生活垃圾卫生填埋及地质环境效应概论

论述当前世界各国城市建设中必不可少的重要工程设施类型之一——生活垃圾处置工程。总结当前垃圾处置的主要方式,分析卫生填埋在各种处理方式中独具的优势,并简要介绍组成卫生填埋工程的各个部分及其功能;论述垃圾填埋体中进行的各种化学和生物化学作用及其变化;指出垃圾填埋体是其中的核心部分,填埋体结构的优化设计是控制污液污染地质环境的关键,提出填埋体结构设计的技术路线和系统方法。最后,根据当前卫生填埋场实施中存在的问题,为进一步有效地控制垃圾填埋处置对地质环境污染中的研究不足,提出意见和建议     

MIS 3晚期东亚季风强度和DO事件年龄

基于神农架山宝洞石笋(SB46)的9个230Th年龄和326个氧同位素数据,建立了末次冰期32.2～26.7kaB.P.和17.0～15.4kaB.P.的东亚季风降水序列。该序列和同一洞穴全新世石笋记录的对比发现,在MIS3晚期东亚季风区可能存在极强夏季风降水事件,相当于全新世季风强度,可能与岁差旋回太阳辐射及海陆水汽潜热释放增强有关。与葫芦洞石笋δ18O记录和格陵兰冰芯δ18O记录对比表明,东亚夏季风千年尺度气候振荡与高北纬地区海-气快速重组存在遥相关效应。山宝洞石笋年龄与葫芦洞石笋和格陵兰冰芯时标(SS09sea)在定年误差范围内基本一致,但山宝洞石笋与冰芯记录在DO事件的年龄、波形和持续时间上更为一致,不仅进一步说明了低纬季风气候与极地气温同步变化,而且有效地弥补了葫芦洞记录在这一时段的不足。     

Effect of the alidade thermal behavior on the pointing accuracy of a large radio telescope

The alidade's non-uniform temperature field of a large radio telescope is very obvious under solar radiation. Estimating a radio telescope's pointing errors, caused by the alidade deformation under solar radiation, is significant to improve the telescope's pointing accuracy. To study the effect of the alidade thermal behavior on the pointing accuracy of a large radio telescope, a temperature experiment is first carried out in a 70-m radio telescope on a sunny day. According to the measured results, the temperature distribution rule of the alidade is summarized initially. In addition, the alidade's temperature field is calculated by finite element thermal analysis. The simulated results are proved to be in good agreement with the experimental results. Finally, the alidade deformation under solar radiation is computed by finite element thermalstructure coupling analysis. The telescope's pointing errors caused by alidade deformation are estimated via the alidade's node displacements. The final results show that the effect of alidade thermal behavior on the telescope's elevation pointing errors ?ε_2 + ?ε_r is much more than the effect on the telescope's crosselevation pointing errors ?ε_1. The maximum of ?ε_2 + ?ε_r is more than 45, while the maximum of ?ε_1 is less than 6. This study can provide valuable references for improving the pointing accuracy of large radio telescopes.     

A very bright (i=16.44) quasar in the ‘redshift desert' discovered by the Guoshoujing Telescope (LAMOST)

The redshift range from 2.2 to 3 is known as the ‘redshift desert' of quasars because quasars with redshifts in this range have similar optical colors as normal stars and are thus difficult to find in optical sky surveys.A quasar candidate, SDSS J085543.40001517.7, which was selected by a recently proposed criterion involving near-IR Y-K and optical g-z colors, was identified spectroscopically as a new quasar with a redshift of 2.427 by the Guoshoujing Telescope (LAMOST) commissioning observation in 2009 De...     

分布式水文模型全局敏感性高效分析方法研究(英文)

Sensitivity analysis of hydrological model is the key for model uncertainty quantification. However, how to effectively validate model and identify the dominant parameters for distributed hydrological models is a bottle-neck to achieve parameters optimization. For this reason, a new approach was proposed in this paper, in which the support vector machine was used to construct the response surface at first. Then it integrates the SVM-based response surface with the Sobol’ method, i.e. the RSMSobol’ method, to quantify the parameter sensitivities. In this work, the distributed time-variant gain model (DTVGM) was applied to the Huaihe River Basin, which was used as a case to verify its validity and feasibility. We selected three objective functions (i.e. water balance coefficient WB, Nash-Sutcliffe efficiency coefficient NS, and correlation coefficient RC) to assess the model performance as the output responses for sensitivity analysis. The results show that the parameters g1 and g2 are most important for all the objective functions, and they are almost the same to that of the classical approach. Furthermore, the RSMSobol method can not only achieve the quantification of the sensitivity, and also reduce the computational cost, with good accuracy compared to the classical approach. And this approach will be effective and reliable in the global sensitivity analysis for a complex modelling system.     

Two-dimensional properties of nearby galaxies

Research on two-dimensional (2-D) properties of galaxies is a significant component of the study of galaxy formation and evolution. Through the spatial distribution of physical properties (derived from integrated luminosity and spectroscopy) of galaxies, we are allowed to realize the inner environment and evolution history of each individual galaxy and finally answer how galaxies were assembled. In this paper, with reviewing previous work, we present a proposal for study on 2-D properties of nearby galaxies. In our prospective work, we will make use of multi-wavelength data covering a range from ultraviolet to far-infrared to determine the distributions of properties such as age, metallicity and dust-reddening in nearby galaxies, and try to remove the degeneracy among them. Combining with surface photometry and spectroscopy, we will also analyze the distribution of HII regions and star formation properties in galaxies. In our future plan, the World Space Observatory for Ultraviolet (WSO/UV) will be applied to our research and allow detail diagnosis of nearby galaxies at ultraviolet band.     

Measurements of electronic properties of the Miyun 50 m Radio Telescope

Measurement results of some properties of the Miyun 50 m radio telescope (MRT50) of the National Astronomical Observatories, such as pointing calibration, an-tenna beams, system noise temperature, gain and gain variations with elevation are intro-duced. By using a new de-convolution technique developed by our group, the broadening effect on measured beams caused by the width of an extended radio source has been re-moved so that we obtained higher accuracy on the measurements of MRT50 beams.     

The Influences of Shock Thickness and Alfven Waves on the Particle Acceleration by Diffusive Shocks

The influences of the shock thickness and Alfven waves on the particle acceleration by diffusive shock waves are numerically studied through solving one-dimensional diffusive equation including the second-order Fermi effect. It is shown that the spectral index of the energetic particles strongly depends on the shock thickness. For example, the spectral index increases from 2.1 to 3.7 in the low energy range of 3—10 MeV and from 2.5 to 5.0 in the high energy range of 20—60 MeV as the thickness increases. The spectral index decreases from 4.3 to 3.1 as the particle injection energy increases. The spectral index decreases from 4.0 to 1.8 at the quasi-steady stage with the enhancement of the compression ratio from 2 to 4. The results indicate that under the influence of Alfven waves, the energetic particle spectrum at lower energy becomes flat and the spectral index decreases from 2.5 to 0.6 in the low energy range of 3—10 MeV and from 11.6 to 5.0 in the high energy range of 20—60 MeV. At the same time, the turning point energy reaches 19.6 MeV. The spectral index decreases from 5.8 to 2.9 as the energy density of Alfven waves increases. All these results are basically consistent with the theoretical models, as well as the observations of typical energetic particle events.     

松辽盆地朝73-87井青山口组缺氧事件层的有机地球化学特征

松辽盆地白垩纪青山口组下部广泛分布一套富含有机碳的黑色泥岩、页岩和油页岩沉积,是全盆地划分泉头组与青山口组的一级标志.朝73-87井青山口组黑色页岩、油页岩的地球化学特征研究表明：它具有干酪根碳同位素正偏和重排甾烷含量低,存在28,30一双降藿烷、伽马蜡烷生物标志化合物等有机地球化学特征,表征为白垩纪温室效应时间窗内古湖泊缺氧事件的产物.结合生物地层研究成果,认为青山口期缺氧事件层大体可与白垩纪古海洋Cenomanian-Turonian界线事件层进行对比,进而提出松辽盆地青山口组的时代归属晚白垩世晚cenomanian-Turonian期的新观点.     

金沙江何时开始向东流

青藏高原的东南缘具有独特的地貌特征,不像其它边缘,这里坡面非常平缓,这上面发育的主要河流有金沙江,雅砻江和大渡河。金沙江的主支流河谷保存着大量的湖相沉积--昔格达层,我们通过宇宙成因埋藏年龄法定出湖相沉积的年龄为158～134 Ma。对金沙江上游的碎屑锆石U Pb年龄分析表明其物源主要体现了所流经的羌塘地块的冈瓦纳地体特征,并加入了华北地体的特征,明显有别于雅砻江流域的物源。对昔格达及其下伏河流砂砾的U Pb年龄分布特征研究表明昔格达古湖形成之前攀枝花至涛源河流流向为自东而西,与现流向相反; 伴随着昔格达古湖的形成与切穿,攀枝花至涛源一带的水流开始由西向东,金沙江从此开始向东流去。