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981.
982.
在中国科学院大气物理研究所的三维全弹性对流风暴云催化数值模式(简称为IAP-CSM3D)的基础上,对模式中催化部分的参数化方案进行了改进,推导出人工冰晶与其它粒子之间相互作用的微物理过程的参数化方程。改进后的模式将催化产生的人工冰晶单独作为预报量进行处理,把人工冰晶与自然冰晶区分开,且考虑的人工冰晶谱型为双参数粒子谱,使模式更符合实际。利用改进后的模式模拟了2005年7月8日发生在辽宁省朝阳市的一次冰雹云天气过程,着重分析了催化云人工冰晶的微物理过程、空间分布和谱型,以及对冰相降水粒子的贡献。数值试验表明,自然雹云模拟结果与观测事实相吻合,说明改进后的模式对冰雹云具有较可靠的模拟能力。模拟分析表明,冻滴是该例自然雹云冰雹胚胎的主要来源,对该冰雹云进行AgI催化可明显地减少降雹量,特别是在云中冰雹形成初期进行催化防雹效果最好,既可产生最大的防雹作业效果又不至于过度减少降雨量。催化减雹的主要原因是催化显著地减少了云中冻滴向冰雹胚胎的转化总量。进一步研究发现,人工冰晶在云的不同阶段对各种冰相降水粒子的贡献是不同的。人工冰晶对雪花总质量的贡献较小,对霰总质量的贡献有所增大,而对冻滴总质量的贡献较大。模拟的冰晶粒子谱可较好地反映出人工冰晶谱型较窄,浓度较大,尺度较小的特征。  相似文献   
983.
Fabric and crystal characteristics of Bohai and Arctic sea ice   总被引:1,自引:0,他引:1  
1 IntroductionBohaione yeariceandAntarcticonehavethesimilarsurface featuresandcorre spondingfabricandcrystalcharacteristics (Allison 1 997;Lietal.1 997;Qin 1 991 ) .DuringtheChinaFirstArcticExpedition ,theresultsinthestudyofone yearicefromBohaiandAntarcticwereusedfo…  相似文献   
984.
Ice core records provide the most direct, detailedand complete measure of past climate change[1,2]. Gla-ciochemical records have been used to investigate thechanges in atmospheric circulation patterns overGreenland Ice Sheet and West Antarctic[3—6]. Mostrecently, major ion series developed from new suban-nual scale sampling of GISP2 ice core from centralGreenland are calibrated with instrumental series ofsea level pressure (SLP) provide proxy records of ma-jor marine (Icelandic Low) and…  相似文献   
985.
Models of glacio‐hydroisostatic sea‐level change have been published for the British Isles that are broadly consistent with the observational evidence, as well as with glaciological constraints. It has been argued, however, that the models fail to represent sea‐level change along the Irish Sea margins and in southern Ireland for the post‐deglaciation period. The argument rests on the interpretation of the depositional environment of the elevated ‘Irish Sea Drift’ on both sides of the Irish Sea: whether this is terrestrial or glaciomarine. The isostatic models for the British Isles are consistent with the former interpretation in that sea‐levels on either side of the Irish Sea, south of about the Isle of Man, are not predicted to have risen above present sea‐level at any time since the deglaciation of the Irish Sea. This implies that ice over both the Irish Sea and Ireland was relatively thin (ca. 600–700 m over Ireland). If the glaciomarine interpretation of the elevated Irish Sea Drift is correct, then the maximum ice thickness over central and southern Ireland would have to reach 2000 m, exceeding that over Scotland. Furthermore, for the resulting sea‐level change to be consistent with the Holocene evidence, this thick ice sheet could not have extended to the eastern side of the Irish Sea. Nor could it have been very thick at its northern and western limits. If such an ice model is extreme and incompatible with glaciological observations then the alternative is to accept the interpretation of the Irish Sea Drift as terrestrial in origin. Copyright © 2001 John Wiley & Sons, Ltd.  相似文献   
986.
Infrared observations of comets C/1996 B2 (Hyakutake) and C/1995 O1 (Hale-Bopp) benefited from the high spectral resolution and sensitivity of échelle spectrometers now equipping ground-based telescopes and from the availability of the Infrared Space Observatory (ISO). From the ground, several hydrocarbons were unambiguously detected for the first time: CH4, C2H2, C2H6. Water was observed through several of its hot vibrational bands, escaping telluric absorption. CO, HCN, NH3 and OCS were also observed, as well as several radicals. This permitted the evaluation of molecular production rates, of rotational temperature, and — taking advantage of the 1-D imaging of long-slit spectroscopy — of the space distribution of these species. With ISO, carbon dioxide was directly observed for the second time in a comet (after its detection from the Vega probes in P/Halley). The spectrum of water was investigated in detail (several bands of vibration and far-infrared rotational lines), permitting the evaluation of the rotational temperature of water, and of it spin temperature from the ortho-to-para ratio. Water ice was identified in the grains of Hale-Bopp as far as 7 AU from the ground and possibly at 3 AU with ISO. The composition of cometary volatiles appears to be strikingly similar to that of interstellar ices. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   
987.
There are very strong thermal gradients between the Antarctic continent and the sea-ice zone, and between that zone and the ocean to the north. As a result of these contrasts the sea-ice domain is one of strong cyclogenesis and high cyclone frequency. In this study we explore many aspects of that cyclonic behaviour and investigate the manner in which these systems influence, and are influenced by, the sea ice. Using the NCEP-DOE re-analyses (1979–2002) we have determined variables that are proportional to the mean of the wind stress and the mean rate at which mechanical energy is imparted to the surface. Using two decompositions of the wind field we have obtained estimates of how much of these fluxes are contributed to by the transient eddies. We find these to be significant over the sea ice and the ocean to the north, particularly when a new decomposition is used. The presence of frequent and vigorous cyclones is a central factor that determines the positive mean freshwater flux over the sea-ice zone in all seasons. This transfer to the ocean is smallest in summer (0.49 mm day−1) and assumes a maximum of 1.27 mm day−1 in winter.  相似文献   
988.
Factors controlling the magnitudes of, and short-term variations in, the potential temperatures of the snow surface and the air at the height of 2 m θS and θ2 m over Arctic sea ice in winter are analysed. The study addresses the winters of 1986–1987 and 1987–1988, and is based on the temperature, wind, and cloud observations made by Russian drifting ice stations. It also relies on the ERA40 re-analyses of the European Centre for Medium-Range Weather Forecasts, which were utilised to calculate the lateral heat advection at the sites of the ice stations. The cloud cover and wind speed were more important than the heat advection in controlling the magnitudes of θ2 m and θS, while on a time scale of 24 h, during steady forcing conditions, the heat advection was the most important factor affecting the changes in θS and θ2 m. During changing conditions, and considering individual factors separately, the monthly mean 24-h temperature changes were less than ± 5 °C: the effect of the cloud cover was the largest, and that of the heat advection was the smallest. When simultaneous changes in the three factors were analysed, the seasonal mean temperature changes were even of the order of ±15 °C, with the strongest warming events exceeding 35 K in a single day. The difference θS − θ2 m reached its lowest seasonal mean values during conditions of clear skies (−1.3 °C), light winds (−1.3 °C) and warm-air advection (−0.8 °C). θS and θ2 m followed each other closely, even during major synoptic-scale temperature variations.  相似文献   
989.
The Holocene sea-level high stand or “marine limit” in Wilkes Land, East Antarctica, reached 30 m above present sea level at a few dispersed sites. The most detailed marine limit data have been recorded for the Windmill Islands and Budd Coast at the margin of the Law Dome ice cap, a dome of the East Antarctic Ice Sheet (EAIS). Relative sea-level lowering of 30 m and the associated emergence of the Windmill Islands have occurred since 6900 14C (corr.) yr B.P. Numerical modeling of the Earth's rheology is used to determine the glacio-isostatic component of the observed relative sea-level lowering. Glaciological evidence suggests that most of EAIS thickening occurred around its margin, with expansion onto the continental shelf. Consequently, a regional ice history for the last glacial maximum (LGM) was applied in the glacio-isostatic modeling to test whether the observed relative sea-level lowering was primarily produced by regional ice-sheet changes. The results of the modeling indicate that the postglacial (13,000 to 8000 14C yr B.P) removal of an ice load of between 770 and 1000 m from around the margin of the Law Dome and adjacent EAIS have produced the observed relative sea-level lowering. Such an additional ice load would have been associated with a 40- to 65-km expansion of the Law Dome to near the continental shelf break, together with a few hundred meters of ice thickening on the adjoining coastal slope of the EAIS up to 2000 m elevation. Whereas the observed changes in relative sea level are shown to be strongly influenced by regional ice sheet changes, the glacio-isostatic response at the Windmill Islands results from a combination of regional and, to a lesser extent, Antarctic-wide effects. The correspondence between the Holocene relative sea-level lowering interpreted at the margin of the Law Dome and the lowering interpreted along the remainder of the Wilkes Land and Oates Land coasts (105°–160° E) suggests that a similar ice load of up to 1000 m existed along the EAIS margin between Wilkes Land and Oates Land.  相似文献   
990.
一个热动力海冰模式的改进与实验   总被引:2,自引:0,他引:2  
影响海冰变化的物理因素中热力和动力部分是同等重要的,但多数热动力海冰模式的热力部分考虑得较为简单。针对Hibler热动力海冰模式的不足,以1个3层热力模式为基础改进了其热力部分。比较了原模式中的零层热力模式和用于改进的3层热力模式;并应用改进前后的两种热动力模式对1983年的北极海冰进行了模拟。模拟结果表明,海冰厚度比原模式厚,季节变化减弱,海冰密集度与观测资料更为符合。  相似文献   
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