Comparison of lunar irradiance models and validation of lunar observation on Earth

Lu ZHANG; Peng ZHANG; Xiuqing HU; Lin CHEN; Yang WANG; Wei WANG

doi:10.11834/jrs.20176342

Technology and Methodology | Views : 0 下载量: 1436 CSCD: 16

PDF
Export
Share
Collection
Album

Comparison of lunar irradiance models and validation of lunar observation on Earth
Vol. 21, Issue 6, Pages: 864-870(2017)
Received：23 September 2016，

Accepted：09 June 2017，

Published：15 September 2017
DOI： 10.11834/jrs.20176342
稿件说明：

移动端阅览

张璐, 张鹏, 胡秀清, 陈林, 王阳, 王威. 2017. 月球辐射照度模型比对及地基对月观测验证. 遥感学报, 21(6): 864–870 DOI： 10.11834/jrs.20176342.

Zhang L, Zhang P, Hu X Q, Chen L, Wang Y and Wang W. 2017. Comparison of lunar irradiance models and validation of lunar observation on Earth. Journal of Remote Sensing, 21(6): 864–870 DOI： 10.11834/jrs.20176342.

摘要

月球是除太阳外对地张角最大的天体，反射率稳定性为10

–8

每年，适合用于遥感卫星的辐射定标、夜间地基大气遥感和夜间卫星遥感，但月球辐射照度模型的精度束缚了上述应用的发展。为检验现有ROLO(RObotic Lunar Observatory)和MT2009(Miller-Turner 2009)地基整盘月球辐射照度模型的精度，国家卫星气象中心于2015年底至2016年初在云南丽江组织了3个月的地基对月观测，使用高光谱月球成像光谱仪获取了399.00—1060.00 nm连续光谱的月球辐射照度。基于整盘月球辐射照度模型，利用丽江地基对月观测试验资料，对比模型与模型、模型与丽江地基观测月球辐射照度。结果表明：(1)MT2009与ROLO模型在短波红外谱段的差异明显大于可见光谱段；(2)地基观测高光谱月球辐射照度结果与ROLO模型更接近，但是可见光波段比ROLO模型辐射照度平均小5.86%左右。为探究差异产生的主要来源，对结果还进行了进一步的分析和讨论，以期为今后月球辐射模型的改进和夜间微光遥感研究提供经验和依据。

Abstract

Lunar is the second largest field-of-angle object near the Earth

and its reflectance can be considered stable to 10

–8

per year. Thus

lunar is selected as the radiometric standard for the calibration of Earth-orbiting satellite-borne instruments and as the radiance source at night similar to solar at daytime for ground-based and satellite remote sensing. However

the precision of existing lunar irradiance models is insufficient to satisfy application requirements. To improve lunar irradiance models and verify the accuracy of the models

a three-month Earth-based observation of lunar was conducted on December 2015 by the National Satellite Meteorological Center

China Meteorological Administration. The hyper-spectral irradiance of lunar ranging from 399 nm to 1060 nm was retrieved by an imaging spectrometer in Lijiang

Yunnan. This study compared Earth-based lunar observations and other models (ROLO and MT2009 models). Results show that the observations are more similar to the ROLO model than to the MT2009 model

and the difference between the two models is larger in the shortwave infrared region than in the visible region. The average relative difference between the ROLO model and ground-based observations is approximately 5.86%. Causes of this difference are discussed in this study

which provides a theoretical foundation for establishing an accurate model of lunar irradiance.

关键词

Keywords

references

Acton C H Jr. 1996. Ancillary data services of NASA’s navigation and ancillary information facility. Planetary and Space Science, 44(1): 65–70

Barreto A, Cuevas E, Damiri B, Guirado C, Berkoff T, Berjón A J, Hernández Y, Almansa F and Gil M. 2013. A new method for nocturnal aerosol measurements with a lunar photometer prototype. Atmospheric Measurement Techniques, 6(3): 585–598

Eliason E M, McEwen A S, Robinson M S, Lee E M, Becker T L, Gaddis L, Weller L A, Isbell C E, Shinaman J R, Duxbury T and Malaret E. 1999. Clementine: a global multi-spectral map of the moon from the clementine UVVIS imaging instrument. Lunar and Planetary Science Conference, 30: 1933–1934

Green P D and Lobb D. 2015. The traceable radiometry underpinning terrestrial and helio studies (truths) mission//Proceedings of SPIE 9639, Sensors, Systems, and Next-Generation Satellites XIX. Toulouse: SPIE: 96391C [DOI: 10.1117/12.2192593]

Hapke B. 2012. Theory of Reflectance and Emittance Spectroscopy. 2nd ed. New York: Cambridge University Press

Kieffer H H, Anderson J M. 1998. Use of the moon for spacecraft calibration over 350 to 2500 nm. 325–336 [DOI: 10.1117/12.333646]

Kieffer H H and Wildey R L. 1985. Absolute calibration of landsat instruments using the moon. Photogrammetric Engineering and Remote Sensing, 51(9): 1391–1393

Kieffer H H. 1997. Photometric stability of the lunar surface. Icarus, 130(2): 323–327

Kieffer H H and Stone T C. 2005. The spectral irradiance of the moon. The Astronomical Journal, 129(6): 2887

Lane A P and Irvine W M. 1973. Monochromatic phase curves and albedos for the lunar disk. Astronomical Journal, 78: 267

Lawrence S J, Lau E, Steutel D, Stopar J D, Wilcox B B and Lucey P G. 2003. A new measurement of the absolute spectral reflectance of the moon//34th Lunar and Planetary Science Conference. League City, Texas: LPI

Leckey J. 2015. Climate absolute radiance and refractivity observatory (CLARREO). International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, XL-7/W3: 213–217 [DOI: 10.5194/isprsarchives-XL-7-W3-213-2015]

Miller S D and Turner R E. 2009. A dynamic lunar spectral irradiance data set for npoess/viirs day/night band nighttime environmental applications. IEEE Transactions on Geoscience and Remote Sensing, 47(7): 2316–2329

Pieters C M, Boardman J, Buratti B, Chatterjee A, Clark R, Glavich T, Green R, Head J, Isaacson P, Malaret E, McCord T, Mustard J, Petro N, Runyon C, Staid M, Sunshine J, Taylor L, Tompkins S, Varanasi P and White M. 2009. The moon mineralogy mapper (M 3 ) on chandrayaan-1. Current Science, 96(4): 500–505

Saiki K, Saito K, Okuno H, Suzuki A, Yamanoi Y, Hirata N and Nakamura R. 2008. Estimation of the lunar reflectance by ground-based observation using a tunable liquid-crystal filter telescope. Earth, Planets and Space, 60: BF03352806 [DOI: 10.1186/BF03352806]

Shaw J A. 1999. Modeling infrared lunar radiance. Optical Engineering, 38(10): 1763–1764

Velikodsky Y I, Opanasenko N V, Akimov L A, Korokhin V V, Shkuratov Y G, Kaydash V G, Videen G, Ehgamberdiev S A and Berdalieva N E. 2011. New earth-based absolute photometry of the moon. Icarus, 214(1): 30–45

吴荣华, 张鹏, 杨忠东, 胡秀清, 丁雷, 陈林. 2016. 基于月球反射的遥感器定标跟踪监测. 遥感学报, 20(2): 278–289

Wu R H, Zhang P, Yang Z D, Hu X Q, Ding L and Chen L. 2016. Monitor radiance calibration of the remote sensing instrument with reflected lunar irradiance. Journal of Remote Sensing, 20(2): 278–289 (

Wu Y Z, Besse S, Li J Y, Combe J P, Wang Z C, Zhou X F and Wang C. 2013. Photometric correction and in-flight calibration of chang’E-1 interference imaging spectrometer (IIM) data. Icarus, 222(1): 283–295

Yokota Y, Matsunaga T, Ohtake M, Haruyama J, Nakamura R, Yamamoto S, Ogawa Y, Morota T, Honda C, Saiki K, Nagasawa K, Kitazato K, Sasaki S, Iwasaki A, Demura H, Hirata N, Hiroi T, Honda R, Iijima Y and Mizutani H. 2011. Lunar photometric properties at wavelengths 0.5—1.6 μm acquired by SELENE spectral profiler and their dependency on local albedo and latitudinal zones. Icarus, 215(2): 639–660

Younkin R L. 1970. Optical reflectance of local areas of the moon. Astronomical Journal, 75: 831

Alert me when the article has been cited

提交

Radiometric calibration and cross calibration of HJ-2 06 satellite based on point targets

Radiometric calibration method for deep convective clouds in the reflective bands of FY-4A/AGRI

Construction of directional reflectance reference model for desert stable earth targets

On-orbit radiometric calibration and Validation of GF-7 satellite based on RadCalNet Baotou site

The near-space altitude experiment for satellite radiometric calibration and the first results