台风“摩羯”和“利奇马”经渤海强度变化特征分析

利用FY 4水汽云图、NCEP/FNL资料、自动站资料和ERA Interim海温资料,分析入海增强台风“摩羯”（1814）和入海减弱台风“利奇马”（1909）经过渤海强度变化特征。结论如下：台风“摩羯”中心入海增强过程伴随着中高层冷空气侵入,冷空气深入“摩羯”云系中心,台风强度减弱并逐渐消亡。台风“利奇马”入海前冷空气已经侵入台风中心,台风入海后强度减弱,暖心结构变得不对称,低层有清晰的斜压特征。“摩羯”入海前渤海上空为强辐散区,“利奇马”入海前渤海上空为弱辐合场,北上前进方向出现高空辐散有利于台风加强。台风登陆前垂直风切变与台风强度反位相分布,北上后台风垂直风切变与台风强度同位相分布。“摩羯”入海后水汽通道出现断裂,其入海增强更多依赖于热力条件和动力条件。“利奇马”水汽通量和水汽通量散度源于自身环流的贡献。台风“摩羯”入海后潜热加热率激增,“利奇马”低层维持弱潜热加热直至台风消亡。     

三组火山强迫资料差异及其对模式模拟结果的影响

Gao2008、Crowley2013和Sigl2015火山强迫资料,均基于极地冰芯重建.由于每组重建使用的冰芯数据和分析方法等不同,因此结果存在差异,从而影响气候模式应用.文中详细梳理三组火山强迫资料在原始冰芯数据、信号识别提取和沉积通量计算等方面的差异;介绍重建中涉及的对未知火山事件发生季节、纬度及从极地硫酸盐沉积...     

基于技术经济评价的取心钻进方法设计

提出了一种进行取心钻进设计的新方法,其特点是将技术经济学的思想引入钻探工程设计中,从而实现取心钻进方法的优选。该方法具有通用性,可用于任何钻探项目取心钻进方法的选择。在研究中,建立了评价取心钻进施工的技术经济评价指标体系;推导了钻进时间和成本的计算公式,并以一个5000m取心钻进项目的设计为例,对CCSD科钻一井的取心钻进方法进行了评价,证明由中国大陆科学钻探工程中心发明和研制成功的螺杆马达-液动锤-提钻取心法是一种高效、优质、低成本和安全的取心钻进方法。     

核心筒部分悬挂结构抗震分析的简化力学模型

提出了核心筒部分悬挂结构体系,在已有该体系振动台试验基础上,建立了该体系的抗震分析简化力学模型及其理论公式。按小震、中震和大震3种不同的地震作用情况,分析了该结构体系力学模型和动力方程的差异。利用有限元分析程序SAP2000,对这种结构体系进行了小震和大震作用下的结构地震反应分析,计算结果与试验结果吻合较好。     

The chronostratigraphy of a quaternary sequence at the distal part of the nile littoral cell,Haifa Bay,Israel

The current detailed chronostratigraphic framework of the last 1 Ma of an eastern Mediterranean sequence (Haifa Bay, Israel) aims to examine the relative roles of sea‐level changes, climate and tectonics. Seven continuous marine cores, up to ～120 m long, were recovered from shallow water depths. The cores were dated by optically stimulated luminescence, ¹⁴C, magnetostratigraphy, ²³⁰Th/²³⁴U, ²⁶Al/¹⁰Be, occurrence of index fossils and correlated to the global sea‐level curve and Marine Isotope Stages (MIS). The sedimentary sequence accumulated during the last ca. 1.0 Ma consists of 21 transgression–regression units with hiatuses between them. Five marine/terrestrial cycles, which occur in the lower part of the sequence, are attributed to the Jaramillo subchron and the Brunhes–Matuyama boundary, and correspond to MIS 29–21. The top ～50 m includes three sedimentary cycles deposited in the last ca. 400 ka. The regressive phases during this interval correspond to Glacial MIS 8, 6 and 2, while the transgressions correspond to Interglacial MIS 11, 7, 5 and 1. Thus, for the first time, this study documents the longest Quaternary succession dated so far in a key area of the Levant, sensitive to global history of sea‐level changes and glacial/interglacial fluctuations. Copyright © 2012 John Wiley & Sons, Ltd.     

On the magnetic field diffusion in mhd modeling of the inner coma of comet halley

Abstract

Some approaches of one-dimensional time-dependent magneto-hydrodynamic modeling of the structure of the inner coma of comet Halley are considered. The influence of the magnetic field diffusion on this structure is studied. The solution of Cravens (1989) approach containing classic magnetic diffusion is compared with an approach containing a specific diffusion, caused by non-instantaneous mass-loading of new ions. A case with no magnetic field is also considered. Common features of all the solutions are obtained. Special attention is paid to the sharp velocity jump, synchronized with a local density pick. Some differences between two types of magnetic field diffusion are discussed. A possible connection is supposed between this consideration and the large-scale shock fitting modeling of the solar plasma-comet interaction.     

南丹铁陨石物态方程用于地核的研究

从南丹铁陨石的物态方程和地球的PREM模型出发,求得内外地核交界面处的物质密度为12.83-13.419/cm~3,温度为5440-5680K;地心处物质密度为13.12-13.73g/cm~3,温度为5660-5990K,推估内地核可能由铁镍合金组成.