Models of CN and C2 comae for comet Tago-Sato-Kosaka and comet bennett

Based on the CN and C₂ comae isophotes for two comets (1961 IX and 1970 16) given by Rahe et al. and the relevant theory of physical chemistry, we have deduced the distributions of the CN and C₂ modecules in the coma, their scale heights and mean lifetimes. The results favour the viewpoint that HCN is the parent of CN, and that C₂H₂ is the parent of C₂.     

Modelling the April 15 spectrum of Supernova 1993 J

We present the modeling of the ultraviolet and optical spectra obtained simultaneously on 1993 April 15 with the HST and at Lick Observatory. A Monte Carlo code is employed in the modeling and a comparison is made between models reported by different groups. With an atmosphere similar to the Sun in chemical composition, the observed spectral lines are well reproduced by a power law density structure of index around 20 except the strong H and HeI λ5876 lines which have peculiar absorption profiles. The photospheric velocity is found to be 9500 km/s and the blackbody temperature of the spectrum is 7990 K. For H and HeI λ5876, we suggest a two-component density structure which has a smoother layer located immediately outside the steeply decreasing inner envelope. The power law indices are most probably 20 and 3, respectively, with the transition point at about 13 000 km/s. In addition, this outer smooth layer serves to flatten the far UV spectrum as observed.     

A THREE-DIMENSIONAL ELASTIC NESTED-GRID MESO-(β-γ)SCALE ATMOSPHERIC MODEL——PARTI:MODEL DESCRIPTION

A three-dimensional elastic nonhydrostatic mesoscale(β-γ)model with nested-grid is presented.It uses a set of fullequations in terrain-following coordinates as its basic dynamic frame,which is solved with a time-splitting algorithmfor acoustic and gravity waves.The model physical parameterization includes a K-theory subgrid eddy mixing for cloudand free atmosphere,a bulk planetary boundary layer parameterization,and three types of sofisticated cloudmicrophysics schemes with double-parameters for hail-bearing clouds,warm clouds and snowing clouds respectively.The model is designed to be used flexibly for simulations of a variety of meso-and small-scale atmospheric processes,and can be improved as a regional and local operational NWP system in future.     

初至层析静校正在复杂山地三维地震勘探中的应用

随着地形高差增大、地貌单元多变、近地表模型复杂,目前被广泛应用的初至折射静校正的精度已无法满足精细勘探的要求。初至层析静校正技术,由给定的初始模型进行正演,用射线追踪方法得到初始模型的初至波,利用该初至波和实际拾取的初至波进行比较,计算地表模型的修正量,反复迭代求得准确的地表模型。山西省国阳新能股份有限公司二矿390水平九采扩区地表标高940～1100m,地貌单元复杂,在对该区资料处理时,利用初至层析折射静校正,经9次迭代计算后,真实地刻划出近地表模型。在二种静校正技术对比中,初至折射静校正不但近地表模型精度低于层析折射静校正,而且其叠加剖面精细程度也远低于层析静校正,如在初至折射静校正叠加剖面同相轴上呈现的凹凸形态,在层析静校正叠加剖面并无显示,且后者剖面的信噪比也比前者明显提高。     

路基施工沉降观测精度要求及数据处理

本文通过对路基施工沉降观测的精度分析,提出了路基施工沉降观测的精度要求；根据路基施工沉降观测的特点，提出了相应的观测措施及数据处理方法。     

我国黄铁矿矿床类型、分布规律及前景评估

中国黄铁矿资源丰富，按元素和矿物组合的不同，其矿床类型可分为：黄铁矿矿床；黄铁矿型铜矿床；含锌、铜黄铁矿型矿床；黄铁矿型多金属矿床；含钨黄铁矿型铜矿床；含锡黄铁矿型矿床；含金黄铁矿型矿床。最主要的成因类型是海底喷气沉积矿床，它广泛分布于不同时期的造山带及早前寒武纪克拉通。黄铁矿形成的构造环境可分为５种，即：边缘浅海或优地槽环境；上叠的断裂坳陷带；洋中脊；岛弧地带；陆相火山盆地。     

内陆待开发地区产业发展模式探讨——以内蒙古为例

以内蒙古为例，探讨了内陆待开发地区的产业发展模式，内陆待开发地区经济发展的主要制约因素是缺乏资金，缺乏技术，缺乏人才，因此，其经济发展必须有选择，有重点地优先发展部分行业。一般说来，待开发的内陆地区其经济发展必须以资源优势为依托，以市场为导向，开发优质名牌产品，发展优势产业，建设主导产业，带动地区经济的起飞。     

陆相火山岩铜矿床成矿条件研究

研究陆相火山岩铜矿床的成矿条件，对于多发现新的铜矿资源有着重要的意义。本文就陆相火山岩型铜矿床的实际存在，大陆玄武岩型铜矿的成矿系列，大陆裂谷的成矿环境和热液成矿作用等方面进行讨论。     

管缝式锚杆防治软岩巷道底臌的试验研究

根据对巷道围岩移动趋势的分析，充分考虑到锚杆在垂直于锚杆轴向方向上与围岩的相互作用．将其用于软岩巷道底臌的防治，简化了软岩巷道施工工艺。矿井的实际应用表明支护效果是明显的。     

试谈超大型铀矿床分类及找矿问题

随着核电事业在我国的发展，对铀资源保证的要求将越来越迫切。这里所指的铀资源保证应包含数量和效益两层意思，而超大型铀矿床则能同时满足对这两方面的要求。因此，在我国寻找超大型铀矿床是一项刻不容缓的任务。为了确立找矿目标，作者尝试提出了一种将矿床产出地质特征和经济效益相结合的超大型铀矿床分类方案，共划分出３大类１３个亚类。结合我国情况，作者认为在７个有远景的类型中，有３个（即Ⅰ－２、Ⅱ－１和Ⅲ－５）在我国最有突破的希望，特别是Ⅲ－５。最后，作者参考国外超大型铀矿床的找矿经验，对于加强我国对超大型铀矿床的探索提出了四点具体意见。