Solar radiation transfer in the surface snow layer in Dronning Maud Land, Antarctica

被引:18
作者
Jarvinen, Onni [1 ]
Lepparanta, Matti [1 ]
机构
[1] Univ Helsinki, Dept Phys, FIN-00014 Helsinki, Finland
基金
芬兰科学院;
关键词
Transmittance; Extinction coefficient; Solar radiation; Antarctica; Snow physics; OPTICAL-PROPERTIES; ARCTIC SNOW; ICE; TRANSMISSION; COVER; TRANSMITTANCE; ACCUMULATION; ATTENUATION; EMISSIONS; PROFILES;
D O I
10.1016/j.polar.2013.03.002
中图分类号
Q14 [生态学(生物生态学)];
学科分类号
071012 ; 0713 ;
摘要
Spectroradiometer measurements of solar radiation (the broadest band used 400-900 nm) were performed above and inside the surface snow layer in western Dronning Maud Land, Antarctica, during the austral summer of 2009-2010. The vertical distributions of transmittance and the extinction coefficient were examined from the surface to a depth of 30 cm. Physical characterization of the snowpack included measurements of thickness, density, hardness (hand test), liquid-water content, and grain size and shape (from photographs of grains). The transmittance was <1% in the upper 20 cm and <27% in the upper 10 cm. The mean spectral diffuse extinction coefficient varied between 0.04 and 0.31 cm(-1) (10-20-cm layer). Using the spectral extinction coefficients of the 0-10-cm and 10-20-cm layers, the depth, where broadband (400-700-nm band) irradiance was 1% of the downwelling irradiance at the surface, was 50 cm. The density of the snow in the upper part of the snowpack (depth of 0-55 cm) varied from 300 to 440 kg m(-3). The predominant grain type was large rounded particles (RGIr) and the predominant grain size was 1 mm. (C) 2013 Elsevier B.V. and NIPR. All rights reserved.
引用
收藏
页码:1 / 17
页数:17
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