南极地区Es特性研究          下载免费PDF全文

赵海生  许正文  吴健 《极地研究》2012,24(2):129-135

Es是发生在电离层E层高度上的偶发电离增强结构,其电子密度最高可达E层背景电子密度的100倍以上。Es出现概率和强度全球分布不均,主要分布在中低纬度地区,极区也有较强Es出现并具有显著特点,极区Es的研究,对研究Es成因和物理机理具有重要科学意义。本文利用Syowa站（69.0°S,39.6°E）40余年的观测数据,选取临界频率和虚高两个参数,研究了南极地区Es强度特性、日变化、季节变化及长期变化特性。  相似文献   

Air–sea interaction over ocean fronts and eddies   总被引：1，自引：0，他引：1  

R.J. Small  S.P. deSzoeke  S.P. Xie  L. O&#x;Neill  H. Seo  Q. Song  P. Cornillon  M. Spall  S. Minobe 《Dynamics of Atmospheres and Oceans》2008,45(3-4):274

Air–sea interaction at ocean fronts and eddies exhibits positive correlation between sea surface temperature (SST), wind speed, and heat fluxes out of the ocean, indicating that the ocean is forcing the atmosphere. This contrasts with larger scale climate modes where the negative correlations suggest that the atmosphere is driving the system. This paper examines the physical processes that lie behind the interaction of sharp SST gradients and the overlying marine atmospheric boundary layer and deeper atmosphere, using high resolution satellite data, field data and numerical models. The importance of different physical mechanisms of atmospheric response to SST gradients, such as the effect of surface stability variations on momentum transfer, pressure gradients, secondary circulations and cloud cover will be assessed. The atmospheric response is known to create small-scale wind stress curl and divergence anomalies, and a discussion of the feedback of these features onto the ocean will also be presented. These processes will be compared and contrasted for different regions such as the Equatorial Front in the Eastern Pacific, and oceanic fronts in mid-latitudes such as the Gulf Stream, Kuroshio, and Agulhas Return Current.  相似文献   

柴达木盆地西部地区断裂类型及油气勘探意义   总被引：5，自引：1，他引：4       下载免费PDF全文

王亚东  方小敏  高军平  刘栋梁  张跃中  张伟林 《地质科学》2009,44(3):957-965

为研究柴西地区油气成藏及其与青藏高原隆升的关系,我们借助生长断层定性和定量分析,总结出该区断裂在演化上总体可归纳为两个主要形成时期和4种表现形式：早期形成时期(E1＋2?N),中生代以来开始活动,多数终止于下油砂山组末(约14.9 Ma); 晚期形成时期(N?Q),上油砂山组开始活动,狮子沟组(约8.2 Ma)以来活动尤为剧烈,持续至今。在形式上主要表现为限于下或上构造层的生长断层; 贯穿下、上构造层的生长断层和后期断层4类。柴西地区的这种断裂构造特征,与青藏高原的分阶段隆升相对应,控制着该区的油气运移、成藏、保存及改造,对我们在柴西地区的油气勘探工作具有重大意义。  相似文献   

冷水坑银矿田成矿条件及矿床特征     

黄振强 《地质与资源》1993,2(4):284-291

冷水坑中生代陆相火山-次火山岩型银矿田的成矿地质条件,着重论述矿田层控叠加型、斑岩型矿床的分布规律、物质组分、矿化分带等基本地质特征。  相似文献   

太平煤矿深厚土层的水文地质工程地质性质   总被引：1，自引：0，他引：1  

张改玲  陈德俊 《煤田地质与勘探》1999,27(2):42-44

依据对太平煤矿3号煤区深厚土层的水文地质与工程地质勘测及室内外实验结果,分析了主要的水文地质与工程地质特征及其对3号煤开采的影响,对矿区防水煤岩柱留设高度进行了合理确定。   相似文献   

Post-noon two-minute period pulsating aurora and their relationship to the dayside convection pattern     

S. E. Milan  T. K. Yeoman  M. Lester  J. Moen  P. E. Sandholt 《Annales Geophysicae》1999,17(7):877-891

Poleward-moving auroral forms, as observed by meridian-scanning photometers, in the vicinity of the cusp region are generally assumed to be the optical signature of flux transfer events. Another class of quasi-continuous, short period (1–2 min) wave-like auroral emission has been identified, closely co-located with the convection reversal boundary in the post-noon sector, which is similar in appearance to such cusp aurora. It is suggested that these short period wave-like auroral emissions, the optical signature of boundary plasma sheet precipitation in the region 1 field-aligned current system, are associated with ULF magnetohydrodynamic wave activity, which is observed simultaneously by ground magnetometer stations. This association with ULF wave activity is strengthened by the observation of several harmonic frequencies in the pulsation spectrum, each an overtone of the fundamental standing wave resonance frequency.  相似文献   

应用水化多层次跟踪预报方法研究闽台地区地震的映震特征     

陈小云 《福建地震》1999,(4)

本文针对1990年至1999年福建及沿海中强以上地震和台湾7.0级以上地震,利用“八五”攻关的水化多层次跟踪预报方法,研究福建水氡台网观测资料的异常频次变化特征和演化过程,总结其相应的映震特征。  相似文献   

Possible configurations of the magnetic field in the outer magnetosphere during geomagnetic polarity reversals     

D. M. Willis  A. C. Holder  C. J. Davis 《Annales Geophysicae》1999,18(1):11-27

Possible configurations of the magnetic field in the outer magnetosphere during geomagnetic polarity reversals are investigated by considering the idealized problem of a magnetic multipole of order m and degree n located at the centre of a spherical cavity surrounded by a boundless perfect diamagnetic medium. In this illustrative idealization, the fixed spherical (magnetopause) boundary layer behaves as a perfectly conducting surface that shields the external diamagnetic medium from the compressed multipole magnetic field, which is therefore confined within the spherical cavity. For a general magnetic multipole of degree n, the non-radial components of magnetic induction just inside the magnetopause are increased by the factor 1 + [(n + 1)/n] relative to their corresponding values in the absence of the perfectly conducting spherical magnetopause. An exact equation is derived for the magnetic field lines of an individual zonal (m = 0), or axisymmetric, magnetic multipole of arbitrary degree n located at the centre of the magnetospheric cavity. For such a zonal magnetic multipole, there are always two neutral points and n – 1 neutral rings on the spherical magnetopause surface. The two neutral points are located at the poles of the spherical magnetopause. If n is even, one of the neutral rings is coincident with the equator; otherwise, the neutral rings are located symmetrically with respect to the equator. The actual existence of idealized higher-degree (n > 1) axisymmetric magnetospheres would necessarily imply multiple (n + 1) magnetospheric cusps and multiple (n) ring currents. Exact equations are also derived for the magnetic field lines of an individual non-axisymmetric magnetic multipole, confined by a perfectly conducting spherical magnetopause, in two special cases; namely, a symmetric sectorial multipole (m = n) and an antisymmetric sectorial multipole (m = n – 1). For both these non-axisymmetric magnetic multipoles, there exists on the spherical magnetopause surface a set of neutral points linked by a network of magnetic field lines. Novel magnetospheric processes are likely to arise from the existence of magnetic neutral lines that extend from the magnetopause to the surface of the Earth. Finally, magnetic field lines that are confined to, or perpendicular to, either special meridional planes or the equatorial plane, when the multipole is in free space, continue to be confined to, or perpendicular to, these same planes when the perfectly conducting magnetopause is present.Also Honorary Research Associate, Rutherford Appleton Laboratory, Chilton, Didcot, Oxon OX11 0QX, UK and Visiting Reader in Physics. University of Sussex, Falmer, Brighton BN1 9QH, UK  相似文献   

海上风电吸力基础在分层土中的沉贯特性研究综述     

李大勇  黄凌昰  张雨坤  吴学震 《海洋工程》2023,41(1):110-127

吸力基础与海洋工程大直径钢桩相比,具有成本低、安装周期短、对环境影响小、不受海况影响及可回收再利用等优点,近年来在海上风电工程中得到推广应用。吸力基础沉贯至海床预定位置,是其发挥承载力和确保服役稳定性的前提。海床地基土体常以分层土形式分布,且各层土体强度、压缩性和渗透性等存在显著差别,导致吸力基础吸力沉贯机理非常复杂。明确吸力基础在分层土中沉贯特性,有助于指导吸力基础在海上风电工程中的推广应用。对目前吸力基础在分层土中沉贯特性研究进行综述和总结,归纳了其沉贯机理研究进展,并对影响吸力基础在分层土中沉贯因素进行了分析;提出了分层土中吸力基础沉贯的研究方向和改进的沉贯方法。  相似文献   

来自海底高速层径向波的理论地震图研究   总被引：1，自引：0，他引：1       下载免费PDF全文

姚陈  郝重涛 《地球物理学报》2018,61(1):216-229

本文利用各向异性反射率技术计算理论地震图,提出海底高速薄层会产生沿高速层水平传播的波（简称径向波）,这种波在水层中作为P波,在固液界面激发下行横波,该均匀横波以临界角入射高速薄层,在层内作为超临界角的非均匀横波水平传播,再以临界角转换为上行传播的均匀横波,最终在固液界面上行透射转换为水层中P波.高速薄层传播的径向波不同于界面折射波,也不同于具有频散的面波和通道波.理论地震图的研究表明,径向波具有线性时距,能与海底强反射具有同等振幅水平;径向波有其振幅、时距位置和斜率这些观测记录参数,分别对应高速层的厚度、深度和近似的横波速度;径向波可以克服折射波解释中遇到的振幅强弱和高速层速度等困难.径向波可作为探测海底高速薄层的有力工具,对于研究高速层屏蔽、海底反射类型的多样性和相应的资料处理解释有重要意义.  相似文献