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1.
This article continues our studies of the development of an MHD, waveguide, centrifugalresonance instability as a possible mechanism for the formation of solar magnetic arcades; here, we take into account the non-isentropic nature of this process associated with the presence of dynamical radiative cooling. In contrast to the results of our previous study, our computational data show that five, rather than two, waveguide-resonance families of unstable modes are able to develop in a cylindrical, rotating layer of magnetized plasma. This substantially expands the spectrum of associated wave processes, so that the joint action of all these growing wave harmonics can lead in the non-linear stage of their development to morphologies close to those observed in solar magnetic arcades—to the formation both of the magnetic arcades themselves and of fine structure in such arcades. 相似文献
2.
The development of magnetohydrodynamical centrifugal instability is considered as a possible mechanism for the formation of
solar magnetic arcades. The computations show that the plasma in a cylindrical, magnetized, rotating layer can develop two
families of waveguide-resonance instability modes. These are gyroscopic resonance modes of the rotating, cylindrical layer
and harmonics of fast magnetoacoustic waves that propagate along the forming cylindrical layer and initiate resonance instability
in the layer. The joint action of these two mechanisms is able to produce the observed morphology of solar magnetic arcades. 相似文献
3.
以地下围岩抗爆工程为背景,以小药量模型试验和数值模拟为手段,通过改变空穴位置、形状、组合形式来考察含空穴的防护层对平面爆炸波、球面爆炸波的衰减屏蔽效果。结果表明,含空穴的防护层可以很好地衰减爆炸波的压力峰值,从而达到保护地下洞室的目的;叉排排列的空穴对爆炸压力峰值的衰减效果明显好于顺排,矩形空穴对爆炸波压力衰减效果优于圆形空穴。研究成果为新型围岩抗爆加固技术提供了一定的参考。 相似文献
4.
The stability of synoptic scale waves formed on a frontal surface is studied including nongeostrophic effects with the basic
flow subjected to both vertical and horizontal shear. Spectral method is used to obtain the desired solutions. The stability
characteristics of the developed unstable modes are presented as a function of shears of the basic flow. With the inclusion
of barotropic shear the spectrum of instabilities increase. The lower speeded member of the mixed mode (gravitational-rotational)
pair is influenced by the barotropic shear in the basic current and it appears at lower vertical shears. The structure of
the height perturbations are utilized to distinguish the various unstable modes developed in the system together with their
stability characteristics. This investigation has shown that the ageostrophic effects can be a significant factor in the development
of synoptic scale waves on a frontal surface. 相似文献
5.
《Russian Geology and Geophysics》2014,55(10):1229-1238
Phase change of dielectric magnesiowustite in the lower mantle may leave signatures in geomagnetic records of the globally distributed array of observatories. The related features appear in EM induction responses of lower mantle, which are studied theoretically. The surface EM field corresponding to a response of the earth with conductivity anisotropy in a mantle spherical layer is presented as the sum of the magnetic and electric modes. Equations for the fields of both modes and their relationship in a weakly anisotropic earth are obtained by the perturbation method. The two field modes are analyzed jointly and separately to characterize the conductivity tensor of the anisotropic lower mantle. The tensor elements corresponding to the tangential components of the field can be estimated from the magnetic mode alone recorded currently by the global network of geomagnetic observatories. For the tensor data to be complete, observatory data on lateral variations of the electric field are required in addition to three-component geomagnetic records. 相似文献
6.
The mineralization of bacterial organic matter in the groundwater of Iceland is discussed. Structural relationships between
secondary minerals in cavities within a Pleistocene basaltic sill and the general sequence of their precipitation allowed
us to recognize five stages of the secondary mineral formation. Two stages of layer silicate formation separated by a stage
of zeolite and apophyllite formation were pointed out. The composition and structure of clay minerals formed at different
stages as a result of the interaction between groundwater and basalt with an active participation of bacteria have been investigated.
Clay minerals of the second stage are similar in composition and microstructure to biomorphic structures previously studied
in Miocene plateau basalts. The last stage of mineralization is related to the fossilization of filamentous microbiota residing
in open cavities and covering all older secondary minerals 相似文献
7.
河南灵宝罗山矿区海拔标高640-1100m,山高沟深,地形地貌复杂。自1982年建矿以来,地下采矿工程已在山体下形成大量采空区,这些采空区的变形、破坏和塌陷,加上生产爆破振动等的长期作用与影响,致使矿区目前存在多个受采动影响的潜在滑坡体,并严重影响矿山的正常安全、高效生产。研究、协调并解决采矿与山体稳定性之间的关系,实现在矿山不停产的情况下,完成对矿区山坡的综合治理,成为一项既具有重大经济效益,也具有相当社会影响和环境效益的工程技术难题。针对罗山矿区滑坡体的实际情况,研究指出采空区山体的稳定性具有明显的时间和空间相关特性,随着时间的推移,采矿工程的空间规模会不断扩大,采动影响的空间范围和力度将随之增加。因此,在进行采动诱导山体失稳分析计算以及治理措施研究时,必须充分考虑这种特殊的时空动态影响因素的作用,并采取相应的对策。对于受采动影响的动态不稳定体而言,柔性边坡支护体系比刚性支护体系将更为有效。 相似文献
8.
Two solar radio bursts exhibiting narrow-band millisecond pulsations in intensity and polarization are analyzed. There were considerable time delays between the left-and right-circularly polarized components of the radio emission. The observed oscillations of the degree of polarization are due to the different group velocities of the ordinary and extraordinary modes in their propagation from the source to the observer; the frequency dependence of the delay is in excellent agreement with the theoretically calculated group delay in a magnetoactive plasma. It unambiguously follows that the pulsed radio emission is generated near the double upper hybrid frequency by the nonlinear plasma mechanism, since the source emission has a low degree of polarization. In addition to dispersion effects, a Fourier analysis also reveals effects associated with the source inhomogeneity. We detected a frequency drift of pulsations (autodelays) with different signs for different polarization components. This drift suggests that, apart from the dispersion effects, there are also the effects related to inhomogeneity of the radio source. It is shown, in particular, that the upper hybrid modes (generating the radio emission) are unstable in regions with enhanced gradients of the plasma density and/or magnetic field. 相似文献
9.
A. N. Baushev 《Astronomy Reports》2002,46(10):830-839
The spectrum of cyclotron radiation produced by electrons with a strongly anisotropic velocity distribution is calculated taking into account higher harmonics. The motion of the electrons is assumed to be ultrarelativistic along the magnetic field and nonrelativistic across the field. One characteristic feature of the resulting spectrum is that harmonics of various orders are not equally spaced. The physical properties and observed spectra of four X-ray pulsars displaying higher cyclotron harmonics are analyzed. It was shown that at least in one of them, the cyclotron feature can apparently be only an emission line. Moreover, the observed harmonics are not equidistant, and display certain other properties characteristic of emission by strongly anisotropic ultrarelativistic electrons. In addition, there are indirect theoretical arguments that the electrons giving rise to cyclotron features in the spectra of X-ray pulsars are ultrarelativistic and characterized by strongly anisotropic distributions. As a result, estimates of the magnetic fields of X-ray pulsars (which are usually derived from the energies of cyclotron lines) and certain other physical parameters require substantial revision. 相似文献
10.
以广西柳州白莲洞遗址崖体为研究对象,经地质调查发现,白莲洞遗址崖体存在共计47处不稳定岩体,崖体岩性主要为厚层灰岩,岩溶发育且该厚层灰岩岩体节理裂隙十分发育,存在着诸多危岩体。通过野外地质调查与室内理论分析表明:白莲洞遗址崖体陡峭,灰岩厚层,层理面、构造裂隙、岩溶裂隙和卸荷裂隙发育,在持续暴雨、地震的强有力触发下导致山体松弛,变形加剧,形成了以柱状、楔形体状、块状为主的特大型危岩体,且多处于高位-特高位,从而表现出倾倒、滑移和少量坠落及其复合型的多种破坏模式;其变形破坏绝非突发,厚层块状构造、岩溶发育、坚硬灰岩夹白云岩透镜体及发育的节理裂隙是其形成的主要先天基础因素;降水的渗入、岩溶裂隙水的溶蚀及强烈的根劈作用为其主要触发因素。 相似文献
11.
硅酸盐结构中四面体层立体结构式的表述法 总被引：2，自引：0，他引：2
本文创造一个用立体结构式表述四面体层的方法。首先用四面体Ｕ、Ｄ、Ｖ、Ｈ定向符号组合成结构基元或结构单元。其次把它们在二维空间平移交换（包括平移、滑移、旋转—平移、反伸—平移），得出四面体层的基本符号格式。最后在其固定的位置上标出平移变换的距离和方向、四面体层的厚度和层间连接方式，完成四面体层的立体结构式。由于某些架状硅酸盐结构，可看成是四面体层的叠加，因此，用立体结构式也可表述。 相似文献
12.
A detailed barotropic, baroclinic and combined barotropic-baroclinic stability analysis has been carried out with mean monsoon
zonal currents over western India, eastern India and S.E. Asia. The lower and middle tropospheric zonal wind profiles over
western India are barotropically unstable. The structure and growth rate of these modes agree well with the observed features
of the midtropospheric cyclones. Similar profiles over eastern India and S.E. Asia, however, are barotropically stable. This
is attributed to weak horizontal shear, inherent to these profiles. The upper tropospheric profiles, on the other hand, are
barotropically unstable throughout the whole region. The features of these unstable modes agree with those of observed easterly
waves. The baroclinic and combined barotropic-baroclinic stability analyses show that the baroclinic effects are not important
in tropics.
Though the barotropic instability of the mean zonal current seems to be res ponsible for the initial growth of the mid-tropospheric
cyclones, neither barotropic nor baroclinic instability of the mean zonal current seem to explain the observed features of
the monsoon depressions. 相似文献
13.
渝利铁路青石岩段为深切河谷型边坡,该边坡表部岩体在风化缷荷作用下结构复杂且稳定性差。此外,浅表层岩体在降雨、地震及工程开挖等影响下,局部已经出现了不同模式不同规模的变形失稳现象,严重影响工程建设和运营期间的安全。因此,本文根据边坡岩体结构特征及风化缷荷特征等工程地质条件,结合不同失稳模式的危岩体,提出了相应的稳定性评价理论和方法。最后,针对不同规模和不同稳定状态下的危岩体提出了有效的防治措施。 相似文献
14.
A model for the nonradial motion of an eruptive prominence in the solar corona is proposed. Such motions, which can sometimes be inaccessible to observation, result in an apparent break in the causal link between eruptive prominences and coronal mass ejections. The global magnetic field of the Sun governs coronal plasma motions. The complex structure of this field can form prominence trajectories that differ considerably from a simple vertical rise (i.e., radial motion). A solar filament is modeled as a current-carrying ring or twisted toroidal magnetic rope in equilibrium with the coronal magnetic field. The global field is described using two spherical harmonics. A catastrophic violation of the filament equilibrium followed by its rapid acceleration—eruption—is possible in this nonlinear system. The numerical solution of the equations of motion corresponds well to the eruption pattern observed on December 14, 1997. 相似文献
15.
对安徽凤阳石英砂工业区土壤剖面的磁学参数和SiO2含量进行测试,结果显示：土壤剖面磁性矿物含量低,磁学性质由磁赤铁矿控制,土壤剖面由上而下可分成3个磁性层;从第一层到第三层磁性逐渐减弱;第三层磁学性质主要由成土母质决定,第一层存在明显的磁性增强现象,引起这种现象的原因可能是次生磁赤铁矿和燃烧作用。磁学参数和SiO2含量显示土壤剖面的第一层已被弱磁性石英尾砂污染,在石英尾砂的稀释作用下,其磁性结构特征发生了改变,磁性矿物含量降低。土壤剖面的磁学参数组合特征及SiO2含量反映了弱磁性石英尾砂对第一层土壤的污染过程。 相似文献
16.
结合四川省甘孜州德格县城区色曲河左岸城区不稳定斜坡治理的具体工程实例,通过野外地质勘查,查明了该地区斜坡地形地貌、地层岩性、岩土体结构特征和水文地质条件。在此基础上对该地区进行了边坡变形机理和破坏模式特征研究,以及斜坡稳定性评价分析。并根据上述研究成果,提出了德格县城区色曲河左岸城区不稳定斜坡的治理方案,此方案为相关部门进行地质灾害治理提供了决策支持依据。 相似文献
17.
Quasi-biennial oscillations (QBOs) can clearly be distinguished in uniform series of data on the solar magnetic-field polarity derived from Hα observations in 1915–1999. These have been proven to represent oscillations of the global magnetic field of the Sun. This is verified by spectral analyses executed using various methods: the QBOs are clearly visible in low harmonics (l=1–3), but abruptly disappear for l=4 and higher. First and foremost, the QBOs are displayed in variations of the sector structure of the large-scale magnetic field, demonstrating that they correspond to variations of the horizontal multipoles. 相似文献
18.
在遥感解译、野外调查的基础上,采用高密度电法和电阻率测深法,并结合钻探对川西岷江河谷发育的尕米寺滑坡、俄寨村滑坡、格机寨滑坡等典型大型—巨型古滑坡的空间结构进行了勘探分析,有效确定了古滑坡的空间结构和滑带特征,并认为古滑坡的滑动面多具有高低阻相间的不稳定电性层,且滑坡前缘多位于不稳定电性层变薄收敛的地方。其中,俄寨村滑坡高低阻相间的不稳定电性层厚约0~45 m,为滑坡堆积层,古滑动面紧贴基岩面,滑动面平均埋深约30 m,弱风化基岩面埋深约5.6~61 m,强风化层厚约为3~12 m;尕米寺滑坡高低阻相间的不稳定电性层厚约2.5~43 m,为滑坡堆积层,沿剖面古滑动面平均埋深约35 m,在滑坡中部存在一圈闭的低阻异常体,推测为古河道,并与钻探结果相吻合,其埋深约56~96 m,弱风化基岩面埋深13.3~100 m,强风化及岩溶综合层厚一般约为5~20 m。基于古滑坡的地球物理勘探数据和解译结果,统计分析了川西岷江河谷地区大型—巨型古滑坡空间岩土体的地球物理物性参数,对指导该区滑坡调查分析具有重要的指导意义。 相似文献
19.
Variations in the positions of the intersection points of tangents to ray structures in the polar corona of the Sun during the solar cycle are considered. At first glance, the decrease in the distance q between the tangent intersection point and the center of the solar disk during activity maximum contradicts harmonic analyses that indicate that the relative weight of higher harmonics in the global field increases during this period. Indeed, the higher the harmonic number in an axisymmetric field, the closer the intersection point of the field-line tangents (the magnetic focus) to the solar surface. It is shown that q for a field composed of two harmonics with opposite polarities at the poles can be smaller than q for either of them taken alone. A simple model representing the global field using the third and seventh harmonics is analyzed; this model can reproduce quite satisfactorily the observed dynamics of magnetic foci of the polar field. 相似文献
20.
Variations in the mean solar magnetic field (MSMF) are studied in both the frequency-time and longitude-time domains. A wavelet analysis of the MSMF clearly demonstrates that variations in the mean field are not stationary. Combined with longitude-time diagrams for the background solar magnetic field (BSMF), the analysis reveals the emergence of the background field, which occurs discretely at intervals of 1.5–2 years. Based on an analysis of the fine structure in MSMF variations, we develop a numerical technique to study timedependent heliographic-longitude distribution of the large-scale magnetic field. A detailed picture of the rotation of the large-scale magnetic field is derived for activity cycles 20–23. Coherent structures are detected in longitude-time diagrams obtained by deconvolving the MSMF series. These structures are related to discrete rigid-rotation modes of the large-scale magnetic fields. Various rotational modes coexist and replace one another. During the phase of activity growth, modes with periods of 27.8–28.5 days dominate, whereas a mode with a rotational period of about 27 days dominates during the decline phase. Occasionally, modes with periods of 29–30 days appear. Most structures in the longitude-time MSMF distribution correspond to similar structures in the BSMF distribution for the northern or southern hemisphere. Chronologically, the emergence of the BSMF has frequently been accompanied by changes in the solar rotational regime and has been correlated with variations in the polarity asymmetry in the course of the 11-year activity cycle. 相似文献