共查询到19条相似文献，搜索用时 234 毫秒
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本文通过地质构造形象的分析,对我国西南地区地质时期构造应力场转变特征进行了尝试研究。认为我国西南地区构造应力场,是随时间在变化的,并表现出一定的规律。上古生代之前,地壳竖直运动主要表现为东南部相对上升,西北部相对下降;上古生代以后表现为西部相对上升,东部相对下降。水平应力场自古生代以来,北部主要承受自北而南的压应力作用,西部主要承受自西向东的压应力作用,东部、东南部除加里东晚期外其压应力方向有自北北西向北西西方向偏转的趋势;而应力作用方式,已由上古生代前的南东方向挤压为主,转变为西部的自西向东挤压为主。 相似文献
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根据地球物理探测资料,基于二维模型,利用黏弹性有限元方法,研究青藏高原西、东剖面的地壳均衡和岩石圈根拖曳的构造应力机制.数值模拟结果表明,青藏高原西部（B B′剖面）的造山水平挤压力主要来源于岩石圈根的向下拖曳,印度板块向北挤压为次要因素,形成“山隆盆降”的地表形态;而青藏高原东部（A A’剖面）岩石圈根向下拖曳还不足以形成硬上地壳中挤压造山的主要力源.对比结果认为,青藏高原的深部层圈结构和应力体系在西、东部存在明显的差异,反映了高原内部造山演化的西、东分异特征. 相似文献
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本文探討了耀斑日面位置与磁扰关系的不对称性。經分析研究,得到（βγ+γ+βf）型活动区耀斑的磁扰效应有明显的南北不对称性,但（βp+β）型活动区耀斑却无此南北不对称效应。在太阳南半球,不論那种磁場类型活动区,发生在西边的耀斑要比东西或中心子午线附近耀斑的影响强,而在北半球只有（βp+β）型活动区耀斑才有这种东西不对称性效应。在最近三个太阳黑子周內,这些不对称是經常存在的,而在春秋季表現最为明显。 相似文献
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利用1951～2002年全国733个测站经过非均一性检验的月平均气温资料,在剔除50万以上人口大城市测站后,分析了52年来中国东、西部及青藏高原地区的气温变化趋势的一致性和差异性,并讨论了其可能原因.结果表明我国东、西部地区年、季平均气温变化有着较好的一致性;近52年来,我国东、西部和青藏高原地区年平均气温均呈升温趋势,年平均气温的增温速率东部为026℃/10a,西部018℃/10a,东部比西部高008℃/10a;季平均气温东部地区冬、春季的增暖趋势大于西部和青藏高原,而其夏、秋季的增暖趋势小于西部和青藏高原.我国东、西部地区年、季平均气温变化关系密切,说明其主要是受全球气候变化的影响而变化,但东部年平均气温的增暖总趋势大于西部,又说明地域差异在气温变化中也有重要作用. 相似文献
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A. V. Belov E. A. Eroshenko M. A. Abunina A. A. Abunin V. A. Oleneva V. G. Yanke 《Geomagnetism and Aeronomy》2016,56(6):645-651
Variations in the cosmic ray density during the initial phase of the Forbush effect during the first hours after the arrival of the interplanetary shock wave have been studied with the use of data on variations in the cosmic ray density with a rigidity of 10 GV obtained by the global survey method by the world network of neutron monitors in 1957?2012. It is found that behavior of this parameter after the arrival of the shock wave demonstrates high variability. A small (~1/5 of total number), though distinct, group of Forbush effects, in which the density of the cosmic ray increases (not decreases) after the arrival of the shock wave, is defined. As a whole, the initial variation in cosmic ray density is correlated with the Forbush effect magnitude and the strength of the associated geomagnetic disturbance. 相似文献
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采用二维理想MHD模型，分别在日球赤道面（二维二分量模型）和日球子午面（二维 三分量模型）内研究太阳风中纯速度增幅扰动的演化. 结果表明，该扰动在向外传播的过程 中逐渐演化为双重激波对，即由4个激波组成的激波系统. 该4个激波按离太阳由近及远依次 为后向快激波、后向慢激波、前向慢激波和前向快激波. 双重激波对在子午面内相对扰动源 中心法线基本对称，而在赤道面内则不对称：扰动源中心法线西侧双重激波对结构更为明显 ，所跨经度范围宽于东侧. 初步分析表明，行星际磁场的螺旋结构是产生日球赤道面内双重 激波对结构东西不对称性的主要原因. 相似文献
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猴石顶太古界重褶皱位于阜平太古宙穹状复合褶皱群中一个钩状褶皱的“钩子”部位。其中一层斜长角闪岩标志层的岩石磁性组构的分布情况为:1.在翼部的磁化率量值椭球是压扁形的,磁性叶理面的方向与变质层面及片麻理的方向基本一致,表现为向北西倾斜的倒转褶皱;2.在太古宙再次变形阶段所形成的转折端部位,磁性叶理面的走向变化较大,并出现拉长形的磁化率量值椭球,反映了经受过拉张作用的变形和多于一次的不同方向应力的作用;3.西翼的磁性线理值与磁性叶理值以及磁化率各向异性度都大,反映它经受过较强的剪切应力与压应力的作用;4.磁性线理主要倾向北半球,而且部分磁性线理近南北方向分布。 推测猴石顶重褶皱可能处于向北倾伏的主体构造的东侧。 上述岩石磁性是由自行设计的静态测量方法,用国产的数字式无定向磁力仪测定的。 相似文献
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通过对太阳风-磁层-电离层系统的全球MHD模拟,研究地球弓激波相对日地连线的旋转非对称性．模拟限于太阳风速度沿日地连线、地球磁偶极矩和行星际磁场（IMF）与日地连线垂直的简单情况．模拟结果表明,即便对于IMF强度为零的情况,弓激波相对日地连线也不具备旋转对称性质：终端面（晨昏子午面）及其向阳侧的弓激波截线的东西宽度大于南北宽度（约9%~11％）,终端面尾侧的弓激波截线东西宽度小于南北宽度（约8％）．在存在IMF的情况下,弓激波的位形同时受到磁层顶的形状和快磁声波速度各向异性的影响．磁层顶向外扩张并沿IMF方向拉伸,且其扩张和拉伸程度随IMF由北转南而增强．在磁鞘中,垂直于磁场方向的快磁声波速度高于平行方向．因此,磁层顶拉伸方向与快磁声波速度最大方向垂直,它们对弓激波位置的效应恰好相反;弓激波的最终形状取决于何种效应占据主导地位．对于终端面尾侧,快磁声波速度的各向异性起主导作用,弓激波截线沿IMF垂直方向的宽度大于平行方向．对于终端面及其向阳侧,弓激波截线的形状与IMF取向有关：在准北向或晨昏向IMF情况下,弓激波截线沿IMF垂直方向的宽度仍大于平行方向;在准南向IMF情况下,弓激波截线沿IMF垂直方向的宽度小于平行方向的．鉴于弓激波形状同IMF取向之间的密切关系,我们提议以IMF为基准方向,提取弓激波截线的平行半宽度Rb∥和垂直半宽度Rb⊥作为尺度参数．这些尺度参数和通常引入的弓激波截线的东西半宽度yb和南北半宽度zb相比,更为合理地表征了弓激波的几何性质．模拟结果表明,在终端面上,yb/zb和Rb∥/Rb⊥在IMF各向同性取向下的统计平均值均低于1,与观测得到的结论一致. 相似文献
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A. V. Belov M. A. Abunina A. A. Abunin E. A. Eroshenko V. A. Oleneva V. G. Yanke 《Geomagnetism and Aeronomy》2017,57(5):541-548
We consider the behavior of anisotropy and density of galactic cosmic rays in the first hours of Forbush effects from 1957 to 2014 initiated by the arrival of a shock wave. It has been shown that, as early as the event commencement, the first harmonic of anisotropy tends to increase substantially and its direction changes significantly. The more is powerful the interplanetary disturbance, the greater are the changes. Based on changes in some parameters of anisotropy and density, we can estimate the heliolongitude of the disturbance source, as well as the further development of the Forbush effect and geomagnetic activity. 相似文献
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A. A. Melkumyan A. V. Belov M. A. Abunina A. A. Abunin E. A. Eroshenko V. A. Oleneva V. G. Yanke 《Geomagnetism and Aeronomy》2018,58(2):154-168
The IZMIRAN database of Forbush effects and interplanetary disturbances was used to study features of the action of high-speed solar wind streams from coronal holes on cosmic rays. Three hundred and fifty Forbush effects created by coronal holes without other actions were distinguished. The mean values and distributions have been found for different characteristics of events from this group and compared with all Forbush effects and Forbush effects caused by coronal ejections. Despite the great differences in high-speed streams from coronal holes, this group turned out to be more compact and uniform as compared to events related to coronal ejections. Regression dependences and correlation relations between different parameters of events for the studied groups have been obtained. It has been shown that Forbush effects caused by coronal ejections depend considerably more strongly on the characteristics of interplanetary disturbances as compared to Forbush effects related to coronal holes. This suggests a significant difference between the modulation mechanisms of Forbush effects of different types and corroborates earlier conclusions based on indirect data. 相似文献
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The contribution of resonant wave-particle interactions to the formation and decay of the magnetospheric ring current is analysed in the framework of a self-consistent set of equations which take into account azimuthal plasmasphere asymmetry. It is shown that the cyclotron interaction of westward drifting energetic protons with Alfven waves in the evening-side plasmaspheric bulge region leads to the formation of a ring current asymmetry located near 18:00 MLT. The time-scale of this asymmetry is determined by the proton drift time through the plasmaspheric bulge and is about 1 - 3 h. A symmetrical ring current decays mainly due to charge exchange processes. The theory is compared with known experimental data on ions and waves in the ring current and on low-latitude magnetic disturbances. New low-latitude magnetometer data on the magnetic storm of 24 - 26 July 1986 are also discussed. The model presented explains the observed localization of an asymmetrical ring current loop in the evening sector and the difference in relaxation time-scales of the asymmetry and the Dst index. It also explains measured wave turbulence levels in the evening-side plasmasphere and wave observation statistics. 相似文献