Approximations of phase function in calculating the spectral albedo of snow surface with multiple scattering.

Q4 Earth and Planetary Sciences
T. Aoki, T. Aoki, M. Fukabori
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引用次数: 3

Abstract

Four types of approximations of the Mie phase function were studied in calculating multiple scattering by snow particles with the doubling method. These involve the two renormalizations of Hansen and Grant, the delta-M method and direct truncation. These four approximations were compared for snow surface albedo with effective grain radii of 50, 200 and 1000μm in a wavelength region from 0.3 to 3.0μm with the delta-Eddington approximation as a reference. In the Hansen's renormalization, the maximum albedo error exceeds 0.1 for snow with an effective radius of 1000μm at small solar zenith angles. The delta-M method overestimates snow albedos at all solar zenith angles in a wavelength region smaller than 1.4μm for snow with effective radius of 1000μm. This is due to insufficient angle resolution (0.1° in a scattering angle region less than 2°) in the forward peak region of the look-up table of the Mie phase function. It has been shown that even with ten times higher resolution in the scattering angle region less than 10° a sufficient accuracy could not be obtained for an effective radius of 1000μm in a wavelength region smaller than 0.6μm. Reasonable results were obtained by the Grant's renormalization and direct truncation approximation for all cases of effective grain radii studied. It was also found that these methods save computation time and memory because sufficient accuracy is obtained even with a low angle resolution of 0.1° in the forward peak region of phase function. In direct truncation, the result was not sensitive to the choice of a truncation angle between 5° and 20°.
多次散射下雪面光谱反照率计算中的相函数近似。
研究了四种近似的Mie相函数,并用加倍法计算雪粒子的多次散射。这包括Hansen和Grant的两种重整化,delta-M方法和直接截断。以delta-Eddington近似为参考,对0.3 ~ 3.0μm波长范围内有效颗粒半径为50、200和1000μm的积雪表面反照率进行了比较。在Hansen’s重整化中,在太阳天顶角较小时,有效半径为1000μm的雪的最大反照率误差超过0.1。对于有效半径为1000μm的积雪,delta-M方法高估了波长小于1.4μm区域内所有太阳天顶角的积雪反照率。这是由于Mie相函数查找表的前峰区域的角度分辨率不足(在散射角小于2°的区域为0.1°)。结果表明,在小于10°的散射角范围内,即使提高10倍的分辨率,在小于0.6μm的波长范围内,有效半径为1000μm时,也无法获得足够的精度。采用格兰特重整化和直接截断近似法对所有有效晶粒半径进行了研究,得到了合理的结果。这些方法在相位函数前峰区角分辨率为0.1°的情况下也能获得足够的精度,节省了计算时间和存储空间。在直接截断时,截断角在5°~ 20°之间的选择对结果不敏感。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Papers in Meteorology and Geophysics
Papers in Meteorology and Geophysics Earth and Planetary Sciences-Geophysics
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