台风“麦莎”的强度对台风前部飑线发展过程影响的研究   总被引：7，自引：4，他引：3  

刘佳  沈新勇  张大林  许映龙  毕明玉 《大气科学》2013,37(5):1025-1037

对2005年8月5日16时(UTC,下同)至6日00时发生的一次台风前部飑线过程进行了数值模拟,分析表明:台前飑线在母体台风和副高之间的湿区生成。台风为这次台前飑线过程提供了有利的条件,包括强的低空急流输送充沛的水汽,强的不稳定环境产生大的对流有效位能以及强的地表辐合,使得初始的离散的对流单体组织发展形成台前飑线。成熟时期的台前飑线虽然比中纬度和热带飑线的变压强度小,但是具有更强的低层暖湿空气入流,中层的入流范围也更加宽广。敏感性试验结果表明:台风强度越强,其台前飑线的回波强度越强,移动速度更快,生命史也更长。强台风使得低空垂直风切变更大,有利于台前飑线的生成和发展,在台前飑线发展成熟后,低空垂直风切变强度减小,不利于台前飑线的维持,加之低空水汽输送的减少,使其逐渐趋向衰亡。  相似文献   

新建地面气象自动站资料质量控制方法设计   总被引：9，自引：6，他引：3  

徐枝芳  陈小菊  王轶 《气象科学》2013,33(1):26-36

随着观测系统的加强,中国陆续出现许多新建的地面台站、地面自动观测站,但对这些新出现的台站由于缺少长时间序列的历史观测资料,无法通过本站观测统计分析建立质量控制技术.本文在传统的质量控制方法基础上,将全国地面观测站按照地域和气候特征分为8个区域,利用过去25 a存档的地面观测资料建立一套适合于新建地面自动站资料控制技术,对气压和温度采用极值检查、时间一致性检查和空间一致性检查等方法进行质量控制.并利用该质量控制技术对华南、长江中下游及华北地区2005年地面资料进行质量控制,结果表明:该控制方案能有效地将有问题的资料标识出来,可为新建地面自动站资料的应用提供一定的质量保障.不同区域的资料质量控制检查需依据不同地区的气候特点进行划分和统计,这样更能保障质量控制后资料的质量.  相似文献   

Implications of early action for JI baselines     

《Climate Policy》2013,13(1):57-66

Abstract

This article discusses possible implications of early Joint Implementation (JI) action. Some projects which would otherwise be non-additional during the first commitment period, can become additional by implementing them before 2008 through early JI. For example, several environmental investments that will be mandatory under the European Union (EU) Acquis Communautaire as of, e.g. 2008 or 2010 could be carried out earlier than that with early JI action. As such, candidate countries could partly finance the accession process through JI credits and their environmental standards would earlier be in line with the Acquis. The theoretical risk that projects would have to follow a slow track if JI parties are not eligible for the fast track is not large for JI hosts that are candidate for EU membership.  相似文献   

舒适度测量仪探测系统开发     

雷卫延  敖振浪  杨志健  蔡耿华 《气象科技》2013,41(5):960-964

舒适度测量仪探测系统主要由采集器、传感器、支架、供水系统、通信模块、数据采集软件6个部分组成.除通信模块之外,其他5个部分都是全新设计.采集器是系统的核心,负责数据的采集、处理和传输;数据采集软件安装在中心服务器上,负责数据的采集、处理、显示和存储,并能远程监测和遥控探测现场的设备.此外,对舒适度的相关理论进行分析,给出适合广州地区的舒适度指数分级标准,并对舒适度测量仪探测数据进行分析.近一年的试运行表明,系统运行稳定、探测数据可靠、适合业务组网的要求.  相似文献   

2010-2011年鞍山市能见度特征          下载免费PDF全文

赵胡笳  马雁军  朱轶明  高清源 《气象与环境学报》2013,29(1):18-22

利用2010年6月至2011年5月鞍山大气成分观测站的能见度资料,统计分析能见度与PM₁₀、PM_2.5、PM_1.0质量浓度、风速、降水强度和气溶胶光学厚度等气象要素的相关性。结果表明：鞍山市能见度月均值从8月份开始呈上升趋势,11月份达到峰值后开始显著下降,2月份达到最低值,自3月开始又出现较大幅度增长,进入夏季后略有下降;PM_2.5/PM₁₀、PM_1.0/PM₁₀比值与能见度呈反相关,能见度增大,PM_2.5/PM₁₀、PM_1.0/PM₁₀比值减小,且PM_1.0/PM₁₀的减小趋势更大,说明影响能见度的颗粒物以细粒子为主。平均风速与能见度变化趋势基本一致,与PM_2.5/PM₁₀、PM_1.0/PM₁₀的变化趋势呈反相关。随着雨强的增大,降水日能见度平均值随之减小,降水前一日和后一日的能见度平均值均大于降水日,且降水前一日及后一日的能见度改变量及改变率的绝对值随着降水强度的增加而增加。波长指数的变化说明影响鞍山能见度变化的污染物粒子整体较稳定,能见度与AOD成明显的反相关。  相似文献   

Distribution of CMEs with Different Angular Widths and Comparison with the Phase of Sunspot Number in the 23rd Solar Cycle     

MENG Wei-juan  LE Gui-ming  LIN Zhao-xiang  ZHANG Yong  YANG Xing-xing 《Chinese Astronomy and Astrophysics》2014

The variation of the number of coronal mass ejections (CMEs) with different angular widths in the period of 1996-2008 is analyzed statistically in this paper, together with a comparison of the feature of time variation between the number of CMEs with some typical angular widths and the number of sunspots.  相似文献   

UTEVA树脂分离纯化珊瑚中铀、钍的改进研究     

汤震宇  瞿建国  张安余  李秀保  杜金洲 《海洋学报》2022,44(2):11-20

珊瑚是记录海洋环境变化信息的载体之一,测定其U/Ca比值可重建海水温度或测定Th/U同位素比值可计算年龄重建海平面高度等.准确测定珊瑚中U、Th含量及同位素比值是提取所记载的海洋环境变化信息的前提,其难点在于高Ca基体分离和痕量U、Th富集纯化.基于此,本研究拟采用UTEVA树脂改进了一步富集分离珊瑚中U、Th的前处理...  相似文献   

RADIUS协议研究及在VOIP中的应用     

吴贞东  曾德胜 《成都信息工程学院学报》2006,21(6):837-840

对RADIUS协议进行了深入研究，给出了基于RADIUS协议的具有数据采集、认证授权、计费处理、查询统计和系统管理功能的VOIP安全认证计费系统设计与实现方案；系统可运用于IP电话安全认证和灵活计费。  相似文献   

More Emission Cones: Multi-frequency Simulation of the Pulse Profiles of PSR J0437-4715     

Guo-Jun Qiao  Xu-Dong Wang  Hong-Guang Wang  Ren-Xin XuDepartment of Astronomy  CAS-PKU Joint Beijing Astrophysics Center  Peking University  Beijing 《中国天文和天体物理学报》2002,2(4)

Pulsar radio emission beams have been studied observationally for a long time, and the suggestion is that they consist of the so-called core and conal components. To reproduce these components is a challenge for any emission model, and that the pulse profile of pulsars changes with frequency presents even a greater challenge. Assuming a local surface magnetic structure (to produce the core or central beam) and a global dipole magnetic field (to produce the conal beams), Gil & Krawczyk (1997) applied curvature radiation to the pulse profile simulation of PSR J0437-4715 (hereafter the GK model). Here we present an alternative multi-frequency simulation of the same profiles within the framework of the Inverse Compton Scattering (ICS) model. It is obtained from our simulation (1) that besides the core, the inner cone and the outer cone, there is an outer-outer cone; (2) that the emission components of the core and cones evolve strongly with frequency. Some important differences between the ICS model and the  相似文献   

A MERLIN survey of 4.7-GHz excited OH masers in star-forming regions     

L. Harvey-Smith  R. J. Cohen 《Monthly notices of the Royal Astronomical Society》2005,356(2):637-646

Phase-referenced observations of 13 star-forming regions in the  ²Π_1/2, J = 1/2  transition of rotationally excited OH at 4765 MHz have been carried out using MERLIN. Two of the regions were also observed at 4750 MHz and one at 4660 MHz. There were 10 maser detections at 4765 MHz and three non-detections. There were no detections at 4750 and 4660 MHz. The 4765-MHz masers have brightness temperatures of  ∼10⁷ K  at MERLIN resolution (∼50 mas). Several cases of 4765-MHz masers overlapping in position and velocity with 1720- and 1665-MHz masers are reported. There are also isolated 4765-MHz masers with peak flux densities ≥30 times that of any ground-state counterpart. Most of the 4.7-GHz maser spots are unresolved at 50-mas angular resolution, but in four of the nearest sources the maser spots are resolved, indicating a characteristic size for 4765-MHz maser regions of ∼100 au. In W3(OH) we discovered that 20 per cent of the 4765-MHz emission comes from a narrow low-brightness filament that stretches north–south for ∼1.0 arcec (∼2200 au) between two previously known 4765-MHz maser spots. The filament appears in projection against the H  ii region and has a brightness temperature of  ∼4 × 10⁵ K  . There are matching absorption features in mainline transitions of highly excited OH. The filament may trace a shock front in a rotating disc.  相似文献