ANALYSIS OF EVOLUFIONARY RELATIONSHIP BETWEEN ASTASIA LONGA AND EUGLENA GRACILIS BY USING RAPD TECHNIQUE AND CLADISTIC ANALYSIS

Although both Astasia longa and Euglena gracdlis belong to different genera, they share many morphological characters except that A. longa has no chloroplast. In the 1940‘ s, on the basis of the finding that in darkness or upon addition of scrne chemicals, E. gmcilis would fade reversibly or irreversibly, scrne scholars hypothesised that A. longa evolved from E. gracilis by losing chloroplast.The authors‘ use of RAPD and cladistic analyses in a study on the evolutionary relationship between A .longa and E. gmcilis showed that the A. longa ‘ s relationship with E. gmcilis was closer than that with other green euglenoids. This proves the hypothesis that A. longa evolved from E. gmcills is reasonable. The results d this study suggest that saprophytic colorless euglenoids were transformed fromgreen euglenoids by losing their choroplasts.     

青海省地质灾害防治工作刍议

通过对青海省地质灾害形成的地质环境条件及主要灾种分布特点、灾害现状及典型实例的初步分析,结合目前地质灾害防治工作的进展和存在的问题,探讨了我省地质灾害防治的基本原则和思路,提出了地质灾害防治工作的对策和主要措施。     

江汉洞庭盆地的非对称扩张与潜在地震危险性

本文依据地震地质、地球物理、第四纪地质和构造地貌等资料，参照目前可以接受的应力－荷载模型、热扩散模型和非对称扩张模型，较详细地论述了江汉洞庭盆地（ＪＤＢ）的构造演化历史、主要活动断裂的新构造变形与地震活动的相关特征，尝试性地预测未来强震危险程度，并提出若干抗震防灾的对策，目的在于为ＪＤＢ的长远开发规划、生命线和重要城市的抗震减灾提供基础资料。     

滇西试验场区地壳的试验均衡研究

本文利用滇西试验场区最新完全布格重力异常和地形高资料，采用设置虚拟数区和边界限定、消除趋势项、低道滤波等预处理措施，按试验均衡理论，计算了该区地壳的均衡响应函数及试验均衡异常；结合文献［１］的研究结果，对其均衡异常分布特征、区域构造运动机制、活动断裂与强震展布间的关系进行了研究；结果表明：１）该区均衡响应函数值高于美国、加拿大及我国华北等地区，其地壳处于亚均衡状态；２）区内各部位的均衡状态并不均一，且异常幅值大小多与地壳的相对隆起或沉降相关；３）红河断裂带两侧均衡异常值差异明显，全区均衡异常的展布同活动断裂与强震分布有较密切的联系。     

Gamma-Ray Line Versus Continuum Emission of Electron-Dominated Episodes During Solar Flares

Electron-dominated episodes or events during solar flares are characterized by a flattening of the electron bremsstrahlung continuum above about 1 MeV. This flattening leads to a dominance of the continuum at MeV energies over nuclear emissions. We analyzed events recorded by the gamma-ray spectrometer on SMM with the aim to determine the nuclear contribution in the energy range between 4 and 8 MeV. We find that for comparable continuum fluences it is less by about an order of magnitude than for other flares. The spectral index of the best-fit power law of the > 1 MeV continuum with a median at –1.84 turns out to be independent of the heliocentric angle of the events, implying that the degree of anisotropy of the radiating particles was low. It is of interest to note that a value of –1.5 seems to be a limit. The spectral index of the continuum between 0.3 and 1 MeV does not differ significantly from that of other flares. Only measurements with detectors sensitive up to at least 10 MeV can, therefore, sort out electron dominated episodes during solar flares.     

我国对外贸易中的环境问题与可持续发展对策

从可持续发展概念入手,针对我国经济发展现状,分析了当前我国对外贸易中存在的诸如污染密集型产业和有害危险废物的越境转移,国际贸易中环境标志制度的兴起等环境问题及形成的主要原因,提出了加强可持续发展教育,完善环境法规,强化政府管理职能,实现对外贸易走可持续发展道路的若干对策。     

大口径嵌岩钻进技术发展与展望

分析了大口径嵌岩钻进面临的主要技术难点,并对目前国内常用的３种大口径嵌岩钻进方法－牙轮／滚刀钻进法、冲击钻进法（包括无循环和反循环）和气动／液动潜孔锤钻进法的技术现状作了介绍,提出了提高我国大口径嵌岩钻进技术水平的建议。     

赣南贵,有色金属矿床成矿地质条件初步分析

赣南贵金属、有色金属成矿与其特有的构造岩浆条件息息相关。本文用较详细的实际资料,初步分析其成矿条件,提出了一些新的认识,为进一步找矿指明了方向。     

Time-match semi-empirical models of the chromospheric flare on 3 February, 1983

Spectra of a 2B flare on 3 February, 1983 were observed simultaneously at H, H, and Can H, K lines with a multichannel spectrograph in the solar tower telescope of Nanjing University. The flare occurred in an extended region of penumbra at S 17 W07 from 05 : 41 to 07 : 00 UT. By use of an iterative method to solve the equations describing hydrostatic, radiative, and statistical equilibrium for hydrogen and ionized calcium atoms, five semi-empirical models corresponding to different times of the chromospheric flare have been computed. The results show that after the beginning of the flare, the heating of the chromosphere starts and the transition layer begins to be displaced downwards. However, during the impulsive phase the flare chromospheric region has a rapid outward expansion followed by a quick downward contraction. At the same time the transition layer starts to ascend and then descend again. After the H intensity maximum, the flare chromospheric region continues to condense and attains its most dense phase more than ten minutes after the maximum. Finally, the flare chromospheric region returns slowly to the normal chromospheric situation.     

Dynamic Analysis of a Single-Column Platform

In this paper, a single-column structure used as well-head platform is studied. The loads of wave and current exerted on the single-column will be greatly reduced, therefore the cost of the structure will be decreased. The advantages of the single-column structure compared with ordinary jacket structure are explained. A dynamic analysis of this type of structure is made and some problems related to dynamic analysis are solved. In order to check the reliability of computation theory and programme, model tests have been carried out. However, as space is limited, the conclusion of tests will be introduced in another paper. Therefore, this type of structure is applicable for proctical engineering.