首页> 外文会议>Conference on earth observing missions and sensors: development, implementation, and characterization IV >Cross-calibration of the Oceansat-2 Ocean Colour Monitor (OCM) with Terra and Aqua MODIS
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Cross-calibration of the Oceansat-2 Ocean Colour Monitor (OCM) with Terra and Aqua MODIS

机译:海洋型海洋彩色监视器(OCM)的交叉校准与Terra和Aqua Modis

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The Ocean Colour Monitor (OCM) sensor on-board the Oceansat-2 spacecraft has been operational since its launch in September, 2009. The Oceansat 2 OCM primary design goal is to provide continuity to Oceansat-1 OCM to obtain information regarding various ocean-colour variables. OCM acquires Earth scene measurements in eight multi-spectral bands in the range from 402 to 885 nm. The MODIS sensor on the Terra and Aqua spacecraft has been successfully operating for over a decade collecting measurements of the earth's land, ocean surface and atmosphere. The MODIS spectral bands, designed for land and ocean applications, cover the spectral range from 412 to 869 nm. This study focuses on comparing the radiometric calibration stability of OCM using near-simultaneous TOA measurements with Terra and Aqua MODIS acquired over the Libya 4 target. Same-day scene-pairs from all three sensors (OCM, Terra and Aqua MODIS) between August, 2014 and September, 2015 were chosen for this analysis. On a given day, the OCM overpass is approximately an hour after the Terra overpass and an hour before the Aqua overpass. Due to the orbital differences between Terra and Aqua, MODIS images the Libya 4 site at different scan-angles on a given day. Some of the high-gain ocean bands for MODIS tend to saturate while viewing the bright Libya 4 target, but bands 8-10 (412 nm - 486 nm) provide an unsaturated response and are used for comparison with the spectrally similar OCM bands. All the standard corrections such as bidirectional reflectance factor (BRDF), relative spectral response mismatch, and impact for atmospheric water-vapor are applied to obtain the reflectance differences between OCM and the two MODIS instruments. Furthermore, OCM is used as a transfer radiometer to obtain the calibration differences between Terra and Aqua MODIS reflective solar bands.
机译:海洋彩色监视器(OCM)传感器车载船上雪橇 - 2宇宙飞船以来,自2009年9月推出以来一直在运营。海洋2 OCM主要设计目标是为Oceansat-1 OCM提供连续性,以获得各种海洋的信息 - 颜色变量。 OCM在八个多光谱带中获取地球场景测量范围为402至885nm。 Terra和Aqua SpaceCraft上的MODIS传感器已经成功运营了地球土地,海洋表面和大气的十年。为陆地和海洋应用设计的MODIS光谱带,覆盖412至869 nm的光谱范围。本研究侧重于使用近同时TOA测量与利比亚4目标获取的近同时TOA测量比较OCM的辐射校准稳定性。选择了来自所有三个传感器(OCM,Terra和Aqua Modis)的当天场景对,2015年和2015年9月在此分析中选择了。在给定的一天,OCM立交桥大约是Terra立交桥和Aqua立交桥前一小时的一小时。由于Terra和Aqua之间的轨道差异,MODIS在给定日期以不同的扫描角图像图像图像。 Modis的一些高增益海洋带往往在观察明亮的利比亚4靶的同时饱和,但带8-10(412nm-486nm)提供了不饱和的反应,并且用于与光谱相似的OCM频带进行比较。应用了双向反射率因数(BRDF),相对光谱响应不匹配和对大气水蒸气的影响的所有标准校正,以获得OCM和两个MODIS仪器之间的反射差异。此外,OCM用作转移辐射计,以获得Terra和Aqua Modis反射太阳能带之间的校准差异。

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