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DOI10.1117/12.2223912
On-orbit Performance and Calibration Improvements for the Reflective Solar Bands of Terra and Aqua MODIS
Angal, Amit1; Xiong, Xiaoxiong (Jack)2; Wu, Aisheng1; Chen, Hongda1; Geng, Xu1; Link, Daniel1; Li, Yonghong1; Wald, Andrew3; Brinkmann, Jake1
通讯作者Angal, Amit
会议名称Conference on Earth Observing Missions and Sensors - Development, Implementation, and Characterization IV
会议日期APR 04-07, 2016
会议地点New Delhi, INDIA
英文摘要

Moderate Resolution Imaging Spectroradiometer (MODIS) is the keystone instrument for NASA's EOS Terra and Aqua missions, designed to extend and improve heritage sensor measurements and data records of the land, oceans and atmosphere. The reflective solar bands (RSB) of MODIS covering wavelengths from 0.41 mu m to 2.2 mu m, are calibrated on-orbit using a solar diffuser (SD), with its on-orbit bi-directional reflectance factor (BRF) changes tracked using a solar diffuser stability monitor (SDSM). MODIS is a scanning radiometer using a two-sided paddle-wheel mirror to collect earth view (EV) data over a range of +/- 55 degrees off instrument nadir. In addition to the solar calibration provided by the SD and SDSM system, lunar observations at nearly constant phase angles are regularly scheduled to monitor the RSB calibration stability. For both Terra and Aqua MODIS, the SD and lunar observations are used together to track the on-orbit changes of RSB response versus scan angle (RVS) as the SD and SV port are viewed at different angles of incidence (AOI) on the scan mirror. The MODIS Level 1B (L1B) Collection 6 (C6) algorithm incorporated several enhancements over its predecessor Collection 5 (C5) algorithm. A notable improvement was the use of the earth-view (EV) response trends from pseudo-invariant desert targets to characterize the on-orbit RVS for select RSB (Terra bands 1-4, 8, 9 and Aqua bands 8, 9) and the time, AOI, and wavelength-dependent uncertainty. The MODIS Characterization Support Team (MCST) has been maintaining and enhancing the C6 algorithm since its first update in November, 2011 for Aqua MODIS, and February, 2012 for Terra MODIS. Several calibration improvements have been incorporated that include extending the EV-based RVS approach to other RSB, additional correction for SD degradation at SWIR wavelengths, and alternative approaches for on-orbit RVS characterization. In addition to the on-orbit performance of the MODIS RSB, this paper also discusses in detail the recent calibration improvements implemented in the MODIS L1B C6.


来源出版物EARTH OBSERVING MISSIONS AND SENSORS: DEVELOPMENT, IMPLEMENTATION, AND CHARACTERIZATION IV
ISSN0277-786X
EISSN1996-756X
出版年2016
卷号9881
EISBN978-1-5106-0122-2
出版者SPIE-INT SOC OPTICAL ENGINEERING
类型Proceedings Paper
语种英语
国家USA
收录类别CPCI-S
WOS记录号WOS:000385792900030
WOS关键词TIME-DEPENDENT RESPONSE ; SCAN-ANGLE
WOS类目Engineering, Electrical & Electronic ; Remote Sensing ; Optics ; Imaging Science & Photographic Technology
WOS研究方向Engineering ; Remote Sensing ; Optics ; Imaging Science & Photographic Technology
资源类型会议论文
条目标识符http://119.78.100.177/qdio/handle/2XILL650/305615
作者单位1.Sci Syst & Applicat Inc, 10210 Greenbelt Rd, Lanham, MD 20706 USA;
2.NASA GSFC, Sci & Explorat Directorate, Greenbelt, MD 20771 USA;
3.Global Sci & Technol Inc, 7855 Walker Dr,Suite 200, Greenbelt, MD 20770 USA
推荐引用方式
GB/T 7714
Angal, Amit,Xiong, Xiaoxiong ,Wu, Aisheng,et al. On-orbit Performance and Calibration Improvements for the Reflective Solar Bands of Terra and Aqua MODIS[C]:SPIE-INT SOC OPTICAL ENGINEERING,2016.
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