地球同步轨道附近哨声湍流对“种子电子”的加速

本文在等离子体准线性理论下研究了地球同步轨道附近哨声湍流对亚暴“种子电子”的波-电子共振相互作用. 当发生这种共振时，“种子电子”的动量分布函数经动量扩散而随时间演化，部分低能电子数减少了，而高能尾部分的相对论电子（能量大于1MeV）数增加了，说明“种子电子”得到了哨声湍流的有效加速，且哨声湍流的能量越高，其加速效率越高. 另外，哨声湍流的频率越低（或波数越小），共振电子的能量越高（或单位质量的动量越大）；频率范围越宽，共振电子的能量范围越宽，被加速的电子数也越多. 磁层哨声湍流加速“种子电子” 大约在30h内就可以造成相对论电子数显著增加，这正好和大多数磁暴期间观测到的相对论电子通量的增长时间相当.     

云南楚雄盆地波动特征及构造沉积演化

云南楚雄盆地是扬子板块西南缘的中新生代含油气盆地, 具有复杂的构造、沉积演化历史.应用沉积波动过程分析方法, 研究了楚雄盆地演化过程中的主要周期, 得出楚雄盆地存在3个一级沉积波动周期(2 2 0Ma)、6个二级沉积波动周期(1 0 0Ma)、9.5个三级沉积波动周期(4 5Ma) 以及高频波动周期(1 0Ma、5Ma).通过对不同波动单元的波动曲线对比, 得出楚雄盆地构造沉积演化规律: 在古生代沉积中心位于盆地东部的云龙凹陷; 中生代早期, 沉积中心具有自西南向东北, 由盆地边缘向中心迁移的规律, 晚期受构造运动影响, 沉积中心有自东北向西南回迁的趋势.      

近45年拉萨深层地温变化趋势分析

利用1961—2005年拉萨0.8 m, 1.6 m和3.2 m逐月平均地温, 采用气候倾向率、累积距平、信噪比等气候诊断方法, 分析了近45年拉萨深层平均地温的变化趋势, 以及异常、突变等气候特征。结果表明:近45年拉萨0.8 m和1.6 m年平均地温呈极显著的增温趋势, 倾向率为 (0.58~0.69 ℃)/10a;0.8 m和1.6 m平均地温倾向率春季最大, 秋季最小; 3.2 m平均地温却以夏季升幅最大, 冬季最小; 与同时期平均气温的增温幅度比较, 地温增幅更大; 20世纪60—90年代0.8 m和1.6 m年平均地温呈明显的逐年代升高趋势; 季平均地温20世纪60—70年代均偏低, 80年代大部分季节仍略偏低, 90年代都表现为正距平; 0.8 m, 1.6 m和3.2 m年平均地温均在1999年出现了异常偏暖, 异常偏冷现象仅发生在1.6 m土层上, 时间为1963年; 夏季深层平均地温异常偏暖均发生在1999年; 冬季0.8 m和1.6 m平均地温多异常偏冷年份, 主要发生在20世纪60年代; 1999, 2002—2005年冬季3.2 m平均地温异常偏暖; 夏、秋季和年平均地温的气候突变都出现在1986年, 冬、春季发生在1983年。     

SIMULATION OF HEAVY RAINFALL IN THE SUMMER OF 1998 OVER CHINA WITH REGIONAL CLIMATE MODEL

The heavy rainfall in the summer of 1998 over China has been simulated with the NCCRegional Climate Model(RegCM_NCC).It was successful for RegCM_NCC to reproduce thelocation and seasonal shift of the seasonal rain belt in the summer of 1998 over China.The rainyseason in the summer of 1998 over China can be divided into 7 episodes,including the pre-summerrainy season in South China.the Meiyu onset over the Yangtze-Huaihe River Basin,shortappearance of North China rain season and the retreat of seasonal rain belt,the second Meiyuseason over the Yangtze River Valley,the rainy period over the Yellow and Huaihe River Valleyand the seasonal retreat of rain belt over North China.The shortcoming of the RegCM_NCC isover-estimation of precipitation amounts.The regions with large latent heat flux,upper soilmoisture and total runoff are located in the rainy area and move with the simulated rain belt duringthe different episodes.On the contrary,the regions with small sensible heat flux are located in thesimulated rainy area and move with the simulated rain belt during the different episodes.     

RESPONSES OF A GLOBAL CGCM TO CO_2 INCREASE

The responses of the climate system to increase of atmospheric carbon dioxide(CO_2)arestudied by using a new version of the Bureau of Meteorological Research Centre(BMRC)globalcoupled general circulation model(CGCM).Two simulations are run:one with atmospheric CO_2concentration held constant at 330 ppm,the other with a tripling of atmospheric CO_2(990 ppm).Results from the 41-year control coupled integration are applied to analyze the mean state,seasonal cycle and interannual variability in the model.Comparisons between the greenhouseexperiment and the control experiment then provide estimations of the influence of increased CO_2on climate changes and climate variability.Especially discussed is the question on whether theclimate changes concerned with CO_2 inerease will impact interannual variability in tropical Pacific,such as ENSO.     

IAP GCM模式大气波谱结构及其在厄尔尼诺年的异常

本文分析了中国科学院大气物理研究所大气环流模式(IAP GCM)模式大气波谱结构(沿纬圈的谐波波谱和时域上的频率谱)及其在厄尔尼诺年的异常。结果表明,超长波是低纬波动的主要空间形式,准40天振荡在一定地理区域内显著存在,并与观测结果有一定联系,它们在厄尔尼诺年均发生明显异常。本工作对鉴定GCM性能及开发GCM的研究领域可能是一种有益的尝试。     

IAP GCM模式大气背景环流在厄尔尼诺年的异常

本文分析了中国科学院大气物理研究所大气环流模式(IAP GCM)模式大气5～9月平均环流(本文称为背景环流)。结果表明;厄尔尼诺年一系列重要系统(南方涛动、瓦克环流、哈德莱环流、西太平洋副热带高压和热带辐合带)及大范围降水均发生明显异常;北半球西太平洋热带、副热带是环流异常的主要区域。它们与观测资料的分析结果基本一致,从而论证了该模式在低纬环流研究中的应用前景。     

ARTIFICIAL NEURAL NETWORK CORRECTION OF ROUGH ERRORS OF OBSERVATIONS

In the context of tower measured radiation datasets.following the correction principle meetinga diagnostic equation in data quality control and in terms of a technique for model construction ondata and ANN(artificial neural network)retrieval for BP correction of radiation measurementswith rough errors available,a BP model is presented.Evidence suggests that the developed modelworks well and is superior to a convenient multivariate linear regression model,indicating its wideapplications.     

A Probable Short Decimetric Type Ⅰ-like Noise Storm: Associated with Type Ⅲ Bursts?

A rare Type I-like noise storm was observed with the solar radio spectrometers (1.0-2.0 GHz and 2.60-3.8 GHz) at National Astronomical Observatories of China (NAOC) on September 23, 1998. We concentrate on checking the Type I-like noise storm occurred in the decay phase of a Type Ⅳ radio burst. This noise storm consists of many Type I bursts and isolated Type Ⅲ or Type Ⅲ pair bursts. It has a bandwidth of ≤0.5 GHz. The duration of each Type I burst is of the order of 100-300 ms. The total duration is greater than 11 minutes. The circular polarization