地形动力作用对华北暴雨和云系影响的数值研究

为了进一步研究地形对华北暴雨的影响,本文从云微物理学的角度出发,选取了2005年7月22～24日的一次华北暴雨过程为研究对象,利用中尺度数值模式ARPS,通过地形高度敏感性试验,详细讨论了地形高度变化对流场、云及降水微物理过程的影响.结果表明:地形高度变化对水平和垂直流场的大小和分布都有较大影响;地形高度增加有利于迎风坡附近水平风场辐合和垂直上升运动发展,这对云的垂直和水平发展影响都很大,尤其是对中高层云的发展影响最明显,并且能明显扩大地面降水的分布范围,地面最大降水量也有所增多.这主要是由于地形高度增加后能促进中高层云水的产生,尤其是零度层之上的过冷云水含量的增多,这大大促进了冰相粒子(雪和霰)的增多,从而使得以冷云过程为主的此次降水过程中,冰相粒子融化形成的雨水含量增多.虽然地形高度的增加会抑制云系发展前期的暖云过程,但对冷云过程有持续加强作用,而且不会明显改变云内降水的形成机制,冷云过程依然是降水的最大贡献项,总体上促进了云和降水的发展.     

冬春季切变类冰雹发生条件的对比分析

本文以 1996年 12月 31日和 1981年 5月 1日为例 ,对冬、春季节发生在江苏的较大范围的切变类冰雹天气过程作了对比分析。结果指出 ,无论冬季或春季当高原东部有深槽东移 ,冷暖空气在江淮地区交汇 ,地面抬升系统为暖切 ,并有大气层结不稳定 (Δθse( 50 0 - 850 ) <0℃ =中心和较强的风向和风速垂直切变、85 0hPa西南急流轴、85 0hPa最大水汽通量轴线、5 0 0和 85 0hPa正涡度中心等相配置时 ,就可能导致江苏地区较大范围强对流天气的发生。     

基于审查回归模型的公众气象服务支付意愿影响因素分析——以无锡、武汉和西安为例

采用审查回归模型,分别选取了中国东、中、西部的三个典型城市无锡、武汉和西安,计算了三城市受访者的支付意愿值,并对其影响因素进行了分析。结果表明：（1）支付意愿值与地区经济发展水平直接相关。无锡、武汉和西安受访者的支付意愿分别为21.68,17.15和10.07元/年;（2）年龄越长者,由于其天气知识更丰富、日常消费较节俭,对气象服务的支付意愿越低;（3）文化程度越高者,更能理解和支持气象服务事业,对气象服务的支付意愿越高;（4）月收入变量对气象服务的支付意愿有显著影响,但就不同城市的受访者而言,影响的方向并不一致。     

Simulation Study on High Energy Cosmic Electron Detection by Shower Image

Many projects have recently been carried out and proposed for observing high energy electrons since it is realized that cosmic ray electrons are very important when study-ing the dark matter particles and the acceleration mechanism of cosmic rays. An imaging calorimeter,BETS (Balloon-borne Electron Telescope with Scintillator fiber),has been de-veloped for this purpose. Using pattern analysis of the shower development,the electrons can be selected from those primary cosmic ray proton events with flux heights one-tenth that of the electrons. The Monte-Carlo simulation is indispensable for the instrument design,the sig-nal trigger and the data analysis. We present different shower simulation codes and compare the simulation results with the beam test and the flight data of BETS. We conclude that the code FLUKA2002 gives the most consistent results with the experimental data.     

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未来北极夏季陆面气温变化区域特征及其与北大西洋海面温度的关系

未来变暖背景下北极气候变化特征研究具有重要意义,基于国际耦合模式比较计划第六阶段（Coupled Model Intercomparison Project Phase 6,CMIP6）中对北极气候变化模拟能力较好的模式模拟结果,研究SSP2-4.5情景下21世纪北极2 m气温的时空变化特征及其影响因素。结果表明：（1）极地陆地的欧亚大陆（Eurasia,EA）和北美-格陵兰（Greenland,GL）对全球变暖具有不同的响应。EA在21世纪中叶前变暖趋势显著,之后主要表现为年代际尺度的冷暖振荡;GL则始终保持增暖趋势。EA、GL分区气温均存在年际、年代际（10~20 a）尺度上的波动,GL分区还存在20~40 a的准周期变化。（2）前冬北大西洋涛动正位相会引起次年夏季北大西洋呈南北向“-、+、-”三极型海面温度异常,并通过影响大气环流导致EA分区气温正异常,这种影响主要体现在年代际尺度上。（3）北大西洋多年代际振荡为正异常时,北美至格陵兰位势高度偏高,GL分区增暖,并且这种影响在21世纪70年代后更重要;北太平洋北部的海面温度正异常对GL分区增温也有贡献。     

西藏洞错晚白垩世花岗闪长斑岩: 岩石圈拆沉的产物

班公湖-怒江缝合带是国内外备受关注的特提斯构造域的重要组成部分,可为恢复和反演特提斯洋构造演化提供重要依据。对南羌塘地块南缘洞错地区晚白垩世花岗闪长斑岩进行了详细的岩石学、锆石U-Pb定年、全岩地球化学和Lu-Hf同位素研究。锆石U-Pb定年和Lu-Hf同位素研究结果显示,该花岗闪长斑岩形成时代为74.1±1.1 Ma,εHf（t）值为4.5~6.9。全岩地球化学特征显示,其为高钾钙碱性系列,富集轻稀土元素,轻重稀土元素分馏较强,具弱负Eu异常;富集Rb、Th、U、K和Pb,亏损Ba、Nb、Ta、La、Ce、P和Ti。该花岗闪长斑岩为加厚新生下地壳部分熔融的产物。在综合区域最新研究成果的基础上,认为该花岗闪长斑岩形成于后碰撞环境,为班公湖-怒江洋闭合后岩石圈拆沉的产物。     

四川九寨黄龙机场高填方地基变形三维动力分析

四川九寨黄龙机场具有高填方、高地震烈度、高海拔等三高的特点,高填方体地基在地震作用下的动力稳定与变形问题成为该机场需着重考虑的主要工程地质问题之一。在对目前各种动力分析方法研究的基础上,选用快速拉格郎日差分分析(FLAC)程序,对该机场元山子沟段高填方地基在地震作用下的变形规律进行了系统地研究,获得了一些有实际意义的认识。     

High-precision repeat-groundtrack orbit design and maintenance for Earth observation missions

The focus of this paper is the design and station keeping of repeat-groundtrack orbits for Sun-synchronous satellites. A method to compute the semimajor axis of the orbit is presented together with a station-keeping strategy to compensate for the perturbation due to the atmospheric drag. The results show that the nodal period converges gradually with the increase of the order used in the zonal perturbations up to \(J_{15}\). A differential correction algorithm is performed to obtain the nominal semimajor axis of the reference orbit from the inputs of the desired nodal period, eccentricity, inclination and argument of perigee. To keep the satellite in the proximity of the repeat-groundtrack condition, a practical orbit maintenance strategy is proposed in the presence of errors in the orbital measurements and control, as well as in the estimation of the semimajor axis decay rate. The performance of the maintenance strategy is assessed via the Monte Carlo simulation and the validation in a high fidelity model. Numerical simulations substantiate the validity of proposed mean-elements-based orbit maintenance strategy for repeat-groundtrack orbits.     

Observational evidence for solar coronal decimetric radio pulsations with very short periods

Using the decimetric (700–1500 MHz) radio spectrometer and the synchronous observational system with high temporal resolution at four frequencies (1420, 2130, 2840 and 4260 MHz) of Yunnan Observatory, two rare events were observed on 2001 June 24 and 1990 July 30. The former was a small radio burst exhibiting pulsations with short periods (about 29, 40 and 100 ms) in the impulsive phase. The latter was a large radio burst, which at 2840 MHz produced radio pulsations with period of about 30 ms. This paper focuses on pulsations with very short periods in the range of 29–40 ms. The mechanism of generation of such pulsations may be modulation of radio radiation by the periodic trains of whistler packets originating in unstable regions of the corona. Alternatively, these pulsations can be attributed to wave-wave non-linear interactions of electrostatic upper hybrid waves driven by beams of precipitating electrons in flaring loops.