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根据采用动力学方程对亚暴期间磁尾磁场向偶极形弛豫过程中离子分布函数的模拟结果 ,研究了磁尾来自电离层的O+,H+和He+离子的速度及能量随时间的变化 .主要结果为 :（1 ）离子的加速及能量变化主要发生在磁场偶极化过程的中期 ,对应的地心距离位于- 1 2RE到 - 8RE 之间 ;（2 ）垂直于磁场方向上离子加速及能量变化较快 ,平行方向上较慢 ;（3）轻离子较重离子加速及能量变化快 ,磁场偶极化终结 ,3种离子的能量均可增加 2 0 0倍左右 ;（4）初始能量较高时 ,离子加速及能量变化较快 ,离子最终获得的能量较大 .理论计算的磁尾离子能量在磁场偶极化过程终了可达 1 0 2 keV的量级 ,这与观测结果一致 . 相似文献
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曹馨 濮祖荫 张辉 傅绥燕 马志伟 肖池阶 刘振兴 谢伦 Dunlpo M. W. Korth A. Frazen M. Zong Q. G. Lueck E. Carr C. Reme H. 《地球物理学报》2007,50(4):995-1004
利用TC1、Cluster和Polar结合极光和同步高度及地磁的观测，研究了2004年9月14日1730～1930 UT时间段的亚暴偶极化过程.此前行星际磁场持续南向几个小时.亚暴初发(Onset)开始于1823 UT.2 min之后，同步高度的LANL 02A在子夜附近观测到了明显的能量电子增强（Injection）事件，而TC1在1827UT左右在磁尾(-10,-2, 0)RE (GSE)观测到了磁场BX的突然下降，伴随着等离子体压强和温度的突然增加及磁场的强烈扰动.在(-16, 1, 3)RE (GSE) 的Cluster上相同的仪器观测到相同的现象，只是比TC1观测到的晚大约23 min，在1850 UT左右.虽然Polar在更靠近地球的较高纬度(-75, 35, -40)RE (GSE)附近，也在1855 UT左右观测到了这种磁场偶极化现象.以上的观测时序表明TC1、Cluster观测到的磁场偶极化比亚暴偶极化初始发生分别晚4 min和27 min.说明偶极化由近磁尾向中磁尾传播.详细计算表明偶极化源区的位置大约在X=-77RE～-86RE，而传播速度大约为70 km·s-1.在这个事件中亚暴的物理图像可能是中磁尾的近地重联产生的地向高速流到达近磁尾，为近磁尾的亚暴触发创造了条件；亚暴在近磁尾触发之后，磁场偶极化峰面向中磁尾传播. 相似文献
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用三维可压缩MHD数值模拟研究了在磁场重联过程中电子压力梯度项的效应研究结果发现在较高等离子体β,较小离子惯性尺度条件下,广义欧姆定理中压力梯度项在重联过程的作用不可忽略.在磁重联过程中,压力梯度项虽然没有明显改变磁场拓扑结构和重联速度,但它使电子和离子速度明显增大.由于在离子惯性尺度下,离子和电子运动解耦,电子是电流的主要载流子,所以场向电流也增大,并导致核心磁场明显增大.考虑到场向电流是磁层电离层耦合的一个重要因素,所以电子压力梯度项的引入加强了行星际磁场南向期间磁层电离层的耦合.电子压力梯度项还在重联区激发了波动,该波动可向重联区外传播. 相似文献
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《中国科学:地球科学》2015,(10)
TC-2卫星上的中性原子成像仪(NUADU)在2005年5月15日磁暴期间(并伴随有系列亚暴事件)记录了反映环电流离子连续变化的能量中性原子(ENA)图像探测数据.比较由中性原子图像反演的4 min时间分辨的环电流离子空间分布与地球同步轨道LANL系列卫星(环绕赤道面~6.6 RE)上同步轨道粒子分析仪(LANL-SOPA)原位离子通量探测数据,以及相同高度的同步系列卫星GOES的磁场数据,发现环电流区离子通量增长发生在磁力线尾向拉伸的亚暴增长相阶段,而不是发生在磁场偶极化之后.这一发现挑战了以往的环电流离子注入是磁场偶极化时由磁尾直接注入的概念,但仍需更多的观测实例进一步认证. 相似文献
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等离子体片离子向内磁层的渗透在亚暴和磁暴过程中都起到了重要作用.以往对于等离子体片离子向内磁层的渗透都是通过固定磁矩的磁层离子漂移轨道理论来进行的.本文将过去的(U,B)空间中固定磁矩的磁层离子漂移轨道理论扩展为固定能量的磁层离子漂移轨道理论,讨论了等离子体片质子在向地球输运过程中,不同能量的质子开放轨道和封闭轨道的分界线的特性,及其随Kp指数的变化.在高能端,随着能量的升高,等离子体片质子分界线地心距离逐渐增大,且分界线的晨侧地心距离远远大于昏侧的地心距离.在低能端,随着质子能量的降低,质子分界线地心距离逐渐增大,且其分界线的昏侧地心距离要大于晨侧的地心距离.模拟结果还显示随着Kp指数的增强,等离子体片中不同能量的质子分界线都向地球移动.但在低能端和高能端,质子分界线的行为是不一样的.在低能端,随着Kp指数的增大,质子内边界形状基本保持不变.但在高能端,随着Kp指数的增大,质子内边界形状也将发生变化.在E=20 keV,Kp=6和E=10 keV,Kp=3两种情况,质子分界线甚至出现了两个分离的区域,一个是环绕地球的封闭轨道区域,一个是晨侧孤立的锥型区域.等离子体片能量为E的质子的内边界就是具有不同磁矩的Alfven层上能量为E的点的连线.TC-1热离子谱仪对等离子体片离子内边界的观测显示模拟结果与观测结果符合得很好. 相似文献
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采用动力学方程,对亚暴期间磁尾磁场向偶极形弛豫过程中离子分布函数的演化进行了模拟研究,主要结果为：（１）初始时刻分布函数为相对于速度呈指数下降的离子束,在随时间变化过程中,逐渐变为相对于速度（包括平行和垂直速度）的单峰结构,且单峰在速度空间的位置随时间的变化而向高速方向移动;（２）在速度空间中平行于磁场方向上单峰向高速方向移动得较慢,在垂直方向上移动得较快;（３）轻离子分布函数峰值的位置较重离子随时间的变化向高速方向移动较快。（４）初始能量较高时,离子分布函数的单峰位置向高速方向移动较快。（５）离子团在磁场偶极化过程中表现为一束地向流．本文还对上行离子受感应电场的加速进行了讨论． 相似文献
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相比于传统弹性波动方程,非对称弹性波动方程增加的独立自由项,包含有介质特征尺度参数.基于非对称弹性波动方程,可以分析弹性波传播中,由介质内微孔缝隙结构相互作用所导致的地震波传播尺度效应.本文从介质应变能密度函数出发,并结合几何方程和平衡方程,给出修正偶应力理论下的非对称弹性波动方程以及对应的非对称SH型横波波动方程的数学表达式,并在三层煤层模型上进行数值模拟,将检波器分别设置在地表和煤层中线,通过改变介质特征尺度参数值,合成地震记录,研究分析弹性波传播中,由介质内微孔缝隙结构相互作用所导致的尺度效应,对地震记录的影响及规律,并得出以下结论和认识:(1)非对称弹性波动方程模拟的弹性波传播表现出明显的尺度效应;(2)地震记录需要考虑介质内部多尺度的微孔缝隙相互作用的影响. 相似文献
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2004年7月14日TC-1卫星在近地磁尾(-9.3Re,-5.4Re,1.2Re)附近观测到了伴随有持续尾向流的等离体片变薄和偶极化过程.尾向流持续时间为32分钟.偶极化过程中磁场By分量没有明显变化.在偶极化过程发生两分钟之后,地面台站观测到的Pi2脉动.ACE卫星的观测表明行星际磁场有弱的南向行星际磁场（-2nT）,持续时间约55分钟.Imagine卫星在电离层区域没有观测到极光出现.和伴随有极光增亮的亚暴过程相比,南向行星际磁场明显较弱,且持续时间短.TC-1卫星和ACE卫星的联合观测表明尾部释能有大有小,并非达到某值才能发生.但能量小时,不能够引起极光亚暴.其次南向行星际磁场有可能与近地磁尾尾向流有密切关系. 相似文献
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Yutaka Nakamura Akira Fukukita Kazuo Tamura Issei Yamazaki Taichi Matsuoka Kazuhiko Hiramoto Katsuaki Sunakoda 《地震工程与结构动力学》2014,43(4):507-527
This paper presents a new type of electromagnetic damper with rotating inertial mass that has been developed to control the vibrations of structures subjected to earthquakes. The electromagnetic inertial mass damper (EIMD) consists of a ball screw that converts axial oscillation of the rod end into rotational motion of the internal flywheel and an electric generator that is turned by the rotation of the inner rod. The EIMD is able to generate a large inertial force created by the rotating flywheel and a variable damping force developed by the electric generator. Device performance tests of reduced‐scale and full‐scale EIMDs were undertaken to verify the basic characteristics of the damper and the validity of the derived theoretical formulae. Shaking table tests of a three‐story structure with EIMDs and earthquake response analyses of a building with EIMDs were conducted to demonstrate the seismic response control performance of the EIMD. The EIMD is able to reduce story drifts as well as accelerations and surpasses conventional types of dampers in reducing acceleration responses. Copyright © 2013 John Wiley & Sons, Ltd. 相似文献
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Michael E. McCormick 《地震工程与结构动力学》1989,18(2):199-216
Expressions for both the rectilinear and rotational inertial and damping coefficients for a circular monolithic tower of uniform radius are derived. The analysis matches the fluid velocity, derived from potential theory, with the structural velocity in sway. That is, the motions of the tower are assumed to be in a vertical plane. The analysis is then applied to a tower composed of (lumped-mass) elements, where the expressions for the added-mass and damping coefficients are shown to be functions of wave number. The added-mass is shown to be a product of two wave systems: a travelling wave system, which is responsible for the radiation damping, and a standing wave system, called the evanescent system, which is attached to the structure. The added-mass of the evanescent system is negative for small wave numbers, while that of the travelling waves is positive. The negative sign simply means that the inertial force of the evanescent waves is 180° out of phase with that of the travelling system. Furthermore, it is shown that the contributions of the two wave systems to the total added-mass of the structure counteract each other, resulting in a total added-mass which varies gradually with the wave number. Finally, the analysis is applied to an experiment, and results of the analysis and the experiment are found to agree rather well. 相似文献
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本文通过利用包含离心力的自洽、轴对称稳态木星磁层模型,以及等离子体细丝运动理论对磁尾重联产生的磁通量管向内输运进行研究.基于细丝运动理论模型,通过MHD数值模拟我们可以得到磁通量管随时间变化的许多特性.模拟结果表明,重联产生的磁通量管向内运动可到达10RJ以内,磁通量管赤道部分的速度可以达到350km·s-1左右,表现出很强的向行星方向的流动.初始磁通量管中的等离子体密度和压强均小于周围介质,随着它迅速向木星方向运动,它的等离子体密度由于体积压缩逐渐上升,等离子体压强则逐渐上升到与周围介质相当.磁通量管在电离层上足点向赤道方向的运动滞后于它在赤道面上向行星方向的运动. 相似文献
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Pavel N. Mager Dmitri Yu. Klimushkin Nickolay Ivchenko 《Journal of Atmospheric and Solar》2009,71(16):1677-1680
An often observed and still unexplained feature of the high-m Alfvén waves in the terrestrial magnetosphere is their equatorward phase motion, in contrast with low-m waves. We suggest an explanation of this fact in terms of a model of wave excitation by an azimuthally drifting particle inhomogeneity injected during substorm activity. The azimuthal direction of the phase velocity coincides with that of the cloud. If the drift velocity increases with the radial coordinate, the particle cloud is stretched into spiral in the equatorial plane which leads to a radial component of the phase velocity directed toward Earth, that is, an equatorward phase propagation. 相似文献
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N. I. Izhovkina I. S. Prutensky S. A. Pulinets N. S. Erokhin L. A. Mikhailovskaya Z. Klos H. Rothkaehl 《Geomagnetism and Aeronomy》2009,49(2):210-218
The measurements of the broadband wave radiation in the topside ionosphere in the region of the geomagnetic equator (the APEX satellite experiment) are presented. The region of unstable plasma with increased density was observed in the nightside topside ionosphere. This region could be formed by heating of the ionosphere from below. An asymmetric distribution of the frequency band width and electrostatic radiation intensity relative to the geomagnetic equator was registered. It has been indicated that a substantial effect of the geomagnetic equator on plasma diffusion from the heating region could be related to the generation, propagation, and damping of electrostatic oscillations and large-scale (as compared to the Larmor ion radius) plasma vortices. The anisotropy in the temperature of the plasma electron component can increase in the regions where the transverse electric field of disturbances damps. The intensity of the electromagnetic radiation, caused by the external sources, apparently, of an artificial origin at frequencies higher than the local plasma frequency, decreases to the radiation detection threshold level in the region of increased plasma density. 相似文献
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针对地震-台风耦合作用下的近海导管架海洋平台,运用Morison方程将台风对导管架平台的拖曳力及波浪对导管架平台的拖曳力和惯性力施加在结构上,并在基底施加地震动,建立地震-台风耦合作用下的运动方程。通过模态分析,确定结构的基本自振频率,进而选取卓越频率与该频率较为接近的海底地震动进行输入。对通过数值模型计算得到的导管架平台动力响应,参考相关文献中的限值,对耦合作用下的平台进行安全评估,给出了近海导管架海洋平台在地震-台风耦合作用下的损伤状态评定标准。本文关于导管架平台动力响应的统计结果,对导管架结构性态设计具有一定参考意义。 相似文献
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Eunjong Yu Daniel H. Whang Joel P. Conte Jonathan P. Stewart John W. Wallace 《地震工程与结构动力学》2005,34(7):737-761
This paper describes the development and numerical verification of a test method to realistically simulate the seismic structural response of full‐scale buildings. The result is a new field testing procedure referred to as the linear shaker seismic simulation (LSSS) testing method. This test method uses a linear shaker system in which a mass mounted on the structure is commanded a specified acceleration time history, which in turn induces inertial forces in the structure. The inertia force of the moving mass is transferred as dynamic force excitation to the structure. The key issues associated with the LSSS method are (1) determining for a given ground motion displacement, xg, a linear shaker motion which induces a structural response that matches as closely as possible the response of the building if it had been excited at its base by xg (i.e. the motion transformation problem) and (2) correcting the linear shaker motion from Step (1) to compensate for control–structure interaction effects associated with the fact that linear shaker systems cannot impart perfectly to the structure the specified forcing functions (i.e. the CSI problem). The motion transformation problem is solved using filters that modify xg both in the frequency domain using building transfer functions and in the time domain using a least squares approximation. The CSI problem, which is most important near the modal frequencies of the structural system, is solved for the example of a linear shaker system that is part of the NEES@UCLA equipment site. Copyright © 2005 John Wiley & Sons, Ltd. 相似文献
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The kinematic soil–foundation interaction changes the free field ground motion to a different motion at the foundation of a structure. This interaction effect may be expressed by the ratio of the peak horizontal acceleration of a rigid and relatively lightweight foundation to the peak horizontal acceleration at the ground surface in the free field. It is found that the interaction effect can be defined by a simple function of the ratio of the peak horizontal ground velocity and ground acceleration in the free field, the length of the foundation and the shear wave velocity in the soil. Predictive equations for the kinematic soil foundation effect are derived using 350 strong motion records generated by 114 earthquakes world-wide. At the same time, an attenuation relationship is derived for the ratio of the peak horizontal ground velocity and acceleration from the same set of data. Ten case histories are studied; the interaction effects are calculated by using the predictive equations and then compared with measured field values. The results of the comparison illustrate the degree of predictive capability of the method when the foundation mass and the inertial soil–foundation interaction are not considered. 相似文献