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Hemispherical-Directional Reflectance (HDRF) of Windblown Snow-Covered Arctic Tundra at Large Solar Zenith Angles

机译:大太阳天顶角下被风吹雪覆盖的北极苔原的半球方向反射率(HDRF)

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摘要

Ground-based measurements of the hemispherical- directional reflectance factor (HDRF) of windblown snow- covered Arctic tundra were measured at large solar zenith angles (79°–85°) for six sites near the international research base in Ny-Ålesund, Svalbard. Measurements were made with the Gonio RAdiometric Spectrometer System over the viewing angles 0°–50° and the azimuth angles 0°–360° , for the wavelength range 400–1700 nm. The HDRF measurements showed good consistency between sites for near-nadir and backward viewing angles, with a relative standard deviation of less than 10% between sites where the snowpack was smooth and the snow depth was greater than 40 cm. The averaged HDRF showed good symmetry with respect to the solar principal plane and exhibited a forward scattering peak that was strongly wavelength dependent, with greater than a factor of 2 increase in the ratio of maximum to minimum HDRF values for all viewing angles over the wavelength range 400– 1300 nm. The angular effects on the HDRF had minimal influence for viewing angles less than 15° in the backward viewing direction for the averaged sites and agreed well with another study of snow HDRF for infrared wavelengths, but showed differences of up to 0.24 in the HDRF for visible wavelengths owing to light-absorbing impurities measured in the snowpack. The site that had the largest roughness elements showed the strongest anisotropy in the HDRF, a large reduction in forward scattering, and a strong asymmetry with respect to the solar principal plane.
机译:在斯瓦尔巴特群岛Ny-Ålesund国际研究基地附近的六个地点,在大太阳天顶角(79°-85°)上测量了被风吹雪的北极苔原的半球方向反射率(HDRF)的地面测量。使用Gonio RAdiometric光谱仪系统在400°至1700 nm波长范围内的视角0°–50°和方位角0°–360°范围内进行了测量。 HDRF测量结果显示,在接近最低点和向后视角的站点之间具有良好的一致性,在雪堆光滑且雪深大于40 cm的站点之间的相对标准偏差小于10%。平均HDRF相对于太阳主平面显示出良好的对称性,并显示出与波长密切相关的前向散射峰,在整个波长范围内,所有视角的最大HDRF值与最小HDRF值之比增加2倍以上400-1300 nm。对于HDRF的角度影响,对于平均位置的向后视角小于15°的视角影响最小,并且与雪HDRF的红外波长的另一项研究吻合得很好,但显示可见光的HDRF差异最大为0.24波长是由于在积雪堆中测量的吸光杂质引起的。具有最大粗糙度元素的位置在HDRF中显示出最强的各向异性,正向散射的大幅减少以及相对于太阳主平面的强烈不对称性。

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