川渝地区夏季降水变化气候特征分析

利用川渝地区34站1960—2006年共计47年的逐月降水量资料,采用经验正交函数（BOF）分解、旋转经验正交函数（REOF）分解、小波分析等方法详细讨论了川渝地区夏季降水量的时空变化特征。结果表明：川渝地区夏季降水量时空分布不均,川渝地区夏季降水量可以分为3个区,分别是川西高原区、盆地中部区和盆地东部区。近50年来,川渝地区夏季降水量具有显著不同的年代际变化特征,川西高原和盆地东部夏季降水量长期变化呈增加的趋势,而盆地中部呈减少的趋势。川渝各区夏季降水量具有显著不同的多时间尺度的周期变化特征,其中川西高原具有准15年和准5年的周期变化特征,盆地中部具有准14年、准6年和准3年的周期变化,盆地东部具有准16年、准8年和准3年的周期变化特征。     

A Case study of a snowstorm at the Great Wall Station,Antarctica

A case of a snowstorm at the Great Wall Station was studied using data of NCEP (National Centers for Environmental Prediction) analysis, in situ observations and surface weather charts. The storm occurred on August 29th,2006, and brought high winds and poor horizontal visibility to the region.It was found that the storm occurred under the synoptic situation of a high in the south and a low in the north. A low-level easterly jet from the Antarctic continent significantly decreased the air temperature and humidity.Warm air advection at high level brought sufficient vapor from lower latitudes for the snowstorm to develop.The dynamic factors relating to strong snowfall and even the developmentof a snowstorm were deep cyclonic vorticity at middle and low levels,the configuration of divergence at high level and convergence at low level, and strong verticaluplift. There was an inversion layer in the low-level atmosphere during the later phase of the storm.This vertical structure of cold air at low levels and warm air at high levels may have been important to the longevity of the snowstorm.     

赣西北地区P波S波随频率衰减关系研究

利用2009-01—2013-05月发生在赣西北地区的233次M L≥1.0地震数字波形资料,采用尾波归一化方法计算了阳新台、九江台、修水台、高安台、宜春台的P波S波的衰减,结果显示,除修水台最佳流逝时间约为60 s外,其他四个台站的最佳流逝时间为30 s左右;九江-瑞昌震区内平均P波和S波的Q值分别为:Q P(f)=(15.97±1.87)f(1.66±0.06)和Q S(f)=(25.27±1.90)f(1.15±0.04)。     

Status of the Recent Declining of Arctic Sea Ice Studies

In the past 30 years, a large-scale change occurred in the Arctic climatic system, which had never been observed before 1980s. At the same time, the Arctic sea ice experienced a special evolution with more and more rapidly dramatic declining. In this circumstance, the Arctic sea ice became a new focus of the Arctic research. The recent advancements about abrupt change of the Arctic sea ice are reviewed in this paper .The previous analyses have demonstrated the accelerated declining trend of Arctic sea ice extent in the past 30 years, based on in-situ and satellite-based observations of atmosphere, as well as the results of global and regional climate simulations. Especially in summer, the rate of decrease for the ice extents was above 10% per decade. In present paper, the evolution characteristics of the arctic sea ice and its possible cause are discussed in three aspects, i.e. the sea ice physical properties, the interaction process of sea ice, ocean and atmosphere and its response and feedback mechanism to global and arctic climate system.     

逆康普顿散射对中等银纬区银河弥漫γ射线的贡献

使用最近期的ＧＲＯ库中ＥＧＲＥＴ的γ射线数据，研究了逆康普顿散射对中等银纬区银河弥漫γ射线的贡献。采用了两种分析方法：其一为本文的新分析方法，其中银河宇宙与星际气体相互作用的γ射线的发射率ｑ／４π由γ射线数据本身确定；其二为通常的分析方法，即ｑ／４π由使用了局部银河宇宙线强度的观测值的理论估计给出。通过分析，我们获得了两种方法中逆康普顿散射的贡献与能量的依赖关系。结果表明，逆康普顿散射的贡献是大的。     

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.     

A possible explanation for the electron/positron excess of ATIC/PAMELA

Results from PAMELA and ATIC indicate that the Kaluza-Klein type dark matter particles could be the annihilation source of the observed excess of electrons and positrons.Assuming the existence of a nearby black hole with 10000–100000 solar masses and a point source boost algorithm,we apply the standard propagation model and find that the results fit the data well.     

疏散星团M11的研究:4.CM图、光度函数和分层效应

利用上海天文台 40cm天体照相仪底片资料所提供的疏散星团M1 1天区 (团心距r≤2 5′)内的 785颗恒星的相对自行和成员概率 ,讨论了M1 1的CM图、年龄、距离、半径、光度函数、质量和分层效应 ,得到M1 1的距离为 1 659pc ,年龄为 (1 .8— 2 .2 )× 1 0 8年 ,半径约为 2 4 .5pc ,光度质量 4354M⊙ ,位力质量 50 0 0M⊙ ,在确定光度函数时 ,提出了一种考虑样本天区不完备的修正办法 ,以便从观测光度函数导出现时光度函数 .分析表明 ,作为一个中等年龄的疏散星团 ,M 1 1中的团星已表现出较明显的空间质量分层效应 ;而另一方面 ,尽管存在速度质量分层效应 ,但很不明显     

桑塔木地区三叠系曲流河三角洲存在证据与沉积特征

为了厘清桑塔木地区三叠系砂体成因类型,指导油气勘探,利用岩心、钻测井、分析化验及高精度三维地震资料,研究碎屑岩的粒度、结构、沉积构造、砂体的空间展布、地震反射特征等.结果表明:三叠系TⅡ油组具有粒度细、分选磨圆好、发育小型交错层理、波状层理及水平层理,呈指状产出,地震剖面上具有前积反射构型,典型相干体地层切片见曲流特征的特点,是典型的曲流河三角洲沉积;同时,研究区曲流河三角洲发育2种亚相6种微相,其中平原亚相发育天然堤、水上分流河道及河漫沼泽微相,前缘亚相发育水下分流河道、河口坝和支流间湾3种微相;区内TⅡ油组以发育北部和西南部2个主要方向的曲流河三角洲为主,其中北部三角洲规模大,平原和前缘亚相较发育,西南部三角洲以前缘亚相为主,平原亚相以分流河道沉积为主,前缘亚相主要发育分流河道和河口坝微相.该三角洲的形成与地形坡度及气候的变化密切相关.     

MCM-41/β介孔—微孔复合分子筛的合成、表征及催化性能

以β分子筛为前驱体,水玻璃和硫酸铝为外加硅铝源,采用二元混合表面活性剂为结构导向剂,水热晶化合成MCM-41/β介孔—微孔复合分子筛,并利用XRD、SEM、TEM、N2吸附—脱附和Py-IR等对复合分子筛进行表征,以十氢萘为模型化合物考察复合样品的催化裂解反应性能.结果表明:MCM-41/β介孔—微孔复合分子筛中存在MCM-41分子筛六方介孔结构和β分子筛微孔结构,对十氢萘具有较强的催化反应活性,催化裂解转化率为93.16%.