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1.
《地学前缘》2017,(2):202-211
利用中国南北地震带38个固定地电场台站观测数据,研究该区大地电流场流线和电流矢量的分布特点,分析了大地电流矢量场的涡度和散度,并联系动力学机制讨论了大地电流与南北地震带的关系,探讨地震活动与电流涡度时变的对应性。这是首次应用空间密度较高的地电场台站开展这方面的研究工作。结果表明:(1)大地电流线走向和汇聚特点与构造地块的运动特点具有某种一致性,在构造边界上大地电流矢量存在汇集及分异的现象;(2)大地电流汇聚和发散等现象与断裂构造相关,一般表现为流线沿断裂带走向汇集或发散,在断裂交错地区表现出较复杂的形态;(3)大地电流场涡度分布特点可作为大构造块体运移的电性指示,涡度随时间变化可能为某种地震前兆。  相似文献   

2.
We have obtained continuous latitude distributions of the K and F corona brightnesses at various distances for the first time, using both the Hayes—Vourlidas—Howard method and our own recently proposed, simple technique for separating the emission of the K and F coronas. Data from the LASCO C2 and C3 coronagraphs are analyzed. Variations of the angular size of the brightness distribution of the F corona with latitude and distance are estimated, as well as the ratio of the maximum F-corona brightness to the F-corona brightness at the pole. The variations in the F-corona brightness at large distances (R = 25 R , where R is the solar radius) are studied on various time scales—a month, a year, and 11 years (the solar cycle). The latitude distribution of the F-corona brightness varies most appreciably over a year, and only weakly over one solar revolution and one solar-activity cycle (as considered on a fixed day of the year).  相似文献   

3.
近南北向构造在塔里木盆地的踪迹   总被引:3,自引:0,他引:3  
为厘清近南北向构造在塔里木盆地中的性质、地位和作用,笔者通过地质—地球物理分析,确认了以反转断层及相关褶皱为主导的挤压型构造是塔里木近南北向构造的主要表现形式。它发生发展于大陆内部,具有分布的广泛性和等距性、延伸的线性和断续性、纵深的陡倾性和穿透性、主断面的逆冲等特征。它的发育通常是基于先存的NS(—NNE)向张裂带和NNW(—NW)或NNE(—NE)向剪裂带,前者多演化为大、中型南北向构造,而后者多演化为中、小型南北向构造。近南北向构造的反转断层呈现为伸展—走滑—挤缩的演化顺序;最终定型于新生代;其驱动力主要源于太平洋—菲律宾板块向西的推挤动力。近南北向反转构造是种复合型的封闭性构造,对于石油和天然气地质研究,具有实际意义。  相似文献   

4.
A new series of yearly-mean relative sunspot numbers SN 2 that has been extrapolated into the past (to 1610) is presented. The Kislovodsk series with the scale factor b = 1.0094 ± 0.0059 represents a reasonable continuation of the mean-monthly and mean-yearly total sunspot areas of the Greenwich series after 1976. The second maximum of the 24th solar-activity cycle was not anomalously low, and was no lower than 6 of the past 13 cycles. A series A 2 of values for the total sunspot area in 1610–2015 has been constructed, and is complementary to new versions of the series of the relative number of sunspots SN 2 and the number of sunspot groups GN 2. When needed, this series can be reduced to yield a quantity having a clear physical meaning—the spot absolute magnetic flux Φ Σ(t)[Mx] = 2.16 × 1019 A(t) [mvh]. The maximum sunspot area during the Maunder minimum is much higher in the new series compared to the previous version. This at least partially supports the validity of arguments that cast doubt on the anomalously low ampltude of the solar cycles during the Maunder minimum that has been assumed by many researchers earlier.  相似文献   

5.
南北构造带是中国大陆地质构造及深部过程和地表系统的重要分界线,也是地震活动的多发地带,对其在前中生代是否存在、不同时期各区带的构造属性和联系研究薄弱。文中以南北构造带北部为研究对象,重点讨论其中南段,探讨研究区石炭纪地质构造特征及其与具分区意义的南北构造带形成演化的联系。研究表明,在石炭纪,今南北构造带北部所在地区处于伸展裂陷环境,断裂活动强烈,总体控制着河西走廊—北祁连沉积域的东界和隆拗格局及沉积厚度等变化。南北构造带北部及其西沉积区的断裂活动和沉积演化,经历了前黑山期初始裂陷、臭牛沟期进一步(向北)扩张、土坡期沉积-沉降鼎盛及太原期衰减4个阶段。其中于晚石炭世土坡晚期(本溪期)和太原期,东(华北)、西沉积域的沉积范围均向南北构造带北部扩展,先后经历了北部连通到全部相通的演变过程。石炭纪各期诸断裂与中、新生代断裂在位置和方向上具有明显的相关性,反映二者成生和演化联系密切。南北构造带北部及邻区,在石炭纪主要时期分隔华北和河西走廊—北祁连两大沉积域,东、西沉积域的沉积边界在该区带的分合演变和建造特征及断裂的主控因素,显示该区带在石炭纪已属具明显分区作用的重要地质构造单元,为此后南北构造带北部的进一步发展演化和重要的构造地位奠定了基础。  相似文献   

6.
《岩土力学》2017,(2):507-516
高拱坝工程基础地质及地形条件的不对称是威胁拱坝安全的重要问题。以白鹤滩高拱坝作为工程实例,通过地质力学模型试验重点研究基础不对称的高拱坝应力、变形及破坏模式的特点。针对初始方案和改进后方案分别建立三维数值模型,并进行弹塑性有限元超载计算。对比分析两方案坝体变形、坝肩应力分布、局部和整体稳定性等的不同,并结合试验现象,分析和评价针对基础不对称性的改进措施的加固效果及加固机制。结果表明:体形不对称性设计及基础加固的协同作用能有效改善坝体变形对称性、坝肩应力状态和传力效果,并提高拱坝-地基系统的整体稳定性。白鹤滩拱坝不对称性问题的研究对深入高拱坝设计优化和工程加固的认识具有重要意义。  相似文献   

7.
The rare phenomenon of the coalescence of two rotating sunspots of the same magnetic polarity during the emergence of the active region NOAA 11117 is investigated using data from the SDO space observatory. The coalescing spots rotated in opposite directions. The leading spot which formed from this process rotated counterclockwise with an angular velocity of 4°/h. A possible explanation is presented, based on a model of the emerging, twisted magnetic Ω flux tube that interacts with convective flows as it crosses the convective zone.  相似文献   

8.
9.
孙立强  闫澍旺  徐余 《岩土力学》2011,32(Z1):526-0531
在软土地基上修建道路,变形是控制道路质量和正常使用的主要因素。天津东疆港道路建立在经真空预压加固后的吹填土地基上,道路使用3 a后产生了严重的"波浪型"不均匀沉降,严重影响了车辆的行驶及人的生命安全。通过分析软土路基产生波浪变形的机制,提出了道路在建成后产生初始波浪变形,在车辆荷载作用下加剧了这种不均匀沉降的理念;建立了软土路基在波浪变形初值缺陷条件下的力学模型,通过力学分析与计算得出,在初始波浪变形条件下路基波谷受到比波峰大的车辆荷载;路基波峰与波谷处车辆动载大小的不同是加剧地基不均匀沉降变形的原因。提出利用土工格栅的加筋作用可减小不均匀沉降,通过有限元方法分析了该措施的加固效果。  相似文献   

10.
Breakage models and particle analyses have been widely used as tools for describing and interpreting various deposits and providing parameters for assessing the particle-size distribution of the deposits. Debris flows can be seen as a two-phase rheological fluid with a clay-fluid composition, and debris-flow deposits comprise mud, silt, sand, and boulders, with grain sizes ranging from less than one μm to more than several meters. As a consequence, according to fractal theory, the particles in debris-flow deposits have self-similarity in geometrical shape and scale invariance in size. In this paper, the fractal dimensions of particles in various debris-flow deposits are calculated and corresponding fractal features are determined based on fractal-statistical theory. The aims of the study are: to provide a quantitative grain parameter that reflects both the grain composition and grain-size distribution in debris-flow deposits; to compare the fractal dimensions of grains in different types of debris-flow deposits and the degree of self-organization of debris flows; as well as to discuss the geological implications of fractal dimensions and fractal features of particles in debris-flow deposits.  相似文献   

11.
12.
The pattern of natural size distributions   总被引:4,自引:0,他引:4  
  相似文献   

13.
14.

Reports

International seminar about North-South cooperation. Sea uses and environmental management  相似文献   

15.
A.J. Vroman 《Tectonophysics》1981,80(1-4):271-283
The formation of the major rift-valleys is proposed to have been triggered off by the E—W oriented tensional “wave” caused by the slow rotation of the equatorial bulge passing as a stretching hoop through the Earth (Paleozoic—Mesozoic). This ‘wave’ follows the wandering of the polar axis through a great circle (e.g. Creer et al., 1969). The polar wandering is regarded as the readjustment of the Earth's rotational instability caused by the growth of a “weight” fixed on the surface of the Earth and endeavouring to increase its moment of inertia until the weight rotates on the new equator (Gold, 1950). This weight, which must topple the Earth through its fixed spacial axis of rotation, may be slowly developing Pangea. The “wave” of E—W tension is imposed on zones already under E—W tension, e.g., crests of N—S running welts, alias “craton ridges”. The intruding asthenosphere expands the crests and fractures them along tensional rift-valleys. These rifts may develop as spreading centers by gliding of the plates over a lubricating basalt magma.

The idea proposed by R. Schweickert (pers. commun., 1979) that the lithosphere is decoupled from the asthenosphere to an extent that the shell may rotate as a separate unit (as a means to explain how fixed plumes move in unison under the “roll” of the lithosphere) is dismissed. The subducted slabs act as braking flaps and cannot overcome the friction against the asthenosphere. The “roll” would be too young (50 m.y.), because the polar wandering according to Creer is much older.  相似文献   


16.
The spatial (latitude) distribution of sunspots is studied, including its dependence on solar activity. It is shown that the latitude distributions of sunspots for a given year can be approximately described by the normal law, with its variance being a linear function of the current level of solar activity. Thus, an increase in activity is accompanied by an expansion of the zone of solar activity, in good agreement with earlier results. As the solar activity increases, the width of the zone of sunspot generation and the latitude maximum of the sunspot density grow somewhat more slowly than the number of sunspots, in agreement with observations. The results obtained can be used to reconstruct the spatial distributions of sunspots in the past, interpret the magnetic activity of stars, and address the requirements of the dynamo theory in the form of constraints imposed on models of cyclicity.  相似文献   

17.
甘肃庄浪全新世黄土-古土壤序列元素分布特征及意义   总被引:5,自引:1,他引:5  
通过对渭河上游XJN全新世剖面的Fe、Al、Si、K、Ca、Mg、Na、Ti和Sr元素含量的分析,发现这些元素的分布与气候密切相关。在剖面中表现为:迁移序列是Ca>Sr>Na>Mg,Fe、Al、Si、K和Ti则相对富集;Ca-Sr关系呈两段式分布,指示全新世早期的一次环境变化;Ki残积系数增大,Ca/Mg比值减小,指示化学风化作用增强。  相似文献   

18.
The distributions of dominant magnetic polarities in synoptic maps of photospheric magnetic fields and their extrapolations to the corona based on Stanford Observatory data are studied. Both dipolar and quadrupolar magnetic patterns are detected in the distributions of dominant polarities in the near-equatorial region of the photosphere for activity cycles 21, 22, and 23. The field in these patterns often has opposite signs on opposite sides of the equator, with this sign changing from cycle to cycle. A longitude-time analysis of variations of the mean solar magnetic field shows that the contribution of the large-scale magnetic patterns to the total field does not exceed 20 µT. The most stable magnetic structures at a quasi-source surface in the solar corona are separated by approximately 180° in heliographic longitude and are close to dipolar. The nature and behavior of these large-scale magnetic patterns are interpreted as a superposition of cyclic dynamo modes and the nonaxially symmetric relic field of the Sun. The contribution of the relic field to the mean solar magnetic field appears as a weak but stable rotational modulation whose amplitude does not exceed 8 µT.  相似文献   

19.
施红霞  王澄海 《冰川冻土》2015,37(2):327-335
基于CMIP5模式模拟的净初级生产力(NPP), 对21世纪初期(2016-2035年), 中期(2046-2065年)和末期(2080-2099年)三种排放情景下(RCP2.6、RCP4.5、RCP8.5)北半球中高纬度陆地NPP的时空变化进行了预估, 并结合气候因子分析了NPP的变化和气温、降水、辐射之间的关系. 结果表明: 相对于1986-2005年, 21世纪北半球中高纬度陆地NPP呈增加趋势, RCP8.5情景下NPP的增加比RCP2.6和RCP4.5情景下更为明显; 在季节变化上, 北半球中高纬度NPP也以增加为主, 且NPP在夏季, 尤其是6月增加最显著. NPP对气候变化的响应存在明显的区域差异性, 在中低排放情景下(RCP2.6、RCP4.5), 相对于1986-2005年, 21世纪北半球中高纬度地区温度显著影响的范围在逐渐缩小, 而辐射和降水显著影响的范围在扩大. 在高排放情景下(RCP8.5), 21世纪北半球中高纬度地区NPP的变化主要与温度有关.  相似文献   

20.
从河南板内 35°构造带地质历史时期的跷板式升降 ,以及构造带南北两侧成煤环境、构造差异、煤变质分带等方面 ,论述了河南板内北纬 35°构造带的主要特征及其地质意义。  相似文献   

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