遗传规划在岩石力学中的应用

本文探讨了遗传规划这一新的优化方法在岩石力学参数确定中的应用。由于影响岩石力学性能的各因素之间关系不明确,而遗传规划特别适用于各影响因素之间因果关系不明确的复杂非线性问题。它为预测岩石力学性能提供了一条新的技术途径。通过例子,说明该方法的实用性。     

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.     

中国地区地震P波和S波走时表的实用检验

中国地区地震P波和S波走时表实测地震的效果如何?本文给出了一系列地震的实测结果,对比J—B表和其他走时表分析表明,建立在中国地区实际观测数据所独立算出的中国地区地震波走时表,更适合于实际情况,用以测定中国地区震中的参数具有较高的精确度。     

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。     

一次弓状降雹回波区流场的反演

通过对一次典型弓状降雹回波区的流场进行反及特点分析,发现用矩不变量法反演出的回波区流场结构,与藤田关于弓状回波的概念模式非常吻合,利用该方法估测出的流场,散度场、涡度场所表现出的信息,与降雹实况是一致的,该研究可为中小尺度强天气的监测,提供高时空分辨率的流场资料。     

一些常见铀矿物的红外吸收光谱特征

作者对我国产出的41种常见的铀矿物进行了红外光谱分析,并收集了国外已有资料,综合了10类53种铀矿物的红外吸收光谱特征。     

暴雨类冷涡与非暴雨类冷涡的合成对比分析

选择了８例典型的东北冷涡暴雨过程和８例典型的东北冷涡弱降水过程进行了合成对比分析，发现暴雨类冷涡其暴雨主要出现在冷涡的发展阶段，而非暴雨类冷涡的降水主要发生在冷涡的成熟阶段；暴雨类冷涡与其南侧的副热带低值系统联系密切，非暴雨类冷涡的这一特点不甚明显；暴雨类冷涡的两个降水中心分别出现在系统东侧偏南和南侧偏东一些的地，距系统中心大约３００－４００ｋｍ和７００－８００ｋｍ，这些区域处于低层辐合、高层辐菜