甘肃河西走廊沙尘暴与赤道中,东太平洋海温之间的遥相关分析

春、夏季甘肃河西走廊沙尘暴发生次数与赤道中、东太平洋海温之间遥相关分析结果表明：春、夏季河西走廊沙尘暴发生次数与前二年赤道中、东太平洋海温的负相关最好,时间过远或过近,相关性反而较差。利用前期的赤道中、东太平洋海温可以较好地预报出河西走廊春季沙尘暴发生的多寡。     

香港全新世沉积物中的风暴潮记录

香港是受台风暴潮影响最严重的地区之一。本项研究是根据近岸及浅海地区沉积物的特征性来分析和获取全新世的时期的台风暴潮信息。根据沉积结构和构造特征,发现有５种类型的沉积层：粉砂质粉土、砂质粒序层、水平或波状层理层、贝屑富集层和含贝屑粉砂层,其中后４种类型与台风暴潮有关。根据沉积物的磁化率分析,上部深度的高磁化率层可能与台风暴潮对现代受污染沉积物的改造致使新老沉积物的混合所致。有孔虫分析显示,风暴沉积层     

磁暴二倍法预报唐山7.8级地震

磁暴二倍法预报地震的依据是,应变能在运移过程中导致地壳膨胀和压缩形成一个周期,在时间上呈有二倍关系．唐山７．８级地震是我国７０年代最大地震,用磁暴二倍法推出有４组磁暴能对应这次地震．每组磁暴前后都发生了地震,由于这些地震释放的剩余能量在聚积过程中,地壳发生膨胀和压缩,地磁场就受到影响形成了磁暴．因此磁暴与地震能量变化有相关性．可见,磁暴二倍法可以预报地震．     

华北北部黑风暴的气候学特征

使用内蒙古中西部72个地面测站1957～1996年历史资料,分析研究了该地区黑风暴的气候学特征,包括黑风暴的地理分布、年代际变化、年际变化、年变化、旬变化、日变化等时间变化特征和强度变化;讨论了形成上述变化特征的气候成因。得到如下结论：内蒙古中西部是黑风暴的易发区和多发区,最大中心位于内蒙古中部的朱日和;黑风暴的时间变化特征显著;强度有较大差异。     

一次弓状降雹回波区流场的反演

通过对一次典型弓状降雹回波区的流场进行反及特点分析,发现用矩不变量法反演出的回波区流场结构,与藤田关于弓状回波的概念模式非常吻合,利用该方法估测出的流场,散度场、涡度场所表现出的信息,与降雹实况是一致的,该研究可为中小尺度强天气的监测,提供高时空分辨率的流场资料。     

利用T106数值预报产品作江西暴雨动态落区预报

首先将江西测站的降水插值到1°×1°的经纬度网格点上,然后利用1°×1°的T106数值预报产品,对江西网格点上的暴雨送行诊断分析与相关普查,最后建立了江西暴雨动态落区预报模式和动态落区预报流程。     

Combined use of spot samples and continuous integrated sampling in a study of storm runoff from a lowland catchment in the south of England

We have used two different sampling techniques to study the geochemical response of a small lowland rural catchment to episodic storm runoff. The first method involves traditional daily spot sampling and has been used to develop a standard end‐member mixing analysis (EMMA) of the relative contributions of ground water flow and surface runoff to the total stream flow. The second method utilizes a continuous sampling device, powered by an osmotic pump, to produce an integrated 24‐h sample of the stream flow. When combined with the EMMA results from the spot samples, analyses of the integrated samples reveal the presence of a third component that makes a significant contribution to the dissolved NO₃, Ca and K export from the catchment during the rising limb of the hydrographic profile of a storm event following a prolonged dry period. The storm occurred in the middle of the night, so that the response of the stream chemistry was not captured by the daily samples. We hypothesize that this third component is derived from the flushing of stored soil water that contains the geochemical signature of decaying vegetation. Copyright © 2011 John Wiley & Sons, Ltd.     

风暴潮灾害情景下海岸带暴露指数时空演变研究——以福建省东山湾为例

暴露指数反映了环境在面对极端天气事件时承受灾害的潜在风险程度。研究利用遥感影像数据、数字高程数据(DEM)、海洋水深及风力数据等, 基于暴露指数模型, 以福建省东山湾为案例研究区域, 对风暴潮灾害情景下的海岸带暴露指数及其时空演变进行分析。研究结果显示: (1)近十年来, 东山湾海岸带暴露指数总体呈下降趋势, 潜在风险程度为“中”及以上区域占比由67.14%下降至59.06%, 海岸带在面对风暴潮灾害等极端天气事件时潜在的风险程度总体降低, 海湾地貌类型差异及其形态变化是影响东山湾暴露指数产生波动的主要原因; (2)基于暴露指数评价结果, 结合海岸带开发利用现状, 研究可对东山湾海岸带生态环境的敏感区域进行识别, 并制定具有针对性的开发利用与风险防范对策, 为海岸带空间规划、生态保护修复格局的科学划定提供理论支撑, 在助力海岸带陆海统筹和可持续发展上具有重要意义; (3)研究提出的一种基于时间序列的暴露指数研究技术路线和框架, 可为海岸带脆弱性评估、海岸带韧性评估、海岸带灾害监测预警等相关研究提供新的研究视角, 在基于深度学习的海岸带灾害风险预警与灾害模拟等方面也具有较为广阔的应用前景。     

Determining the source of dust storms with use of coupling WRF and HYSPLIT models: A case study of Yazd province in central desert of Iran

Dust storm, which has a significant impact on regional air quality, is one of the most hazardous meteorological phenomena in the arid areas. Yazd province is one of the arid areas in Iran that is exposed to dust storms. In this study, two cases of dust storms of Yazd province are studied with the use of coupling numerical models and aerosol optical depth (AOD) from MODIS data. We investigated synoptic condition of such dust storms that were formed downstream of upper level through in the area by focusing on two storms, on May 24 and 25, 2014. For this purpose, a dynamic coupling of this case is done using WRF output the HYSPLIT model. This model was implemented to investigate the sources of the dust storms by calculating the back trajectories from the receptor sites. The trajectories indicated that the first and the second case storms occurred in the northeast and the south of Yazd respectively. These results also showed a good agreement with MODIS aerosol optical depth data and HYSPLIT back trajectories paths.     

Spectrum of Fluctuations of Solar Noise Storms

The calculation of the Fourier transform of noise storm (NS) fluctuations showed that the power spectrum was adequately described by the expression G(F)∼1/F. Our results rule out the possibility that NS radiation is formed from random, short-term bursts (so-called type I bursts), since the spectrum of the sum of random short fluctuations is flat, but the real NS has a hyperbolic spectrum. This spectrum is monotonic and does not contain any components that exceed the level of the statistical fluctuations (i.e., the results of observations do not reveal the presence of periodic or resonant properties of the emission source). The hyperbolic shape of the spectrum shows that the main energy of a NS is contained in the slower temporal fluctuations.