火山喷发过程中岩浆脱气率和脱气量的估算方法及其意义

本文对前人使用的火山喷发过程中岩浆脱气率和脱气量的估算方法进行了评述,并介绍了如何利用岩石学方法估算火山喷发不同阶段岩浆脱气率和脱气量的具体步骤,同时以镜泊湖地区全新世火山为例说明利用该方法估算的具体过程。估算结果表明不同气体在火山喷发过程中的脱气率是不同的,不能用包裹体中挥发分相对含量的高低来判断火山喷发所释放到大气圈中的气体类型和质量。该方法对火山学的研究具有重要意义。     

长江口北支盐水倒灌的数值模型研究

20世纪80年代以来,国内对长江口盐水入侵进行了大量系统专门的研究,对长江口的盐水入侵规律有了一个比较基本的认识.但是,长江口特别是在南支及南北港的盐度变化规律极其复杂,主要有盐度的周日变化峰值与潮流变化关系不尽协调,落潮时盐度反而最大;盐度的纵向分布上游比下游高;盐度的半月变化峰值一般发生在小潮和寻常潮期间,而且各测点盐度峰值的发生时间不尽一致[1,2]等等.其中北支盐水向南支倒灌是引起长江口盐度变化异常复杂的主要原因[1-5].北支倒灌在长江口盐度变化中扮演了重要的角色,掌握北支倒灌是认识长江口盐水入侵规律特别是南支和南北港盐度变化规律的重要内容,同时也是长江口淡水咨源利用的一个重要方面.     

Impact of atmospheric parameters on the atmospheric Cherenkov technique

Atmospheric density profiles as well as several light absorption and scattering processes depend on geographic position and are generally time-variable. Their impact on the atmospheric Cherenkov technique in general (imaging or non-imaging) is investigated. Different density profiles lead to differences in Cherenkov light density of up to 60%. Seasonal variations at mid-latitude sites are of the order of 15–20%. The quest for improved energy calibration of Cherenkov experiments also shows the need for improved transmission calculations, taking all relevant processes into account and using realistic profiles of absorbers. Simulations including the scattering mechanisms also reveal the relevance of Rayleigh and Mie scattering for atmospheric Cherenkov experiments. Refraction and the differences between treating the atmosphere in plane-parallel or spherical geometry are also investigated.     

Optimal Design of TMD Under Long-Term Nonstationary Wave Loading

—Traditionally,the use of a tuned mass damper(TMD)is to improve the surviability of the pri-mary structure under extraordinary loading environment while the design loading condition is describedby either a harmonic function or a stationary random process that can be fully characterized by a powerspectral density(PSD)function.Aiming at prolonging the fatigue life of an offshore platform,this studyconsiders an optimal design of TMD for the platform under long-term nonstationary loading due tolong-term random sea waves characterized by a probabilistic power spectral density(PPSD)function.Inprinciple,a PPSD could be derived based on numerous ordinary PSD functions;and each of them is treat-ed as realization of the corresponding PPSD.This study provides a theoretical development for theoptimal TMD design by minimizing the cost function to be the mean square value of the expectedlong-term response.A numerical example is presented to illustrate the developed design procedure.     

232 MHz太阳爆发与日冕物质抛射

利用综合孔径射电望远镜在 ２３２ ＭＨｚ观测太阳,具有 ３·８’的空间分辨率、 ２０ ｍｓ 的时间分辨率和高灵敏度及很好的抗干扰能力．１９９９年共观测到１２次大爆发,其中８次与日冕物质抛射相关．可以利用米波射电爆发预报ＣＭＥ事件．     

关于OH/IR星的质量损失率计算公式的讨论

利用几种不同的半经验公式计算一批OH／IR星的质量损失率,并通过比较计算结果来讨论所用的公式．在一些情况下,计算质量损失率必须先给定气尘比．通过计算出样品星的气尘比,并讨论气尘比的变化情况,以修正由尘埃质量损失率到总质量损失率的关系式．     

近相接双星室女座BF的轨道周期变化

收集了近相接双星ＢＦ Ｖｉｒ的光极小时刻,并对其轨道周期进行分析。结果表明该星的轨道周期在长期减小的财时也含有３０年的周期性变化,对引起轨道周期变化的各种物理机制的分析研究表明：一个质量为０．２８１Ｍ⊙、绕公共质心的轨道半径为１０．２ＵＡ的第３天体的存在能对轨道周期的周期性变化成份作出解释,如果轨道周期的周期性变化成份是由于次子星的周期性磁活动引起,那么系统总光度就应该有振幅０．０９７Ｌ⊙的周期性     

The K-band luminosity function of nearby field galaxies

We present a measurement of the K -band luminosity function (LF) of field galaxies obtained from near-infrared imaging of a sample of 345 galaxies selected from the Stromlo-APM Redshift Survey. The LF is reasonably well fitted over the 10-mag range −26 M _K −16 by a Schechter function with parameters α =−1.16±0.19, M *=−23.58±0.42 and φ *=0.012±0.008 Mpc⁻³, assuming a Hubble constant of H ₀=100 km s⁻¹ Mpc⁻¹. We have also estimated the LF for two subsets of galaxies subdivided by the equivalent width of the H α emission line at EW(H α )=10 Å. There is no significant difference in LF shape between the two samples, although there is a hint (∼1 σ significance) that emission-line galaxies (ELGs) have M * roughly 1 mag fainter than non-ELGs. Contrary to the optical LF, there is no difference in faint-end slope α between the two samples.     

1950年以来汾河水沙演变规律及影响因素分析

利用汾河河津水文站1950 年以来的水文资料, 应用多种统计分析方法, 系统分析了汾河水沙的季节及年 际变化规律, 并且对人类活动导致的年径流变化影响进行了估算。研究表明, 汾河流域水沙年内分配极不均匀, 年 内不均匀系数有明显上升趋势, 且越到近期稳定程度越低。水沙的年际变化剧烈, 且在20 世纪80 年代之后年径流 基本都是枯水时段。应用累积滤波器对汾河水沙变化趋势进行分析, 结果显示, 汾河流域水沙均呈减少趋势, 且泥 沙变化幅度大于径流变化。通过降水—径流双累积曲线及对天然径流的还原分析表明, 径流变化趋势在1964 年发 生明显偏离, 从多年平均值来看, 人类活动导致的径流减少量占径流减少总量的75.912%, 人类活动是汾河流域径 流减少的主要因素。