基于MapInfo的地质变量自动化选择与赋值

在GIS中实现地质变量选择与赋值的自动化可以显著提高GIS矿产预测工作的效率 ,同时也为实现GIS矿产预测全程自动化提供了技术前提。不同软件平台所提供的“二次开发”环境不尽相同 ,考虑软件平台的实用性、软件价格高低及其二次开发环境的好坏等因素 ,选择MapInfo作为基础平台 ,研究了在该平台内自动选择地质变量并对其赋值的计算机算法 ,用平台的“二次开发”语言MapBasic编制了算法的计算机程序。     

QK-100型多功能全液压取样钻机的研制

QK-100型多功能全液压取样钻机是为满足我国厚覆盖地区地质填图取样而研制的。介绍了该钻机的技术参数、性能特点、主要结构以及试验试制情况。     

隧道衬砌随机分析的区间有限元法

隧道衬砌结构内力计算中,围岩的力学参数和结构的参数具有不确定性,同时,其不确定性是有界的。对于这些参数的不确定性,在工程上可以用一个合理的区间数值来估计。对于单个随机变量,可以采用有限元方程来求解结构内力;而对于多个随机变量的情况,考虑到计算模型的不确定性和数学求解的复杂性,利用有限元程序来导出各变量对结构内力的作用效应,进而得到不同参数组合的区间值,最终确定隧道衬砌的结构内力区间值,为隧道衬砌结构内力的计算和工程应用提供一种新方法。     

Rapid oscillations of five stars in the spectral range G and K. II

The five stars HD 11112, HD 170747, HD 186651, HD 205390 and HD 224834 are a second group of objects enclosed in a larger observational programme for the search of rapid oscillations. They have been observed with the 50 cm photoelectrical ESO telescope at La Silla (Chile). For the star HD 205390 a variation of 163.8 min was found. The two objects HD 11112 and HD 186651 are suspected to be variable with periods of 139 min and 142.2 min and its overtones, respectively. But a verification of these results is necessary. For the last two objects HD 170747 and HD 224834 no variations were detected.     

A new suspected apsidal period for HS Herculis

From a preliminary analysis of observed minima of the eclipsing binary HS Herculis, a new apsidal period is postulated. A general possible error in Oapsidal period is emphasized.     

Rapid oscillations of five stars in the spectral range A and F. I

The five stars HD 4849, HD 24712, HD 182475, HD 184552 and HD 215874 are a small group of objects enclosed in a larger observational programme for searching of rapid oscillations. They have been observed with the 50 cm ESO-telescope at La Silla (Chile). These objects are characterized as a suspected δ Scuti-type star, an Ap star, an A9 V star, an A1m star and an A9 III-IV star, respectively. For the first two stars the periods, dedected by other authors, were confirmed. For HD 182475 a period of 112.3 min has been estimated. In the case of HD 184552 an oscillation with a period of 163.3 min has been found. The star HD 215874 shows unambiguously a variation with a period of 97.2 min.