内蒙古乌兰花盆地上新统砂岩型铀矿成矿地质条件分析

本运用水成铀矿地质理论，对乌兰花盆地上新统铀矿成矿的区域地质背景、铀源条件、岩性岩相古地理、砂体特征和水地质条件进行了初步分析，认为该盆地上新世具备古河道的发育条件，上新统是主要的找矿目的层位之一，具备形成古河道砂岩型铀矿的成矿条件，但是同时也存在对铀矿形成的不利因素。     

内蒙古乌拉山群麻粒岩相岩石中变质矿物的标型特征

晚太古宙乌拉山群高级变质岩系分布于内蒙古大青山地区,包括各种麻粒岩和片麻岩,构成了东西走向的大青山太古宙麻粒岩带。本文对这套岩石中的斜方辉石、单斜辉石、石榴子石、角闪石、黑云母的物性和成分标型特征进行了系统分析。结果表明,这些矿物均为麻粒岩相条件下变质而成,并反映在发生麻粒岩相变质时,大青山南麓乌拉山群岩石的变质温度和压力均高于北边的岩石。     

江绍断裂两侧早元古代变质基底特征及形成的构造环境

江绍断裂东侧出露的早元古代变质基底以一套遭受中压型角闪岩相区域热流变质作用改造的黑云斜长变粒岩、云母石英片岩为主，夹少量斜长角闪岩和大理岩，已遭受４期构造变形作用改造，从原岩建造和主要岩类地球化学特点推测它可能形成于大陆或大陆边缘类似于内硅铝盆地环境。江绍断裂西侧早元古代变质基底则以星子杂岩为代表，由变粒岩、浅粒岩、（十字一石榴）云母片岩和少量斜长角闪岩组成，已遭受中压型高绿片岩相一低角闪岩相区域热流变质作用改造，推测其形成于活动性较强大陆一大陆边缘环境。江绍断裂两侧早元古代变质基底在原岩建造、变质一变形作用等特征上存在明显差异，因此华夏地块和扬子地块在早元古代可能是两个地块。     

增强型地热系统环境地质影响现状研究与对策建议

增强型地热系统（EGS）是目前地热资源开发利用的前沿热点,其发电几乎不受外界环境影响,且几乎不对人类环境产生污染和破坏,因而备受关注。近年来学者们发现EGS开发过程中,热储改造注水运行可导致大量的微震事件出现,少数EGS工程的注水过程与当地3级以上地震明显相关,需要密切关注。文章对增强型地热系统的原理、技术以及开发利用现状进行介绍,并对国内外主要的EGS相关环境影响事件进行了整理分析,在此基础上,总结了目前的EGS环境影响研究进展,提出了下一步可以采取的措施,可以为国内EGS工程选址及开发提供有效借鉴。      

花岗岩酸岩作用反应动力学研究

化学刺激能够改善增强型地热系统(EGS)热储层裂隙连通情况、提高裂隙渗透率。本文以EGS热储化学刺激为出发点,开展土酸体系-花岗岩作用实验,总结实验规律,明确了酸岩作用机理,建立多矿物耦合反应动力学模型并获取重要参数。得出以下结论:土酸中HF浓度越高,对花岗岩的溶蚀率和溶蚀速率就越大,但更易产生二次沉淀;酸液中离子的浓度与不同矿物溶蚀存在对应关系,Na⁺和K⁺分别来自于钠长石和伊利石,Al³⁺和硅来自长石类和黏土类矿物,Ca²⁺前期来自方解石,后期受钙长石和氟石影响;土酸-花岗岩反应为双重机制控制下的动力学反应;HF机制下的矿物溶解反应速率常数数量级约为10^-4～10^-5,比中性机制下的矿物的溶解速率提高了约9个数量级。研究结果可以为EGS储层化学刺激工作提供理论支持。     

Insights into Convective-scale Predictability in East China: Error Growth Dynamics and Associated Impact on Precipitation of Warm-Season Convective Events

This study investigated the regime-dependent predictability using convective-scale ensemble forecasts initialized with different initial condition perturbations in the Yangtze and Huai River basin(YHRB) of East China. The scale-dependent error growth(ensemble variability) and associated impact on precipitation forecasts(precipitation uncertainties) were quantitatively explored for 13 warm-season convective events that were categorized in terms of strong forcing and weak forcing. The forecast err...     

Solar Plasma Density and Spectrum of Accelerated Particles Derived From the 2.223-Mev Line of a Solar Flare

The time profile of the neutron capture line of 2.223 MeV for the flare of 16 December 1988 (its third peak) is analyzed. The enhancements of plasma density in the deep photospheric layers of the Sun under the flare region (an effect of density enhancement) have been deduced by the SINP calculation code. These enhancements are studied based on several modified models of the lower chromosphere, photosphere, and convection zone. Additionally, the case has been examined when the neutron source is placed at the top of the photosphere. The energy spectrum of accelerated particles (protons) is shown to evolve with time. Assuming a stochastic mechanism of acceleration and a Bessel function for the spectrum, we find the spectral index α T to increase from 0.005 to 0.1 during the decay phase of the burst; i.e., the proton spectrum becomes harder. Density enhancements found in the flare of 16 December 1988 are consistent with our previous results on the density enhancement effects deduced for two other flares, 6 November 1997 and 22 March 1991. It is suggested that density enhancements in the deep layers of the photosphere may be rather common features of powerful solar flares. B.M. Kuzhevskij is deseased.     

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。