西澳大利亚皮尔巴拉地块诺思波勒地区太古宙燧石-重晶石矿床的沉积环境

在诺思波勒(North Pole)地区,有一个燧石-重晶石岩石单位,属皮尔巴拉地块东部瓦拉沃纳(Warrawoona)群(3500—3400Ma)的最下部沉积夹层,该群主要为超镁铁-镁铁火山岩岩系。该岩石单位包括四种沉积岩类型:硅化碳酸盐岩、硅化和重晶石化蒸发硫酸盐、原生硅质沉积物变质后的条带状燧石、以及硅化火山碎屑沉积岩。硅化碳酸盐岩,呈砂粗碎屑岩至细屑岩韵律,或呈含有少量层间碎屑砾岩的细屑岩     

铀矿石中钍的离子交换-光谱测定

本文提出了以离子交换与光谱分析相结合测定1克铀矿石中0.01ppm钍的方法。在盐酸和硝酸介质中进行阴离子交换,将钍从化学组成复杂的矿石溶液中分离出来,以锆作内标进行光谱测定。方法的精密度以变差系数表示,估计为±6％。     

东亚地区沙尘气溶胶影响硫酸盐形成的模式评估

利用STEM-II三维区域大气化学模式,耦合沙尘气溶胶表面相过程,研究了1994年3月1日至14日间东亚地区沙尘气溶胶对硫酸盐形成的影响。结果表明,SO2气体在沙尘气溶胶表面上进行的非均相氧化过程是硫酸盐形成的一条重要途径,由这条途径提供的硫酸盐占其总浓度的20%～50%。 并发现在模拟时段,沙尘暴过程主要影响沙尘源地下游的中国东部地区硫酸盐的分布,使得那里的硫酸盐浓度增加60%以上。     

八十年代气象雷达发展展望

一、现状当七十年代开始的时候,多普勒雷达才刚刚开始成为一种可行的定量研究工具。现在多普勒雷达已不再是一种稀奇的东西,它已经达到了非相干雷达的同等地位,成为众所公认的气象探测工具。数字计算机和集成电路的迅猛发展,对于多普勒     

热带气象学——其经济意义及科学任务

载于《世界气象组织公报》1975年7月号。近年来,不管实用方面或科学方面都越来越着眼于热带气象的重要性.在实用方面,农业和水力资源的利用越来越需要热带气象观测资料以及几个月以上的长期天     

在6厘米波长对类星体3C454.3的九站VLBI观测

3C454.3是近几年引起广泛注意的一个强活动射电类星体,它有毫角秒尺度的核——喷流结构,其核在1981年的一次流量密度大爆发之后,显示出“超光速增亮”现象,在6厘米波长,用包括欧洲、美国及南非的9个射电望远镜,于1983年10月对3C454.3进行了甚长基线干涉网观测。观测结果除了证实其核——喷流结构,显示了从毫角秒到角秒尺度上该类星体结构的系统弯曲外,还清楚地揭示了“超光速增亮”所预期的,在1981年8月到1983年1月期间,核的超光速膨胀现象。     

Use of Surface Observations to Estimate Upper Air Humidity for the Objective Analysis of Relative Humidity over Indian Region

In the present study objective analyses of relative humidity (RH) at surface and at the levels of 850,700 and 500 hPa have been made using Gandin’s (1963) optimum interpolation scheme. As the horizontal resolution of the radiosonde stations is rather inadequate for upper air humidity analysis, a scheme has been developed, following Rasmussen (1982) to estimate the upper air RH from the surface observations like surface RH, present weather and cloud cover. The relative humidities at the levels 850, 700 and 500 hPa were related to the surface observations through three separate regression relations. The RH values at 850, 700 and 500 hPa levels were estimated from the surface RH, cloud coverage and present weather using the above regression relations and subsequently the objective analyses at 00 GMT for the period from 4 July to 8 July 1979, were made using these estimated data along with the observed radiosonde data. Objective analyses were also made for the same period using only the radiosonde data for comparison to study the impact of those estimated data. Root mean square errors were computed for all the five days by interpolating RH at the observing stations from the objectively analysed field and comparing them with the actually observed RH to examine how best the analyses (with and without estimated data) fitted the observations. Lastly they were compared with satellite cloud pictures. This study shows that the estimated upper air RH values have positive impact on the analysis of upper air RH and could be used over radiosonde date sparse region and even over oceanic regions.     

Global Annual Mean Surface Air Temperature Anomalies and Their Link with Indian Summer Monsoon Failures

Analysis of the global mean annual temperature anomalies based on land and marine data for the last 88 years (1901-1988) of this century has been carried out with a view to find any relationship with failures in Indian summer monsoon rainfall. On the climatological scale (i.e. 30 years) it has been noticed that there is an abnormal increase in the frequency of drought years during epochs of global warming and cooling, while it is considerably less when global temperatures are near normal. Results are unchanged even when the data are filtered out for ENSO (El-Nino Southern Oscillation) effect.It has also been noticed that during warm and cold epochs in global temperatures the amount of summer monsoon rainfall decreases as compared to the rainfall during a normal temperature epoch.     

Velocity Curve Analysis of Spectroscopic Binary Stars AI Phe, GM Dra, HD 93917 and V502 Oph by Nonlinear Regression

We introduce a new method to derive the orbital parameters of spectroscopic bi-nary stars by nonlinear least squares of (o-c). Using the measured radial velocity data of the four double lined spectroscopic binary systems, AI Phe, GM Dra, HD 93917 and V502 Oph, we derived both the orbital and combined spectroscopic elements of these systems. Our numerical results are in good agreement with the those obtained using the method of Lehmann-Filhe's.     

勘查贱金属硫化物的电化学方法

继近几年来苏联使用的称为“CHIM—10”的野外勘探技术以来,一种基于电化学原理的利用原有设备的方法已用于寻找贱金属硫化物。这个方法利用了金属离子的正电性质,当大片土壤由于输入直流电而被人工电离时,靠近矿化带的潮湿土壤剖面中的金属离子势必会朝大功率大间隔电极系中的阴极运动。首先,进行了实试室模型试验,试验取得了振奋人心的结果。随后,组装了野外试验设备并用于在野外检验它的有效性。试验土壤剖面位于卡纳塔克邦哈桑县Aladahalli地区的贱金属硫化物带上,这里的矿床地质情况是众所周知的。在野外试验中获得的结果相当令人满意,并且与已知的地质情况完全一致。然而,在对该系统不同的可变参数做了必要的改正以后,仍然要对那些数据做细致的评价。以标准化和开发应用为目的,改进方法的工作正在进行,以便定性和定量评价给定地区的隐伏贱金属矿床,尤其是在那些常规地球化学勘查方法不适用的地方。本文论及该方法的细节并讨论在野外试验中所获得的结果。