首页> 外文会议>Geoscience and Remote Sensing Symposium, 2002. IGARSS '02. 2002 IEEE International >Derivation and comparison of bi-directional reflectance functions of first-year and multi-year sea ice types in the Southern Ocean
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Derivation and comparison of bi-directional reflectance functions of first-year and multi-year sea ice types in the Southern Ocean

机译:南大洋第一年和多年海冰类型双向反射函数的推导和比较

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Surface spectral bi-directional reflectance function (BRF) is a fundamental surface property in radiation interaction with the atmosphere-Earth surface system. Knowledge of surface BRFs is also crucial to estimating surface albedo from remote sensing data sets. During two austral summer cruises in 1999 and 2000, surface spectral directional reflectance patterns of first-year (FY) and multi-year (MY) sea ice were measured under clear skies for 512 spectral channels between 350-1050 nm. After smoothing raw data, calibrating spectral albedo of the reference panel, and removing the impact of sky diffuse radiation, representative patterns of BRF of FY and MY sea ice types in the Southern Ocean have been produced. The solar incidence angles (50 to 65 degrees) associated with the derived patterns are moderate. Some common features are seen in the BRF patterns of both FY and MY sea ice types. A moderately strong peak occurs in the principal plane when the sensor is looking into the azimuth from which the solar illumination comes. When the sensor is viewing towards the azimuth perpendicular to the principal plane, the BRF values are close to the surface albedo. However, the FY ice exhibits stronger surface anisotropy than the MY ice because the former has a smoother surface than the latter. The BRF pattern of the FY ice has a minimum in the backward direction. From the backward minimum towards the forward peak, BRF values of the FY sea ice show a monotonous increase along almost all great circle scans in the hemisphere. On the contrary, the MY ice looks similar to an isotropic (or Lambertian) surface when it is viewed from almost all directions except for the forward viewing azimuth with large viewing zenith angles (60-80 degrees). Besides, there is a discernible secondary peak in the backward direction of the MY ice BRF, presumably caused by reflectance from the fore-slopes of surface undulation. The resulting patterns will be especially useful in deriving surface albedo from NASA moderate resolution imaging spectrometer (MODIS).
机译:表面光谱双向反射率函数(BRF)是辐射与大气-地球表面系统相互作用时的基本表面属性。地表BRF的知识对于从遥感数据集中估算地表反照率也至关重要。在1999年和2000年的两次夏季夏季南方巡游中,在晴朗的天空下测量了350-1050 nm之间的512个光谱通道的一年(FY)和多年(MY)海冰的表面光谱方向反射率模式。在对原始数据进行平滑处理,校准参考面板的光谱反照率并消除天空漫射辐射的影响之后,就产生了南大洋的FY和MY海冰类型的BRF的代表性模式。与派生图案相关的太阳入射角(50至65度)适中。在FY和MY海冰类型的BRF模式中可以看到一些共同的特征。当传感器注视着太阳光照的方位角时,在主平面中会出现一个中等强度的峰值。当传感器朝向垂直于主平面的方位角观察时,BRF值接近表面反照率。但是,FY冰比MY冰表现出更强的表面各向异性,因为前者的表面比后者更光滑。 FY冰的BRF模式在向后方向上具有最小值。从向后的最小值到向前的峰值,FY海冰的BRF值在半球的几乎所有大圈扫描中都显示出单调增加。相反,从几乎所有方向观看时,MY冰看起来都与各向同性(或Lambertian)表面相似,除了具有较大观看天顶角(60-80度)的前视方位角。此外,在MY ice BRF的反向方向上有一个可辨别的次级峰,可能是由于表面起伏前斜坡的反射所引起的。所得的图案在从NASA中分辨率成像光谱仪(MODIS)推导表面反照率中特别有用。

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