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91.
1311号强台风“尤特”登陆后给广东带来持续性大范围强降水,对流降水特征显著.分析了“尤特”影响期间大尺度环流背景,重点讨论了此次持续性强降水过程中大气层结问题.发现低空急流向广东输送强的暖平流,是广东大气层结不稳定得以持续维持的根本原因.进一步分析发现,低空急流本身并不是“暖”的,当“尤特”趋向陆地时,陆地上的暖气团在“尤特”环流强迫下向南传播扩散,低空急流穿越这一暖区时温度升高才具备“暖”的特性.这一事实在以前并未被关注到.通过个例反查,在许多登陆后造成连续强降水的台风过程中均发现了这一特征.因此,台风登陆引起环境温度场的演变以及与低空急流的配置需引起重视. 相似文献
92.
Both direct and indirect effects of freezing drizzle on ice accretion were analyzed for ten freezing drizzle events during a comprehensive ice thickness, fog, and precipitation observation campaign carried out during the winter of 2008 and 2009 at Enshi Radar Station (3017'N, 10916'E), Hubei Province, China. The growth rate of ice thickness was 0.85 mm h-1 during the freezing drizzle period, while the rate was only 0.4 mm h-1 without sleet and freezing drizzle. The rain intensity, liquid water content (LWC), and diameter of freezing drizzle stayed at low values. The development of microphysical properties of fog was suppressed in the freezing drizzle period. A threshold diameter (Dc) was proposed to estimate the inuence of freezing drizzle on different size ranges of fog droplets. Fog droplets with a diameter less thanDc would be affected slightly by freezing drizzle, while larger fog droplets would be affected signicantly. Dc had a correlation with the average rain intensity, with a correlation coefficient of 0.78. The relationships among the microphysical properties of fog droplets were all positive when the effect of freezing drizzle was weak, while they became poor positive correlations, or even negative correlations during freezing drizzle period. The direct contribution of freezing drizzle to ice thickness was about 14.5%. Considering both the direct and indirect effects, we suggest that freezing drizzle could act as a catalyst causing serious icing conditions. 相似文献
93.
The South Karakorum margin, east of the Himalayan syntaxis, consist of an E–W elongated zone of young (10–3 Ma) high‐grade metamorphic rocks (M2) and related migmatitic domes. This late tectono‐metamorphic event post‐dates the Palaeogene (55–37 Ma) phase of thickening of the belt featured by NW–SE structures and associated M1 amphibolite facies metamorphism (0.7 GPa, 700 °C). This M2 metamorphism is characterised by low‐pressure, high‐temperature conditions coeval with migmatite formation in response to a thermal increase of c. 150 °C compared to M1, culminating at a temperature of c. 770 °C and a pressure of 0.5–0.6 GPa. Rapid exhumation of migmatitic domes, at a rate of 5 mm yr?1, was accommodated by vertical extrusion, in the core of E–W crustal‐scale folds. These crustal‐scale folds formed in response to N–S syn‐collisional shortening and were enhanced by thermal weakening of the migmatised continental crust. M2 metamorphism is spatially and temporarily associated with granitoids showing a mantle affinity, firmly suggesting that this could be the advective heat source for the granite and syenite generation and the subsequent migmatisation of the mid‐crustal level. Such relationships between a mantle‐related magmatism and a high‐temperature metamorphism in a convergent shortening context are suggestive of the breakoff of the subducted Indian slab since 20 Ma. 相似文献
94.
朱志愚 《成都信息工程学院学报》1997,(4)
作者应用动力学分析方法,结合观测飞机颠簸的事实,对高空急流区飞机颠簸的一种形成机理进行了理论探讨。结果表明,高空急流区温度平流分布的不均匀性,会在急流附近等温线密集区边缘激发出空气垂直运动和湍流,引起飞机颠簸。 相似文献
95.
Xiao-yong Liu Pi-bo Yang Lan-tian Yang Shao-li Chen 《Chinese Astronomy and Astrophysics》1997,21(4):405-414
Considering nonthermal e±-pair production, this paper is focused on the radial structure of hot one-temperature accretion flows with advection under the condition of small viscous parameter ( = 0.1) and low mass-accretion rates. Self-similar relations of hot flow with advection have been adopted. The authors have used a scheme, in which the two regions of accretion flow are calculated separately and then joined together. Some typical features of hot flow with advection have been confirmed, and several new results obtained: there exists a critical radius rcr; the local cooling rate is inversely proportional to the square of the mass of the central object; the e±-pair process affects significantly the radiation of hot flows with advection. 相似文献
96.
We have performed a one-dimensional and transient radiative heat transfer analysis in order to investigate interaction between atmospheric radiation and convective instability within a nocturnal fog. The radiation element method using the Ray Emission Model (REM2), which is a generalized numerical method, in conjunction with a line-by-line (LBL) method, is employed to attain high spectral resolution calculations for anisotropically scattering fog. The results show that the convective instability has a strong dependence on radiative properties of the fog. For the condition of a 20-m droplet diameter and liquid water content of 0.1 × 10–3 kg m–3;, the temperature profile within the fog becomes S shaped, and a convective instability layer forms in the middle or lower level of the fog. However, for the same water content and a 40-m diameter droplet, no strong convective instability layer forms, whereas for a 10-m diameter droplet a strong convective instability is observed. 相似文献
97.
南京冬季浓雾的演变特征及爆发性增强研究 总被引:5,自引:2,他引:3
2007年12月18—19日,南京地区出现了一次持续20h的浓雾过程,其中能见度低于50m的强浓雾几乎占到整个雾过程的1/3。利用同期在南京市北郊的外场观测数据,结合NCEP再分析资料,分析了该次雾的演变过程、微物理结构及边界层特征,探讨了地面雾爆发性增强的成因。结果表明:本次雾在西南平流的增湿作用下触发生成;日出后,平流输送和地表蒸发提供了充足水汽来源,贴地层逆温因高空下沉增温而向上抬升且稳定存在,因此大雾得以维持;整个雾过程中雾滴数浓度、平均直径、含水量随时间的变化趋势基本一致,平均谱曲线均呈指数下降分布,雾滴集中在小滴端;两次地面雾爆发性增强均发生在夜间,其特征为各微物理参量明显增大,滴谱上抬拓宽;爆发性增强的原因是地表气温陡降、贴地层逆温增强及可充当雾滴凝结核的气溶胶大粒子数增多。 相似文献
98.
两次降雪天气过程预报中边界层风廓线雷达资料的应用 总被引:1,自引:0,他引:1
通过分析2009年10月31日至11月1日和2009年11月9-10日北京两次不同类型降雪天气过程中海淀边界层风廓线仪数据发现:①降雪开始前2h内底层偏东气流建立,且该气流里均有风速突然加强的现象,这对短时临近预报中预报降雪的起始时间有一定参考价值;②700 hPa以上出现冷平流或者冷平流加强且高度降低,也是降雪即将开始的一个特征;③风廓线资料计算得到的温度平流廓线可以较好的反应大气稳定度情况,为判断降雪是否为对流性降雪提供可靠依据.在临近预报中加强风廓线和温度平流的监测,对临近转折性天气的预报有指示意义. 相似文献
99.
100.
A Numerical Study of the Urban Intensity Effect on Fog Evolution in the Beijing-Tianjin-Hebei Region 总被引:2,自引:0,他引:2
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The influence of urban intensity on fog evolution in the Beijing-Tianjin-Hebei (BTH) region (China) is investigated numerically with the the Weather Research and Forecasting (WRF) model coupled with the urban canopy parameterization-building energy model (UCP- BEM) urban physics scheme. The experiments were designed with a focus on the influence of different urban intensities, which are represented by a different fractional coverage of natural land, buildings, and energy consumption inside buildings in an urban environment. The results of this study indicate that urban areas notably influence fog evolution when natural land is reduced to a small fraction (e.g., less than 10%). Developed land changes fog evolution through urban effects. Higher urban intensity (HUI) generally results in warmer temperatures and lower wind speeds throughout the day, while inhibiting morning specific humidity loss and afternoon specific humidity gain because of the HUI effect on surface heat flux, surface roughness, and surface moisture flux. HUI leads to later and weaker liquid water content formation, with a higher liquid water content base, primarily due to its effect on near surface temperatures. This finding implies that HUI may inhibit the conditions for fog formation. In addition, urban areas with equal natural and developed land coverage seem to greatly enhance the upward surface moisture flux, which is attributed to the combination of a relatively large potential evaporation on developed land and an ample moisture supply from natural land. As a result, the specific humidity increases in the afternoon. 相似文献