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On-Orbit Calibration and Performance of Aqua MODIS Reflective Solar Bands

机译:Aqua MODIS反射太阳波段的在轨校准和性能

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摘要

Aqua MODIS has successfully operated on-orbit for more than 6 years since its launch in May 2002, continuously making global observations and improving studies of changes in the Earth's climate and environment. 20 of the 36 MODIS spectral bands, covering wavelengths from 0.41 to 2.2 microns, are the reflective solar bands (RSB). They are calibrated on-orbit using an on-board solar diffuser (SD) and a solar diffuser stability monitor (SDSM). In addition, regularly scheduled lunar observations are made to track the RSB calibration stability. This paper presents Aqua MODIS RSB on-orbit calibration and characterization activities, methodologies, and performance. Included in this study are characterizations of detector signal-to-noise ratio (SNR), short-term stability, and long-term response change. Spectral wavelength dependent degradation of the SD bidirectional reflectance factor (BRF) and scan mirror reflectance, which also varies with angle of incidence (AOI), are examined. On-orbit results show that Aqua MODIS onboard calibrators have performed well, enabling accurate calibration coefficients to be derived and updated for the Level 1B (L1B) production and assuring high quality science data products to be continuously generated and distributed. Since launch, the short-term response, on a scan-by-scan basis, has remained extremely stable for most RSB detectors. With the exception of band 6, there have been no new RSB noisy or inoperable detectors. Like its predecessor, Terra MODIS, launched in December 1999, the Aqua MODIS visible (VIS) spectral bands have experienced relatively large changes, with an annual response decrease (mirror side 1) of 3.6% for band 8 at 0.412 microns, 2.3% for band 9 at 0.443 microns, 1.6% for band 3 at 0.469 microns, and 1.2% for band 10 at 0.488 microns. For other RSB bands with wavelengths greater than 0.5 microns, the annual response changes are typically less than 0.5%. In general, Aqua MODIS optics degradation is smaller than Terra MODIS and the mirror side differences are much smaller. Overall, Aqua MODIS RSB on-orbit performance is better than Terra MODIS.
机译:自2002年5月发射以来,Aqua MODIS已在轨道上成功运行了6年多,不断进行全球观测并改进对地球气候和环境变化的研究。反射太阳波段(RSB)是36个MODIS光谱带中的20个,覆盖从0.41到2.2微米的波长。使用车载太阳能扩散器(SD)和太阳能扩散器稳定性监控器(SDSM)在轨道上对它们进行了校准。此外,定期进行月球观测以跟踪RSB校准的稳定性。本文介绍了Aqua MODIS RSB在轨校准和表征活动,方法和性能。这项研究包括检波器信噪比(SNR),短期稳定性和长期响应变化的特征。考察了SD双向反射系数(BRF)和扫描镜反射系数的光谱波长相关衰减,这些衰减也随入射角(AOI)而变化。在轨结果表明,Aqua MODIS机载校准器运行良好,能够为1B级(L1B)生产得出和更新准确的校准系数,并确保连续生成和分发高质量的科学数据产品。自发射以来,对于大多数RSB检测器而言,逐个扫描的短期响应一直非常稳定。除频段6外,没有新的RSB噪声或不可操作的检测器。像其前身Terra MODIS(于1999年12月推出)一样,Aqua MODIS可见(VIS)光谱带经历了相对较大的变化,第8波段在0.412微米处的年度响应下降(镜面1)为3.6%,对于8波段的年响应下降为(2.3%)。 9号带在0.443微米处,带3在0.469微米处为1.6%,带10在0.488微米处为1.2%。对于其他波长大于0.5微米的RSB波段,年响应变化通常小于0.5%。通常,Aqua MODIS的光学性能下降要小于Terra MODIS,并且镜侧差异要小得多。总体而言,Aqua MODIS RSB在轨性能优于Terra MODIS。

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