Impact of the Vertical Velocity Field on Charging Processes and Charge Separation in a Simulated Thunderstorm

A three-dimensional(3D) charging-discharging cloud resolution model was used to investigate the impact of the vertical velocity field on the charging processes and the formation of charge structure in a strong thunderstorm. The distribution and evolution of ice particle content and charges on ice particles were analyzed in different vertical velocity fields. The results show that the ice particles in the vertical velocity range from 1 to 5 m s-1obtained the most charge through charging processes during the lifetime of the thunderstorm. The magnitude of the charges could reach 1014 n C. Before the beginning of lightning activity,the charges produced in updraft region 2(updraft speed 13 m s-1) and updraft region 1(updraft speed between 5 and 13 m s-1) were relatively significant. The magnitudes of charge reached 1013 n C, which clearly impacted upon the early lightning activity. The vertical velocity conditions in the quasi-steady region(updraft speed between –1 and 1 m s-1) were the most conducive for charge separation on ice particles on different scales. Accordingly, a net charge structure always appeared in the quasi-steady and adjacent regions. Based on the results, a conceptual model of ice particle charging, charge separation, and charge structure formation in the flow field was constructed. The model helps to explain observations of the"lightning hole" phenomenon.     

A brief introduction to BNU-HESM1.0 and its earth surface temperature simulations

Integrated assessment models and coupled earth system models both have their limitations in understanding the interactions between human activity and the physical earth system. In this paper,a new human–earth system model,BNUHESM1.0,constructed by combining the economic and climate damage components of the Dynamic Integrated Model of Climate Change and Economy to the BNU-ESM model,is introduced. The ability of BNU-HESM1.0 in simulating the global CO2 concentration and surface temperature is also evaluated. We find that,compared to observation,BNU-HESM1.0underestimates the global CO2 concentration and its rising trend during 1965–2005,due to the uncertainty in the economic components. However,the surface temperature simulated by BNU-HESM1.0 is much closer to observation,resulting from the overestimates of surface temperature by the original BNU-ESM model. The uncertainty of BNU-ESM falls within the range of present earth system uncertainty,so it is the economic and climate damage component of BNU-HESM1.0 that needs to be improved through further study. However,the main purpose of this paper is to introduce a new approach to investigate the complex relationship between human activity and the earth system. It is hoped that it will inspire further ideas that prove valuable in guiding human activities appropriate for a sustainable future climate.     

甘肃北山—河西走廊—祁连山区域地下水循环模式

山区地下水流动受到区域气候条件、地形地貌、地质构造等因素共同控制,限于资料有限,其流动模式与控制机理尚不清晰.特别是地处甘肃北山的高放废物地质处置库预选区、河西走廊以及祁连山北麓区域地下水的流动模式,直接决定了处置库在万年时间尺度上的安全性.基于区域遥感构造解译、地质构造演化分析、地球物理勘探以及水文地质钻探,获取了典...     

2.4m望远镜网络安全初步设计

云南天文台将在2.4m望远镜建立远程观测系统。由于远程观测系统通过网络实现通信,必然会面临网络上的各种威胁。为了保证整个网络系统的安全,避免各种不安全因素造成的损失。在对现在望远镜网络分析基础上设计了安全的网络结构,并实现了具有入侵检测功能的防火墙,这些措施初步保障了2.4m望远镜网络系统的安全。     

2.4m望远镜曝光时间计算器的设计和实现

望远镜的曝光时间计算器对于远程观测以及不熟悉整个观测系统的观测人员尤为重要,因为它可以帮助观测者制定合理的观测计划。设计并实现了高美古2.4m望远镜系统的曝光时间计算器(exposuretimecalculator,ETC),它可以根据望远镜及其终端设备的参数,通过计算给出待测天体曝光时间的参考值。这为观测者了解现有条件下极限观测能力,设置曝光时间或者是给定星等和曝光时间计算信噪比提供了依据。将ETC计算结果与实际测光标准星的数据进行了比较,结果表明ETC对测光标准星的计算结果是可靠的。     

青海天峻新关角隧道涌排水水源识别与量化分析

涌排水严重影响隧道施工与运行安全,查明隧道涌排水的来源,是隧道防水止水重要科学依据.青海天峻新关角隧道南北洞口处的地下水排水量分别为10021,60877 m3/d,两者存在近50000 m3/d的差异,涌排水量大,且来源不明.基于水文地质条件分析,分别采集了新关角隧道隧址区内大气降水、不同类型地下水和隧道出口涌排水水...     

Iron and phosphorus effects on the growth of Cryptomonas sp. (Cryptophyceae) and their availability in sediments from the Pearl River Estuary, China

Based on lab-culture experiments analyzing limitation and combination of iron and phosphorus on the growth of Cryptomonas sp. (Cryptophyceae), and the study of accumulation and release of Fe-bound P in sediment cores collected from the marine region of the Pearl River Estuary, China, reasons for the high frequency of phytoplankton bloom therein are discussed. Results show that the combined effect of Fe and P can obviously accelerate algal development, and the optimum culture conditions maintaining maximum growth rate are 0.05 μM Fe and 50 μM P. Cellular contents of Fe and P is consistent and the P:Fe molar ratio is 159:1. The optimum range of the P:Fe molar ratio in culture experiments for cell incubation is 500–1400. The vertical trends of total Fe and total P variations in sediments are parallel. Fe-bound P is the main species of inorganic sedimentary P. Through continuous leaching with agitation, 34–80% of exchangeable P and 4–23% of exchangeable Fe are concurrently released from the surficial sediments. This is a possible way by which nutrients are made available to phytoplankton. These factors might be responsible for a high frequency of harmful algal blooms in the Pearl River Estuary.     

安徽庐枞火山岩盆地橄榄玄粗岩系的地球化学特征及其对下扬子地区晚中生代岩石圈减薄机制的约束

庐枞盆地内的中生代火山-潜火山岩具高钾和相对富碱为特性,属典型的橄榄玄粗岩系列。它们在地球化学上表现出明显富集Rb、Th、U、K等强不相容元素和轻稀土元素,亏损高场强元素Nb和Ta的特征。Nd、Sr同位素组成总体位于富集型的扬子克拉通岩石圈地幔的范围内或其附近,显示其母岩浆主要是由富集型地幔部分熔融形成的。火山-潜火山岩的成分变异趋势显示橄榄玄粗质幔源岩浆在高压下(斜长石稳定压力之下,1.5GPa)经历过以单斜辉石和钛铁氧化物为主的矿物分离结晶作用。低压下矿物的分离结晶作用及上地壳物质的混染则不明显。这套火山-潜火山岩的部分地球化学性质(如Ce/Yb比值)类似于大洋岛弧内的橄榄玄粗岩,可能意味着区内由于岩石圈的减薄,软流圈地幔上涌到了岩石圈相对较浅的部位,控制源区部分熔融的主要是尖晶石相地幔岩。虽然局部(如靠近郯庐断裂的盆地西缘)可能存在着明显的热侵蚀,但"突发性的"机械拆沉是区内(乃至整个长江中下游地区)岩石圈减薄的主要机制。在整个晚中生代岩石圈减薄的过程中,这两种机制可能一直相互促进着。