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The ablation zone in northeast Greenland: ice types, albedos and impurities

机译:格陵兰东北部的消融区:冰类型,反照率和杂质

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Ice types, albedos and impurity content are characterized for the ablation zone of the Greenland ice sheet in Kronprinz Christians Land (80° N, 24° W). Along this ice margin the width of the ablation zone is only about 8 km. The emergence and melting of old ice in the ablation zone creates a surface layer of dust that was originally deposited with snowfall high on the ice sheet. This debris cover is augmented by locally derived wind-blown sediment. Subsequently, the surface dust particles often aggregate together to form centimetre-scale clumps that melt into the ice, creating cryoconite holes. The debris in the cryoconite holes becomes hidden from sunlight, raising the area-averaged albedo relative to surfaces with uniform debris cover. Spectral and broadband albedos were obtained for snow, ice hummocks, debris-covered ice, cryoconite-studded ice and barren tundra surfaces. Broadband ice albedos varied from 0.2 (for ice with heavy loading of uniform debris) to 0.6 (for ice hummocks with cryoconite holes). The cryoconite material itself has albedo 0.1 when wet. Areal distribution of the major surface types was estimated visually from a transect video as a function of distance from the ice edge (330 m a.s.l.). Ablation rates were measured along a transect from the ice margin to the slush zone 8 km from the margin (550 m a.s.I.), traversing both Pleistocene and Holocene ice. Ablation rates in early August averaged 2 cmd~(-1) . I mpurity concentrations were typically 4.3 mg L~(-1)in the subsurface ice. Surface concentrations were about 16 g m~(-2) on surfaces with low impurity loading, and heavily loaded surfaces had concentrations as high as 1.4 kg m~(-2) . The mineralogical composition of the cryoconite material is comparable with that of the surrounding soils and with dust on a snowdrift in front of the ice margin, implying that much of the material is derived from local sources. A fine mode (clay) is present in the oldest ice but not in the nearby soil, suggesting that its origin is from wind deposition during Pleistocene glaciation.
机译:克朗普林茨基督徒土地(80°N,24°W)中格陵兰冰盖消融区的冰类型,反照率和杂质含量被表征。沿着该冰缘,消融区的宽度仅约8 km。消融区中旧冰的出现和融化会形成一层表面尘埃,该尘埃最初是由降雪沉积在冰原上形成的。杂物覆盖物因局部风吹沉积物而增加。随后,表面的尘埃颗粒经常聚集在一起,形成厘米级的团块,这些团块融化到冰中,形成冰晶孔。冷冻圆锥孔中的碎屑对日光变得不可见,相对于碎屑覆盖均匀的表面,面积反照率升高。获得了光谱,宽带反照率的雪,冰山丘,覆盖有碎屑的冰,冰晶石散布的冰和荒芜的苔原表面。宽带冰反照率从0.2(对于带有大量均匀碎片的冰)到0.6(对于具有超低温洞的冰山丘)不等。低温时,冰晶岩材料本身的反照率为0.1。根据与冰边缘距离(330 m a.s.l.)的函数,从横断面视频直观地估算出主要表面类型的地域分布。沿从冰缘到距缘8 km(550 m a.s.I.)的横越新世和全新世冰的冰冻带的断面测量消融率。八月初的消融率平均为2 cmd〜(-1)。地下冰中的杂质浓度通常为4.3 mg L〜(-1)。在低杂质负载的表面上,表面浓度约为16 g m〜(-2),在重负载的表面上,浓度高达1.4 kg m〜(-2)。冻土材料的矿物学组成与周围土壤的矿物学组成相当,并且在冰缘前的雪堆上有灰尘,这意味着大部分材料都来自当地。精细模式(粘土)存在于最古老的冰中,但附近的土壤中不存在,这表明其起源来自更新世冰川期的风积。

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