中国建设用地变化的空间分异特征

采用变异系数、希尔指数与空间自相关方法对我国2002—2008年建设用地变化的区域差异及空间相关性进行了探讨。结果显示:(1)2002—2008年我国区域建设用地的变化差异总体上呈减小趋势,但区域差异仍较为明显。(2)我国区域建设用地的增长呈现明显的空间二元结构,东部地区"高高"聚集,西部地区"低低"聚集。当前我国土地利用处于"倒U"型变化曲线的顶部区域,土地利用的压力依然很大,应根据土地利用变化的差异性及空间相关性,科学地制定区域土地供给政策。     

华北地区晴空颠簸的分类特征及分析

以2005-008年发生在北京飞行管制区范围内的18例晴空颠簸为样本,在普查颠簸发生时天气形势的基础上,对造成华北地区晴空颠簸的天气形势进行分类,分为高空急流型、高空槽线型、切变线型和高空脊型.并结合卫星云图,归纳总结了每类晴空颠簸的特点和预报着眼点.通过对2006年1月2日发生在华北地区的一次飞机颠簸过程进行诊断分析,结果表明:在高空急流区边缘风切变较大及与高空急流相联系的等温线密集区边缘温度梯度较大的区域易产生颠簸.飞机颠簸的发生, 是温度平流通过在高空急流附近的等温线密集区边缘所激发出的垂直运动引起.     

豫西深秋一次典型超级单体风暴的多普勒雷达分析

利用三门峡市多普勒天气雷达资料,分析了2009年10月4日发生在河南渑池县的一次产生冰雹的超级单体风暴的回波结构及演变特征,结果表明:超级单体是在上冷下暖的大尺度环流背景和不稳定层结下产生的;其演变过程经历了生成、发展、成熟、消亡四个阶段;局地生成的弱回波若发展较快,速度场中又有逆风区与之配合,则容易发展成超级单体风暴,应引起高度重视;发展阶段回波强度加速增大,诸如底层钩状回波、有界弱回波区、中气旋等超级单体的典型结构特征开始出现,是发布预警的关键时段,大约可以提前15-30 min;成熟阶段最重要的特征是持续存在的中气旋。超级单体风暴其初始回波出现在4 km左右的中空,具有向上向下迅速发展的特点;最强回波强度大,顶高伸展高;当最强回波底到达地面时意味着冰雹、降水的开始,因而可以通过分析最强回波顶高的演变趋势来确定降雹强弱和时间;VIL可用来判断对流风暴强度,持续高的VIL值可能与超级单体风暴有关。     

运用能量学方法分析大冰雹的落区

运用大气能量学的方法,对2002年7月19日发生在河南省中西部地区的降雹过程进行了分析,结果显示:大冰雹均出现在高空能量锋区以内,落区在低层湿有效能量平流正值中心附近。利用能量分析作为预报基础,再结合地面和雷达探测等资料进行综合分析,可以得出有无冰雹天气及冰雹落区的预报结论。     

Holocene environmental change inferred from the loess–palaeosol sequences adjacent to the floodplain of the Yellow River, China

Chinese loess deposits are generally considered to be the product of dust storms and dust falls from the central Asia arid zones that were transported across China by the northwesterly continental monsoon. In contrast, the Zhengzhou Loess found southeast of the Loess Plateau, adjacent to the floodplain of the Yellow River, records a different eolian regime and dust source. The Zhengzhou Loess was investigated by field observations, measurements of magnetic susceptibility, particle-size distribution, loss-on-ignition, CaCO₃ and chemical contents. Both field observations and the laboratory results indicate that, during the last glacial, the Zhengzhou Loess was supplied by two different eolian regimes and dust sources, one was from the fresh flood deposits of the Yellow River driven by the northeast winds from the low-lying floodplain, and the other was from the dust storms and dust falls that traveled across the Loess Plateau driven by the northwesterly continental monsoon from the central Asian arid lands. The early Holocene, 11,500–8500 a BP, was a transition during the change in eolian regime and dust source because of the weakened northwesterly monsoon along with the global climatic amelioration. Following the retreat of the northwesterly monsoon from the onset of the mid-Holocene Climatic Optimum at 8500 a BP, dust supply from the drifting sand zone on the Yellow River floodplain became dominant because of the intensified strength of the northeast winds from the Bohai Sea. From 3100 a BP onwards, climatic aridity and extensive human disturbance have resulted in intensive eolian processes causing the incursion of the drifting sand into the Zhengzhou Loess zone. These results show that loess accumulation is more complex than traditionally assumed. The origin of loess deposits elsewhere outside the Loess Plateau may be related to dust sources derived from alluvial sediments of major river systems.     

Star formation in the starburst cluster in NGC 3603

We have used new, deep, visible and near infrared observations of the compact starburst cluster in the giant HII region NGC 3603 and its surroundings with the WFC3 on HST and HAWK-I on the VLT to study in detail the physical properties of its intermediate mass (∼1–3 M_⊙) stellar population. We show that after correction for differential extinction and actively accreting stars, and the study of field star contamination, strong evidence remains for a continuous spread in the ages of pre-main sequence stars in the range ∼2 to ∼30 Myr within the temporal resolution available. Existing differences among presently available theoretical models account for the largest possible variation in shape of the measured age histograms within these limits. We also find that this isochronal age spread in the near infrared and visible Colour-Magnitude Diagrams cannot be reproduced by any other presently known source of astrophysical or instrumental scatter that could mimic the luminosity spread seen in our observations except, possibly, episodic accretion. The measured age spread and the stellar spatial distribution in the cluster are consistent with the hypothesis that star formation started at least 20–30 Myrs ago progressing slowly but continuously up to at least a few million years ago. All the stars in the considered mass range are distributed in a flattened oblate spheroidal pattern with the major axis oriented in an approximate South-East–North-West direction, and with the length of the equatorial axis decreasing with increasing age. This asymmetry is most likely due to the fact that star formation occurred along a filament of gas and dust in the natal molecular cloud oriented locally in this direction.     

CFRP加固一字形竖缝耗能预制剪力墙抗震性能研究

以一字形竖缝耗能预制剪力墙作为研究对象,设计了3个装配式剪力墙试件及1个现浇剪力墙对比试件,进行低周往复荷载试验,并对破坏墙体进行CFRP加固,再次进行拟静力试验。试件变化参数包括轴压比、混凝土强度等级及配筋率,对比分析加固前后试件滞回性能、刚度退化、承载力和耗能能力等性能。试验结果表明,与现浇剪力墙相比,一字形竖缝耗能预制剪力墙工作性能良好,阻尼器屈服耗能提高了试件整体工作性能;CFRP加固可有效抑制墙体斜裂缝的发展,对墙体承载力及耗能能力均有显著改善作用;各试件均满足剪力墙弹塑性层间位移角限值要求,延性较好;试件整体表现出良好的抗震性能。