海上风电场高桩承台群桩基础平台的设计研究

针对国内海上风电基础设计没有统一的规范及标准，为提升海上风电基础设计建设的水平，通过对东南沿海某海域海上风电基础的设计进行了有限元计算分析论证，验证了群桩高承台结构设计方案的设计方法和设计参数。分析结果表明该设计的最大应力主要发生在塔筒底座与承台接触部位及钢管桩与承台连接段，应在连接部位加强措施处理；基础竖直位移较小，水平位移相对较大；分界部位应力较集中，刚度不能顺畅过渡，可考虑填充碎石土等方法加强。本研究对海上风电基础设计技术的研究与探索，可为将来制定中国海上风电行业标准提供可靠的依据，对中国未来大批量的海上风电能源的开发有着重要意义。     

北秦岭西段早侏罗世A型花岗岩及其地质意义

本文通过岩相学、岩石地球化学、锆石U?Pb定年和Lu?Hf同位素组成分析等方法,对出露于北秦岭西段宝鸡岩体王家山一带的黑云母花岗岩和其中的包体进行了研究。结果表明,该花岗岩形成时代为187±2 Ma,属于高钾钙碱性—钾玄岩系列岩石,富集Rb、Th、U等大离子亲石元素以及Nb、Zr和Hf等高场强元素,亏损Ba、Sr和Eu,具有高的全岩锆石饱和温度(825℃~838℃),显示A型花岗岩特征,形成于造山后的板内环境,可能为秦岭岩群副变质岩与安山质岩石部分熔融的产物。暗色包体显示塑性流变特征,具有岩浆结构,发育针状磷灰石和具有复杂成分环带的更长环斑结构长石,是幔源岩浆注入酸性岩浆发生混合作用的产物,形成时代为191±2 Ma,其锆石Hf同位素组成变化范围较大,εHf(t)值介于-11.26~-2.51,主要为富集地幔部分熔融产物。综合本文及前人已有研究结果,认为~190 Ma的早侏罗世早期秦岭地区早中生代碰撞造山过程已经结束,区域开始逐渐进入板内伸展构造演化阶段。     

中国地质大学美术专业简介

1　艺术设计专业 (环境艺术设计方向 )四年制本科。培养系统掌握艺术设计基本原理 ,知识面宽、综合素质强 ,具有创新思维及一定实践能力和创业精神 ,能独立担任环境艺术设计、室内设计的专门人才。毕业生可广泛在企事业单位 ,尤其是在建筑业、室内装饰业、环境艺术、园林等部门 ,从事理论研究、综合管理和项目设计等工作。2　艺术设计专业 (资讯艺术设计方向 )四年制本科。是艺术设计专业的一个最新的专业方向。培养具有创新的艺术思维能力 ,综合扎实的艺术设计素质 ,以计算机高新科技为辅助手段 ,与网络技术相衔接 ,掌握信息技术和艺术设计…     

Statistical Properties of the Highest Pulses in Gamma-Ray Bursts

We study the statistical properties of the highest pulses within individual gamma-ray bursts (GRBs). A wavelet package analysis technique and a developed pulse-finding algorithm have been applied to identify the highest pulses from burst profiles observed by BATSE on board CGRO from 1991 April 21 to 1999 January 26. The statistical light curves of the highest pulses in four energy channels have been derived by an aligning method, which illustrate the temporal evolution of the pulse emission. Our result that narrower pulses go with higher energies is consistent with previous findings. By normalizing both the pulse durations and counts to unity, “characteristic” profiles of the highest pulses in the four channels are also derived. The four characteristic profiles are turned out to be almost the same, thus strongly support the previous conclusion that the temporal profiles in different energy channels are self-similar and the previous conjecture on GRB pulses, implying that the emission process is similar at different energies. The cosmological time dilation effect is examined by investigating the relationship between the pulse flux and pulse duration. An anti-correlation between the two was found, which agrees with the expectation of the cosmological time dilation effect. Also, the evolution of the pulse duration with the observational epoch is studied. The result shows that the pulse duration tends to be shorter in later epochs. This trend cannot be explained by the present theoretical models, and may represent a great challenge to current theories.