Eplee Robert E, Sun Jun-Qiang, Meister Gerhard, Patt Frederick S, Xiong Xiaoxiong, McClain Charles R
Science Applications International Corporation, 4600 Powdermill Road, Suite 400, Beltsville, Maryland 20705, USA.
Appl Opt. 2011 Jan 10;50(2):120-33. doi: 10.1364/AO.50.000120.
Observations of the Moon provide a primary technique for the on-orbit cross calibration of Earth remote sensing instruments. Monthly lunar observations are major components of the on-orbit calibration strategies of SeaWiFS and MODIS. SeaWiFS has collected more than 132 low phase angle and 59 high phase angle lunar observations over 12 years, Terra MODIS has collected more than 82 scheduled and 297 unscheduled lunar observations over nine years, and Aqua MODIS has collected more than 61 scheduled and 171 unscheduled lunar observations over seven years. The NASA Ocean Biology Processing Group Calibration and Validation Team and the NASA MODIS Characterization Support Team use the USGS RObotic Lunar Observatory (ROLO) photometric model of the Moon to compare these time series of lunar observations over time and varying observing geometries. The cross-calibration results show that Terra MODIS and Aqua MODIS agree, band to band, at the 1%-3% level, while SeaWiFS and either MODIS instrument agree at the 3%-8% level. The combined uncertainties of these comparisons are 1.3% for Terra and Aqua MODIS, 1.4% for SeaWiFS and Terra MODIS, and 1.3% for SeaWiFS and Aqua MODIS. Any residual phase dependence in the ROLO model, based on these observations, is less than 1.7% over the phase angle range of -80° to -6° and +5° to +82°. The lunar cross calibration of SeaWiFS, Terra MODIS, and Aqua MODIS is consistent with the vicarious calibration of ocean color products for these instruments, with the vicarious gains mitigating the calibration biases for the ocean color bands.
对月球的观测为地球遥感仪器的在轨交叉校准提供了一种主要技术。每月的月球观测是SeaWiFS和MODIS在轨校准策略的主要组成部分。在12年里,SeaWiFS收集了超过132次低相位角和59次高相位角的月球观测数据;在9年里,Terra MODIS收集了超过82次预定和297次非预定的月球观测数据;在7年里,Aqua MODIS收集了超过61次预定和171次非预定的月球观测数据。美国国家航空航天局海洋生物学处理组校准与验证团队以及美国国家航空航天局MODIS特性支持团队使用美国地质调查局的月球机器人天文台(ROLO)月球光度模型,来比较这些随时间变化且观测几何条件各异的月球观测时间序列。交叉校准结果表明,Terra MODIS和Aqua MODIS在各波段之间的一致性达到1%-3%,而SeaWiFS与任何一台MODIS仪器之间的一致性为3%-8%。这些比较的综合不确定性,Terra和Aqua MODIS为1.3%,SeaWiFS和Terra MODIS为1.4%,SeaWiFS和Aqua MODIS为1.3%。基于这些观测,在-80°至-6°以及+5°至+82°的相位角范围内,ROLO模型中任何残留的相位依赖性均小于1.7%。SeaWiFS、Terra MODIS和Aqua MODIS的月球交叉校准与这些仪器海洋颜色产品的替代校准一致,替代增益减轻了海洋颜色波段的校准偏差。