Synchronous structure control of superlarge ore deposits

The control of synchronous structures on formation of superlarge stratabound ore deposits is immense. Based on studies of ore deposits in South Qiniing, northern Guangdong, Langshan and other areas, three new ideas in comparison with examples of ore control of synchronous structures both in China and abroad are proposed: (i) multiorder ore control of synchronous structures, which means that synchronous structures of different orders display different controls on ore deposits; (ii) synchronous structures in different stages of basin evolution display different controls on basin fluid system and ore-forming system; (iii) synchronous strurture accompanying hydrothermal mineralization as a preexisting weak surface in earth crust often reactivate in later tcctono-thermal event to be a channelway for magma or thermal fluids which superimposed on and reformed preexisting ore beds to form large or superlarge composite ore deposits.     

滇西地区综合环境因子预报地震的研究

本在原有单项预报指标的基础上,研究西地区（Ｎ２３°４８′－２６°２０′;Ｅ９７°００′－９９°３０′）Ｍ≥５．０级的地震。     

某些测震学指标与地震相关性研究

通过对１０项测震学指示宾１０ａ的大范围时空扫描得出的有震和无震“预报”进行了与５．０级以上的地震的相关性研究,结果证明这１０项指标当显性水平较低时,均可通过统计检验,表明是有效的提取异常指标。作还依统计检验结果对１０项测震学指标与地震相关性好坏进行了排序,并通过分析得到各指标今后优化方向．     

前兆异常识别的χ~2统计检验法及其应用

阐述了采用一定时间域前兆观测值的样本分布与其背景分布形式显著性的2 统计检验法识别前兆异常的思路 ,利用云南地区 1 994～ 1 996年的部分台站的水氡观测资料 ,采用上述方法提取了前兆异常 ,并与地震的实际发生情况进行了对比 ,表明强震前震源区附近水氡具有明显的前兆异常。由于分布形式的显著性检验法对异常反映较一般方法敏感 ,并且可以不受具体的分布形式的限制 ,因此本方法在地震前兆异常识别中将发挥一定的作用     

辽西地区中生代义县旋回火山活动特征分析

辽西地区广泛发育中生代火山岩,其中以义县旋回火山岩最为发育。本文在对辽西地区义县旋回火山岩微量元素地球化学特征研究的基础上,认为义县旋回火山岩具有同源性质,由壳幔混溶物质作用于统一的火山活动过程中产生。     

Radiatively driven mass accretion on to galactic nuclei by circumnuclear starbursts

We examine the physical processes of radiatively driven mass accretion on to galactic nuclei, owing to intensive radiation from circumnuclear starbursts. The radiation from a starburst not only causes the inner gas disc to contract via radition flux force, but also extracts angular momentum owing to relativistic radiation drag, thereby inducing an avalanche of the surface layer of the disc. To analyse such a mechanism, the radiation–hydrodynamical equations are solved, including the effects of the radiation drag force as well as the radiation flux force. As a result, it is found that the mass accretion rate owing to the radiative avalanche is given by M ˙ ( r )= η ( L _*/ c ²)( r / R )² (Δ R / R )(1 −  e ^−τ) at radius r , where the efficiency η ranges from 0.2 up to 1, L _* and R are respectively the bolometric luminosity and the radius of the starburst ring, Δ R is the extent of the emission regions, and τ is the face-on optical depth of the disc. In an optically thick regime, the rate depends upon neither the optical depth nor the surface mass density distribution of the disc. The present radiatively driven mass accretion may provide a physical mechanism which enables mass accretion from 100-pc scales down to ∼ parsec scales, and it may eventually be linked to advection-dominated viscous accretion on to a massive black hole. The radiation–hydrodynamical and self-gravitational instabilities of the disc are briefly discussed. In particular, the radiative acceleration possibly builds up a dusty wall, which 'shades' the nucleus in edge-on views. This provides another version of the model for the formation of an obscuring torus.     

Elasticity of orthoenstatite

Elastic constants of orthoenstatite have been determined from Brillouin-scattering measurements. They are c₁₁ = 2.247, c₂₂ = 1.779, c₃₃ = 2.136, c₄₄ = 0.776, c₅₅ = 0.759, c₆₆ = 0.816, c₂₃ = 0.527, c₃₁ = 0.541 and c₁₂ = 0.724 Mbar. Each elastic constant is uniquely defined by the data. Acoustic velocities measured for two directions ultrasonically on the same samples are within 1% of those determined from Brillouin-scattering spectra.     

对流层平流层气溶胶粒子的形态和化学组成

分析研究了１９９３年和１９９４年的８月、９月在香河地区上空采集的单个气溶胶粒子的形态及化学元素和化合物的组成。结果表明：１９９３年,在对流层大气中的气溶胶颗粒经常出现不规则形的粒子,可能是土壤粒子;而在平流层大气中的颗粒以具有“卫星”结构的硫酸粒子为主;硫酸铵粒子则经常出现在对流层的中、下部。香河地区上空颗粒物的化学元素组成比较复杂,单一化学元素组成的粒子较少,粒子主要含有Ｓｉ,Ｆｅ,Ａｌ和Ｓ等元素。气溶胶的化合物有硫酸盐、硅酸盐、硝酸盐和磷酸盐等     

四川盆地干旱动态评估指标的研究

在仔细分析干旱灾害物理成因基础上,围绕定量化和实时化这一核心,根据土壤水分盈亏原理,建立了具有清晰的物理意义的干旱动态评估指标。经检验,该方法符合实际,简便可行。     

全球稻谷主产国遥感估产可行性研究

利用NOAA气象卫星的序列资料,对全球稻谷遥感估产的可行性进行了探讨。并以泰国、美国、越南为例,分别对NDVI植被指数与产量进行相关分析,取得良好的应用效果。此外,还应用数理统计方法对全球稻谷的历史产量进行数学模拟,达到较高的拟合精度。