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A direct method for estimating net surface shortwave radiation from MODIS data

机译:根据MODIS数据估算净表面短波辐射的直接方法

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The Net Surface Shortwave Radiation (NSSR) is of primary interest in climate research because it controls the total energy exchange between the atmosphere and the land/ocean surface. The conventional methods for estimating NSSR rely on broadband satellite data such as Earth Radiation Budget Experiment (ERBE) wide-field-of-view planetary albedo. The spatial resolution of the current ERBE satellite data having nadir footprints larger than 30 kin is too coarse. The primary objective of this study is to estimate NSSR using multispectral narrowband data such as Moderate Resolution Imaging Spectroradiometer (MODIS) data. A direct method was developed for narrowband-to-broadband albedo conversion, which links the narrowband apparent reflectance at the Top Of Atmosphere (TOA) to shortwave broadband albedo for clear and cloudy skies without performing any surface angular modeling. The conversion coefficients were derived as functions of the secant Viewing Zenith Angle (VZA) for a given Solar Zenith Angle (SZA) and a given interval of Relative Azimuth angle (RAA). The result of comparing the values of estimated MODIS TOA shortwave broadband albedos with those of the Clouds and the Earth's Radiant Energy System (CERES) data indicated that this direct method could predict TOA shortwave broadband albedo accurately with Root Mean Square (RMS) error between CERES observations and the estimated instantaneous MODIS TOA albedos less than 0.02. Based on more accurate radiative transfer model MODTRAN 4, the parameterization coefficients of Masuda et al. for the estimation of the NSSR from TOA broadband albedo were recalculated. The result showed that the coefficients should be categorized by land surfaces, ocean surface and snow/ice surface, respectively. Finally, the NSSR estimated from MODIS data was compared with the measurements of meteorological data for an extended period of time covering all seasons in a year 2003. The RMS error is less than 20 Win 2 for clear skies and 35 Win 2 for cloudy skies. (c) 2006 Elsevier Inc. All rights reserved.
机译:净表面短波辐射(NSSR)是气候研究的主要兴趣,因为它控制着大气层与陆地/海洋表面之间的总能量交换。估算NSSR的常规方法依赖于宽带卫星数据,例如地球辐射预算实验(ERBE)宽视场行星反照率。天底足迹大于30 kin的当前ERBE卫星数据的空间分辨率太粗糙。这项研究的主要目的是使用多光谱窄带数据(例如中分辨率成像光谱仪(MODIS)数据)估算NSSR。开发了一种直接方法,用于窄带到宽带的反照率转换,该方法将大气顶部(TOA)的窄带视在反射率与短波宽带反照率相关联,以实现晴朗和多云的天空,而无需执行任何表面角度建模。对于给定的太阳天顶角(SZA)和给定的相对方位角间隔(RAA),可以得出割线视顶角(VZA)的函数的转换系数。将MODIS TOA短波宽带反照率的估计值与云和地球辐射能系统(CERES)的值进行比较的结果表明,这种直接方法可以准确预测TOA短波宽带反照率,且CERES之间的均方根(RMS)误差观测值和估计的MODIS TOA瞬时反照率小于0.02。基于更精确的辐射传输模型MODTRAN 4,Masuda等人的参数化系数为。为了重新估算来自TOA宽带反照率的NSSR。结果表明,系数应分别按陆地表面,海洋表面和雪/冰表面分类。最后,将MODIS数据估算的NSSR与2003年一年中所有季节的气象数据的测量结果进行比较。对于晴朗的天空,RMS误差小于20 Win 2,对于多云的天空,RMS误差小于35 Win 2。 (c)2006 Elsevier Inc.保留所有权利。

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