夏季青藏高原地区降水和低涡的数值预报试验

本文首先分析了１９７９年６—７月的ＦＧＧＥIIIｂ级资料风场和相对湿度场在青藏高原地区的偏差，指出在高原西部应予以订正。然后利用一有限区域模式，通过综合订正初始风场和相对湿度场，改进模式部分物理过程，并提高其水平分辨率，共设计了６组预报试验，对该年的两例高原低涡切变线降水过程进行了２４小时预报。结果表明，利用改进了的初始场和部分物理过程，可明显改善高原地区的降水预报，并在一定程度上改善了流场的预报，即上述改进方案是可行的；但在高原地区嵌套预报方案尚待修改，还应继续努力提高模式对高原低涡流场的预报能力。     

拉张状态下方解石组构的递进变形规律

拉张状态下方解石组构多星环带到，递进变形状态下才可能出现点极密．因为当分解剪应力达最大值时，含有众多方解石颗粒的岩石中，形成ｅ双晶滑动最有利的方位不可能是唯一的，而是不同方位的滑动系在三维空间中的组合，并且ｅ双晶极点和光轴各自构成古钟型。由于系同一应力作用下的产物，二钟型体的顶角大小不同，但彼此共轴，均平行主任应力方向，属共轴叠钟体。该叠钟体记录了岩石变形时的应力状态，未再变形之前，该组构为初始组构。岩石的递进变形过程，实际是初始组构的递进变形过程，最后形成定型组构．岩石递进变形的全过程，就是初始组构到定型组构的全过程．     

吐—哈盆地丘陵油田裂缝定量预测探讨

裂缝油藏非常复杂和难以评价，本文从岩石脆性变形和递进变形的理论出发，从理论上指出了对理解缝发育程度进行定量预测可能性，并尝试着在露头和岩芯裂缝资料的基础上，以脆性岩石的裂缝密度取决于岩石应变量为假设前提，通过构造曲率的定量分析，岩石弹性应变能的数值模拟计算，以及裂缝和断层的关系分析几方面相结合的方法，定量估算丘陵油田不同构造部位缝的发育程序。预测结果表明，丘陵油区裂缝发育程度总体有如下特征：裂缝密     

A First Comparison of the Surface Brightness Fluctuation Survey Distances with the Galaxy Density Field: Implications for H0 and Omega

We compare the peculiar velocities measured in the surface brightness fluctuation survey of galaxy distances with the predictions from the density fields of the IRAS 1.2 Jy flux-limited redshift survey and the optical redshift survey (ORS) to derive simultaneous constraints on the Hubble constant H0 and the density parameter beta=Omega0.6&solm0;b, where b is the linear bias. We find that betaI=0.42+0.10-0.06 and betaO=0.26+/-0.08 for the IRAS and ORS comparisons, respectively, and that H0=74+/-4 km s-1 Mpc (with an additional 9% uncertainty due to the Cepheids themselves). The match between predicted and observed peculiar velocities is good for these values of H0 and beta, and although there is covariance between the two parameters, our results clearly point toward low-density cosmologies. Thus, the unresolved discrepancy between the "velocity-velocity" and "density-density" measurements of beta continues.     

圆顶视宁度和高美古观测室的考虑

本文给出了人为视宁度的定义和产生的原因,强调防止圆顶视宁度的重要性,简述了国际上的研究结果和经验教训,并结合高美古的实际,提出对高美古2m及1m望远镜观测室建造的方案和指标。     

Education challenges in the North Sea area

This paper introduces the North Sea as a fast evolving coastal ecosystem. The variability of natural conditions relates to the global climatic change and to human disturbances, which originate regionally. Education is an integral part of the strategy to improve environmental awareness. Considering contemporary challenges for educating the wider public about the main issues of environmental concern, attention is paid to various plans, which are being developed in North-Western Europe from primary schools to universities. "Learning for life" relies on an opening of the vocation of traditional universities and on the creation of a European university. Sharing resources in a competitive environment is one response given by British universities in the framework of a Discipline Network in Coastal Sciences and Management in 1996-2000. Networking is truly the key to a fast evolving teaching and learning context, notably in relation to ever developing information and communication technologies. The dissemination of scientific information is primordial in this context; a case study relating to the European project "Marine biodiversity in Europe" (BIOMARE) demonstrates the need for an elaborated strategy leading to socio-economic considerations. Empowering communities and governance are the main possible outcomes of such an enlarged approach to education, involving teachers, students, researchers, professionals, and volunteers. Proposals are made for amplifying the involvement of non-scientists into scientific research and its applications to management. Finally, a case is made for facilitating the mobility of all concerned, with a view to annihilate language and cultural barriers.     

Nucleosynthesis and Mixing in Cassiopeia A

We present results from the first light observations of the Cassiopeia A supernova remnant (SNR) by the Chandra X-Ray Observatory. Based on representative spectra from four selected regions, we investigate the processes of nucleosynthesis and mixing in Cas A. We make the first unequivocal identification of iron-rich ejecta produced by explosive silicon burning in a young Galactic SNR. Elsewhere in the remnant, we see silicon-rich ejecta from explosive oxygen burning. The Fe-rich ejecta lie outside the Si-rich material, indicating that bulk motions were extensive and energetic enough in Cas A to cause a spatial inversion of a significant portion of the supernova core. It is likely that this inversion was caused by "Fe"-rich ejecta emerging in plumes from the rising bubbles in the neutrino-driven convection layer during the supernova explosion. In addition, the radioactive decay energy from 56Ni may have contributed to the subsequent evolution of the material. We have also discovered faint, well-defined filaments with featureless X-ray spectra that are possibly sites of cosmic-ray acceleration in Cas A.