A theoretically derived energy coupling function for the magnetosphere

The energy coupling function between the solar wind and the magnetosphere can be obtained for two extreme situations, in which the magnetospheric geometry is determined primarily by either (i) the interplanetary magnetic field, or (ii) the solar wind pressure. In this paper, we obtained an expression for the energy coupling function by assuming a simple interpermeation of the interplanetary and geomagnetic fields. Two important quantities in this case are the potential difference between the two neutral points and the amount of open flux. From these two overall quantities, the voltage and the current of the magnetospheric dynamo are calculated. The dynamo power output represents the rate at which energy is transferred from the solar wind to the magnetosphere. The derived functional dependence on the interplanetary conditions provides a theoretical basis for the energy coupling function previously deduced from observations.     

Particle dynamics in reconnection field configurations

Trajectories of test particles are studied numerically in two types of reconnection magnetic field configurations, a single X-line magnetic field configuration and a tearing magnetic field configuration. Both adiabatic and nonadiabatic motions are examined, with special emphasis on net energy gain and time spent in the neutral line regions. They spend typically one characteristic gyroperiod in the X-line region and are ejected predominantly along field lines in the vicinity of the separatrix. Both adiabatic and nonadiabatic test particles in the tearing-type field configuration are channelled into and accelerated along the O-line region. It may be inferred from these test particle results that particle energizations are significant along the O-line region, but not along the X-line region. These results are in qualitative agreement with those obtained by a self-consistent particle simulation.     

On the mechanisms producing the backscattered and the trapped electrons along auroral field lines

The production mechanisms of backscattered electrons and trapped electrons along auroral field lines are examined. The backscattered electrons are produced not only by electron-neutral collisions, but also by electrostatic turbulence predominantly in the ion-cyclotron and ion-acoustic modes. The trapped electrons can only be produced by electron wave turbulence, most likely in the whistler and upper hybrid modes known as the auroral hiss.     

Environmental impact of drainage of Dianzi Iron Mine on the groundwater system of the Dawu Water Supply Base

Due to growing water extraction for industry and agriculture, the Dawu Water Supply Base, in the east of Zibo, China, has been in a state of serious over-extraction. It will also be affected by the deep drainage of the Dianzi Iron Mine, which will be exploited in 2005. As to the environmental impact on the groundwater system of the Dawu Water Supply Base is concerned, this paper makes a systematic study about the influence of the mine draining on the water-supply environment of the Dawu Water Supply Base by using the numerical model of groundwater system. The result shows that the groundwater level will have an additional drawdown of 1.2–1.8 m/yr by the mine draining alone. The numerical analysis results indicate that the optimal model for determining the best extraction plan is the solution for the contradiction between water supply and water drainage.     

PPGIS实现的难点探讨

大众参与地理信息系统(PPGIS)属于GIS技术应用之一,主要强调普通民众的群体参与,以帮助政府、规划等职能部门更好地进行决策和计划。本文着重从技术、公众权利保障性、数据三个方面论述了实现PPGIS项目中主要的难点和核心问题。     

海高斯”登陆海南西藏遭遇强降雪——2008年10月——

10月,全国平均气温较常年同期偏高1.1℃,平均月降水量较常年同期偏多6.4mm;上旬,0817号台风海高斯先后登陆海南和广东,部分省出现暴雨灾害;上中旬,东北、江南、西南及内蒙古等地的部分地区气象干旱发展;下旬,全国遭遇大范围降温,其中西藏遭遇强降雪天气;此外我国东部和南部的部分地区出现大雾天气.     

风电场风资源测量与计算的精度控制

根据多个复杂地形风电场观测操作实践和大量观测数据的计算分析,提出了对观测数据和计算质量精度控制的主要措施,包括:复杂地形测风站布设的5个原则,仪器的合理选型和设置;对由于测风仪固有的系统误差和缺测数据的插补订正可能引起的计算误差进行了定量估算,通过对大量实测数据的对比计算显示:①目前普遍采用的进口风速计的相对偏差在1.6%～5.25%之间,由此可导致轮毂高度附近的年平均风功率密度误差在5%以上,最大达13.8%;②在季风气候区、复杂地形和风的年变率较大的地区,进行缺测数据插补订正时,应选取同季或同一主导风向的数据作为插补订正的基础数据,否则可能导致其平均风功率密度相对误差达20%～50%.     

登陆热带风暴Bilis（2006）暴雨特征及其可能原因

利用NCEP/NCAR 1°×1°格点再分析资料、FY-2C TBB（black bright temperature）资料及中国740站降水资料,对0604号强热带风暴Bilis登陆后的暴雨特征及其可能原因进行诊断分析,结果表明：（1）Bilis登陆过程中强降水中心位于风暴中心西北侧沿岸,主要影响福建和浙江两省;进入内陆后强降水中心向风暴中心以西转移,最后在风暴中心西南侧聚集,主要影响广东东北部、福建、江西和湖南南部。（2）西北太平洋副热带高压的稳定少动为Bilis陆上西行过程中产生持续性降水提供了稳定的背景场。（3）Bilis西南部季风环流的发展增强为Bilis登陆后强降水的产生提供了必要的水汽条件。（4）涡合并和自激增长形成的中尺度系统与风暴涡旋的相互作用,是Bilis登陆后产生强降水的可能机制。     

全球气候模式对宁夏区域未来气候变化的情景模拟分析

利用多个全球气候模式(GCM)的情景模拟结果分析只考虑温室气体效应的IS92a GG情景和同时考虑温室气体效应和硫化物气溶胶辐射效应的IS92aGS情景以及SRESA2、B2情景下宁夏区域21世纪地面气温和降水量的可能变化,并进行不确定性分析。气候基准时段(1961~1990年)模拟结果与观测资料的对比分析表明,GCM对宁夏气候具有一定的模拟能力;整体上讲,GCM对地面气温的模拟值偏低,对降水量的模拟值偏高,其中ECHAM4和HadCM3对宁夏基准时段地面气温和降水量的模拟结果与观测比较接近。各GCM模拟值的平均结果显示,4种温室气体排放情景下21世纪宁夏区域气温持续升高,至21世纪末宁夏升温幅度可达4~6℃,与全国平均的增温幅度大致相当;与升温趋势相应的是降水量的增加,但降水变化呈现出很大的波动性,至21世纪末宁夏的降水变化幅度可达10%~40%。各个GCM模拟的宁夏气候变化的总趋势是一致的,但各模式在不同情景下模拟结果的差异很大,存在较大的不确定性。     

南极采用飞艇进行航空摄影测量的可行性探讨

随着我国对南极科考工作的加强,迫切需要新的高精度的地形图资料。而由于南极特殊地域的限制,要求作业时间要尽可能地短,基于这种情况,在南极两站地区采用飞艇航摄手段获取高精度的两站地形图将成为最佳的可行手段。