“93.5”黑风暴发展结构和不同模式分辨率的数值试验

1993年5月4～6日在我国西北部地区发生了一次“黑风暴”。用改进的MM1和高分辨PBL参数化及40 km细网格控制试验能基本上模拟出“93.5”黑风暴的结构和演变。模拟结果表明，黑风暴发展时段，在PBL内与一个中尺度气旋性强涡旋相伴，在对流层内与一个垂直涡柱相伴。这个伸展至对流层顶的涡柱下（上）半部是与低（高）空强烈辐合（辐散）入（外）流相伴的气旋（反气旋）性涡柱。该黑风暴结构不同于一般锋面结构，其主要判别是:界面坡度陡，θe水平梯度大，斜压性强，PBL内暖心明显。该暖心结构与下垫面剧烈热力强迫有关。不     

南极中山站与北京地磁中心台1991年3月24日磁暴的变化特征

本文分析了１９９１年３月２４日急始型磁暴的变化特征。分析表明，南极极隙区与中低纬区磁暴形态差异很大。中山站地磁台的磁暴急始为ＳＣ＊型，无明显磁暴主相，它是由一组强烈的磁亚暴所组成。北京地磁中心台的磁暴急始为ＳＣ型，磁暴主相持续时间较短，变化较大。这次磁暴是由磁暴前太阳黑子相对数增多、３月２２日２２ｈ４６ｍＵＴ有３ｂ级耀斑爆发等一系列太阳活动所引起的     

河南晚石炭世含煤地层中的风暴异地煤

河南省晚石炭世含煤地层中,存在着因风暴作用强烈侵蚀滨海泥炭沼泽,而后通过风暴回流把泥炭物质和植物遗体长距离搬运到浅海环境再沉积的风暴异地煤。这种异地煤的直接顶底板是具有风暴沉积特征的浅海碳酸盐岩.煤破碎成粉砂级—泥级,煤层原生结构已完全看不到,煤层下部为含有大量海相动物化石的滞积层,中部为具有类似丘状层理的波状层,上部为水平纹层,其层序特征几乎可与煤层直接顶底板浅海碳酸盐风暴岩类比。研究这种异地煤的沉积背景和形成机制以及这种煤层所反映出的煤质特征、煤岩特征、沉积特征、层序及层序类型特征,不仅可以开拓出一种新型异地成煤类型而扩大煤地质学的研究领域,而且有助于研究古气候、古水深和煤岩层对比等问题。     

Storm surges in the northern part of the Sea of Japan

All the available historic records of sea level and appropriate weather charts have been used to study storm surges in the northern part of the Sea of Japan. The generation of surges in this area was investigated by means of a two-dimensional numerical model. Computed sea levels were compared with hourly observed residual sea levels in De-Kastri. The agreement between computed and observed storm surges is quite satisfactory. The relative importance of various meteorological parameters and bottom topography in formation of the strong storm surge on 20–21 September 1975 was studied numerically.     

Atmospheric pollution assessment near potential source of natural aerosols in the South Gobi Desert region,China

ABSTRACT

Rapid economic growth, a high degree of urbanization and the proximity of a large number of desert and semidesert landscapes can have a significant impact on the atmosphere of adjacent territories, leading to high levels of atmospheric pollution. Therefore, identifying possible sources of atmospheric pollution is one of the main tasks. In this study, we carried out an analysis of spatial and temporal characteristics of five main atmospheric pollutants (PM_2.5, PM₁₀, SO₂, NO₂, and CO) near potential source of natural aerosols, affecting seven cities (Wuhai, Alashan, Wuzhong, Zhongwei, Wuwei, Jinchang, Zhangye), located in immediate proximity to the South Gobi deserts. The results, obtained for the period from 1 January 2016 to 31 December 2018, demonstrate total concentrations of PM_2.5 and PM₁₀ are 38.2 ± 19.5 and 101 ± 80.7 μg/m³ exceeding the same established by the Chinese National Ambient Air Quality Standard (CNAAQS), being 35 and 70 μg/m³, respectively. Based on the data from Moderate Resolution Imaging Spectroradiometer (MODIS) for the whole period, Clean Сontinental (71.49%) and Mixed (22.29%) types of aerosols prevail in the region. In the spring and winter seasons maximum concentrations of pollutants and high values of Aerosol Optical Depth (AOD) in the region atmosphere are observed. PM_2.5 and PM₁₀ ratio shows the presence of coarse aerosols in the total content with value 0.43. The highest concentrations of pollutants were in the period of dust storms activity, when PM_2.5 and PM₁₀ content exceeded 200 and 1000 µg/m³, and AOD value exceeded 1. UV Aerosol Index (UVAI), Aerosol Absorbing Optical Depth (AAOD), and Single Scattering Albedo (SSA), obtained from Ozone Monitoring Instrument (OMI), demonstrate the high content of dust aerosols in the period of sandstorms. Analysis of backward trajectories shows that dust air masses moved from North to Northwest China, affecting large deserts such as Taklamakan, Gurbantunggut, Badain Jaran, Tengger, and Ulan Buh deserts.     

副高异常偏西背景下西北一次漏报的雷暴大风中尺度分析*

摘要：利用西安多普勒天气雷达、L波段风廓线雷达和加密自动站探测资料，结合天气实况，对2018年7月26日发生在陕西一次副热带高压影响下的的强风暴过程进行了中尺度分析。结果表明：（1）本次强风暴伴随的阵风锋共维持了4h，其中有3h出现7级以上的大风，且最大风力10级。（2）在副热带高压影响下，陕西处于高温、高湿气团中，大气层结极不稳定。（3）此次强风暴在高的对流有效位能环境下（CAPE）下，抬升触发的关键因子是关中地区中尺度辐合线，当初生的对流云团下山后，中尺度辐合线触发的对流风暴形成小范围冷池出流与环境风场形成新的辐合线，加强对流风暴发展。（4）当阵风锋移动过程中遇到前方的对流云团时，将低层暖湿空气抬升，并随着上升气流输送到主体对流风暴中，迅速补充了主体风暴的能量，使得主体风暴再次强烈发展，延长了阵风锋的生命史。     

具有尘带的椭圆星系的红外辐射特性

IRAS在12,25,60和100μm的巡天,给我们提供了研究各类星系红外辐射特性的可能。为了研究具有尘带的E和SO星系的红外辐射特性,我们利用了E.Sadler给出的完备的E和SO星系表。在该星系表中共列出248个夭体,其中38个被证记为IRAS点源,且又有确切的60和100μm的流量值。在这38个天体中有6个被列在K.Ebneter和B.Balik最新发表的具有全带的椭圆星系表中。我们以这6个星系作为具有尘带的E和SO星系的样本,其它32个没有尘带的E和SO星系即作为对照样本。为了讨论具有尘带的椭圆星系的红外辐射特性,我们利用非参数Mann-Whitney检验,对这两个样本的LIR和FIR/FB的分布作了讨论,结果是在对于置信度α=0.05的水平上,我们不能拒绝另一假设:这两个样本的LIR和FIR/FB的分布是相同的。对于同时具有25,60和100μm确切流量的E和SO星系我们讨论了它们的双色图,结果发现,不具尘带的E和SO星系都处于Rowan-Robinson.et al所指出的正常星系区,而一些具有尘和带的ESO星系,则远离这一区域,它们是LINER和SEYFERT星系。     

登陆过程中热带风暴"黄蜂"螺旋云带的分析

分析了热带风暴"黄蜂"在登陆过程中逐小时高分辨红外云图上的螺旋云带及其强对流云团的变化规律.从强对流云团发展为主螺旋云带的演变过程中,螺旋云带主要表现为其前端的对流逐渐加强,其余部分逐渐减弱,以及前端的强对流云团总体表现为旋入运动且维持时间较长,而其余部分的云团总体表现为远离中心等的特征.初步探讨了螺旋云带结构变化与风暴强度之间的关系和"黄蜂"在登陆后迅速减弱的可能原因.     

Oxygen isotope compositions of quartz grains (4–16 μm) from Chinese eolian deposits and their implications for provenance

Oxygen isotope compositions were measured in quartz grains extracted from a 7.0 Ma red clay-loess sequence at Lingtai and six late Pleistocene loess sediments (Malan loess). Results show that the changes in oxygen isotope compositions of Malan loess are basically controlled by the geochemical characteristics of the source materials, while the effect of weathering process after dust deposition could be minor. The oxygen isotope distribution of quartz grains from red clay at Lingtai is similar to that of the overlying loess-paleosol sequence, thus indicating that the red clay at Lingtai has the same eolian origin as the loess-paleosol deposits. Furthermore, the oscillations of the isotope compositions in 4–16 μm-sized quartz grains may reflect the changes, to some extent, of the climatic systems of the source region.