济宁市嘉祥县石灰岩矿山地质环境评价与治理

在对嘉祥县石灰岩矿进行地质灾害危险性评估、矿山环境地质问题评价的基础上,建立了一套评价体系,其中地质灾害危险性评估分为2个评价指标,矿山环境地质问题评价分为2种要素3个指标,同时将矿山恢复治理难易程度也作为一个评价因子。评价过程中对各指标危害性大、中、小程度均单独赋值,然后将各指标的分值进行叠加,确定出矿山环境地质问题的等级,将概划出的13个评价单元分为极差、差、一般3个区。提出了强化矿山管理、植树造林、科学避让、修建拦水坝等保护与治理措施及建议。     

南水北调中线初期引汉工程经济效益初探

南水北调是补充华北地区新水源的有效途径之一。“中线”初期引汉工程是从长江支流汉江调水,渠线跨越汉江、淮河、黄河、海河四大水系,直达北京市。引汉水源是丹江口水库。该库集流面积95200平方公里,多年平均年径流量380亿立米,已建成初期规模。坝顶高程162米,正常蓄水位157米,总库容174.5亿立米。     

克拉2大气田的发现与"西气东输"工程

改革开放以来,随着我国经济迅速发展,对能源,特别是对石油的需求急剧增加.2000年,我国年产原油1.62亿吨,进口原油达7,000万吨.据有关部门预测,2010年我国原油需求量为2.8亿吨,其中进口1亿吨.社会经济发展要求我国石油天然气供应有更快的增长,以减少对进口原油的依赖,保证国家经济安全.……     

On the Line Formation in Stellar Magnetized Atmospheres

1 INTRODUCTIONIn the previous paper (on et al. 1999, hereafter Paper I), we investigated the wavelength-dependence of four colltribution functions (CFs) derived from dmerent formal solutions andreferring to different emergellt quantities in the unpolarized case. Because one cannot generallyassign a single formation region to the whole line band in a real stellar atmosphere, e.g., the solaratmosphere, instead, the line formation region can be defined as the layers deviating farthestfrom t…     

Paleoproterozoic Extensional Structure and Its Controlling on Mineralization in the East of Liaoning Province

IntroductionThe area of eastern Liaoning is an importantmetal and nonmetal metallogenetic district in China,and the Liaohe group is one of the most importantstrata that hosts Pb, Zn, Au, B and Mg etcstratabound deposits. Up to now many geo1ogistssuch as Z…     

抗差估计的初值选择

对L1 范估计的平差值和LS估计的平差值作为抗差估计的初值进行了比较 ,指出在 ρ函数是严凸函数时 ,二者无明显的区别。因为LS估计简单且易于计算 ,因此建议用LS估计的平差值作为抗差估计的初值。     

On the influence of magnetic fields on level populations

The influence of magnetic fields on the energy level populations of atoms is firstly studied by analysing the Stokes profiles of Fe  i 6302.5 forming in the solar magnetized atmosphere, with the aid of a departure factor defined to evaluate the deviation from the normal Boltzmann distribution without a magnetic field. This factor is directly related to the ratio of line-source function to the continuum one. The relationship between the departure and the magnetic field reveals an effect that the magnetic field induces an exponential increase in the level population of the lower level of Fe  i 6302.5 (Landé factor   g = 2.5  ) with the field strength. This indicates that the magnetic field can cause the redistribution of populations of those levels whose Landé factors are non-zero. Therefore, this effect should be included in the calculation of the statistical equilibrium. Secondly, an experiment utilizing the Hg5461 line in the laboratory on the Earth is carried out to reveal that the exponential relation is independent of variations in temperature, and the excitation is completely magneto-induced. Finally, the exponential relation is explained by taking account of the magnetic energy in the Boltzmann distribution.     

Direct generation of solar and stellar radio bursts by energetic electron maser

A fully relativistic electron maser is proposed for the explanation of certain non-thermal solar and stellar radio bursts. This mechanism (maser synchrotron) is based on a gyroresonant interaction between waves and electrons of high energies and uses the free energy contained in an electronic distribution function that peaks for energies around 1 MeV.By a calculation of the growth rates of the three electromagnetic modes, we show that the X-mode prevails for values of _p/ _cup to 2 or 3. This result is very different from the standard cyclotron maser case where such values of _p/ _clead to quench the X-mode growth. Hence, the synchrotron maser instability appears to be a direct and efficient amplification process for considerably larger physical conditions than the cyclotron maser. In addition, the radiation, emitted over the second gyroharmonic, freely propagates without a strong reabsorbtion at the 2 _clayer. All these points can constitute major advantages of this mechanism in an astrophysical context.Proceedings of the Second CESRA Workshop on Particle Acceleration and Trapping in Solar Flares, held at Aubigny-sur-Nère (France), 23–26 June, 1986.     

螺旋钻进技术在杉木树煤矿强突出煤层中的应用

通过目前瓦斯抽放孔成孔工艺的比较,介绍了杉木树矿强突出煤层采用螺旋钻进工艺试验的工艺过程及其优势,并介绍了在该煤矿的具体试验情况。     

花岗岩研究的误区——关于花岗岩研究的思考之五

本文在对花岗岩四大基石(混合作用、结晶分离作用、构造环境和源区)问题分析的基础上,指出花岗岩研究存在的三大误区: (1)不恰当地仿效玄武岩的理论和研究方法,忽视了花岗岩的复杂性。(2)不恰当地用板块构造学说解释大陆花岗岩问题。板块构造是地球演化到一定阶段的产物,并成功解释了与板块边界相联系的岩浆活动,但是,它不能解决主要来源于大陆的花岗岩的地质问题。(3)太过重视花岗岩的地球化学研究而忽视了对花岗岩基础地质的研究。作者指出,地球化学方法在花岗岩中的使用应当是有限制的,花岗岩研究陷入误区是我们缺少扎实的基础研究、对板块构造的理解不深和对花岗岩复杂性认识不足等三个方面的原因造成的。文中还批评了学术界存在的人云亦云的奴性思想,指出它严重地阻碍了我们的创新思维,是当前亟待改进和克服的。