 0.695 0.655 0.830 0.762 0.700 540100 0-40 0.701 0.774 STD 0.0060 0.0074 0.0069 0.0064 0.0111 0.0098
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Non-Linear decay of MERSI
First Year Second Year Third Year Forth Year Total linear nonlinear STD linear STD nonlinear Rate% 5.24 3.47 2.44 2.45 13.87 14.01 0.091 0.078
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The difference of 3 kinds of Method for monthly average
Total Nonlinear Mean Mode Medium STD nonlinear Rate% 14.3 14.82 14.4 0.078 0.082 Mean 和 medium得到的衰减率更接近。月平均结果与相应拟合线的标准差来看,Mean方式得到的标准差较小。但每个通道的情况可能会有所不同。
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Degradation has a little
Blue Channels 11.25 14.3 470(250m) 20.81 443 Degradation (Mean %) Wavelength (nm) 490 37.22 412 Shorter the channels wavelength is, Degradation is faster Degradation has a little bit nonlinear effect with time Significant Degradation
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Red Channels(1) 2.29 565 5.57 550(250m) Degradation (Mean %)
Wavelength (nm) 2.57 520
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Red Channels(2) Seem to be a lit bit rise -1.73 685 -2.06 650
Degradation (%) Wavelength (nm) -2.69 650(250m) Seem to be a lit bit rise
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Near Infrared Channels
1.48 865 -0.17 865(250m) Degradation (%) Wavelength (nm) 1030 -0.33 765 15.88 The most stable channel
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Water Vapor Channels 7.78 980 8.99 940 Degradation (Mean %) Wavelength
5.17 905
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WV wing
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Shortwave Infrared Channels
Jump Jump
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Total DegradationRate2 (%)
DCC Multi-Site Band 2σ/Mean (%) Total DegradationRate2 (%) Jul to Jul. 2009 Jul to Jul. 2010 Jul to Jul. 2011 Jul to Jun. 2012 Total Degra Rate2 (%) Multi-DCC 1 14.03 5.24 3.47 2.44 2.76 3.12 17.81 7.85 6.17 5.38 3.78 2 5.58 1.97 1.12 1.21 1.16 2.49 8.93 3.94 2.46 2.99 3.35 3 -2.26 -1.19 -0.5 -0.73 -0.56 2.31 -2.41 -1.45 -1.18 -0.37 -0.15 4 0.34 -1.91 0.73 0.04 0.67 2.08 -0.30 -3.00 -0.80 0.26 -0.64 8 35.88 9.98 8.54 8.03 9.61 5.05 37.30 15.40 10.11 8.02 1.42 9 19.67 6.34 4.55 4.04 5.93 3.68 23.45 10.19 7.26 6.55 10 11.03 3.82 2.88 2.04 2.2 2.70 15.35 6.72 4.71 4.32 11 2.62 -0.42 0.4 -0.91 0.15 2.68 11.79 6.01 3.49 3.88 9.17 12 1.07 0.64 0.11 0.12 2.03 5.88 2.92 2.21 3.42 13 -1.73 -1.3 -0.33 -0.67 -0.53 -1.29 -1.62 -1.89 -1.07 0.44 14 -1.44 -0.94 -0.41 -0.84 -0.65 2.12 -1.56 -1.60 -0.75 -0.12 15 1.59 0.96 0.32 0.06 0.02 2.67 1.77 1.04 0.22 0.37 0.18 16 -2.56 -0.1 -1.58 1.54 1.19 -0.83 1.84 17 4.57 -0.31 0.58 0.29 4.22 6.98 2.41 18 7.32 -0.52 1.58 1.48 14.95 14.22 6.9 19 6.96 1.32 1.34 5.09 9.97 3.01 20 13.15 -0.28 4.05 3.32 3.96 15.73 2.73 3.33 3.58 2.58 The difference between DCC and Multi-site in most Bands are smaller than 4% There are big differences in Band 10 and 11 band Center wl (mm) Width (mm) IFOV (m) NEDρ(%)/ NEDT (300K) Signal Dynamic Range 8 0.412 0.02 1000 0.1 80% 9 0.443 10 0.490 0.05 11 0.520 12 0.565 13 0.650 14 0.685 15 0.765
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DCC as IPM for FY2 Methodology
DCC identification: Thermal IR TBB <205K; For the time of later August 2011, <203K Latitude: 20°S to20°N; Longitude:85°E to 125°E(FY2E); 55°E to 95°E(FY2D); Surface: Ocean; Uniformity test: TBB in 3*3 grid box all less than 205K/ <203K; STD of TBB in 3*3 grid box <1.5k STD of Ref in 3*3 grid box <1.5% Angles: 15°<Sun Zenith Angle<40°;View Zenith Angle<30° Statistics Bin: 30d For FY2E images time is between 5:00 and 8:00; For FY2D images time is between 3:00 and 6:00;
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About 5% Degradation of FY2E in the past 2 years
Compare to FY2E, FY2D is quite stable Big difference of DCC reflectance between FY2D and FY2E is questionable
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Conclusion CMA began a testing of DCC method for FY-3A/MERSI.
DCC method provide good consistent results for MERSI degradation with other method. It is a good reference for MERSI degradation monitoring. DCC can obtain more stable results for NIR water vapor bands with low seasonal oscillation. DCC method is ongoing for FY-2 visible band. DCC inter-calibrtaion for FY-2 visible band based on MODIS will be conducted in the near future (Following Dave Doelling ATBD). Uncertainty analysis of DCC will be also conducted.
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