共查询到17条相似文献，搜索用时 250 毫秒
1.
磁通门磁力仪的零位偏移量在卫星轨道上会因诸多因素而发生改变.为此,基于剪切阿尔芬波动不改变总磁场强度这一特征的Davis-Smith方法被提出用于计算磁力仪的零位补偿.实际上,行星际空间中没有纯粹的阿尔芬波动.本文采用数值模拟分析了存在小的压缩波动情况下,阿尔芬波动的幅度、周期和相位以及数据窗口时间长度等对Davis-Smith方法计算零位补偿的影响.我们发现,只有当阿尔芬波动的周期与压缩波动周期相同时,阿尔芬波动的性质会对零位补偿的计算产生不可忽视的误差.阿尔芬波动的幅度越大,零位补偿的误差越小.磁场各分量零位补偿的误差大小还会受到阿尔芬波动初始相位的影响.此外,数据窗口时间长度越长,则零位补偿误差趋于减小至真实值. 相似文献
2.
本文利用信使号飞船2011-2015年期间在轨磁场数据对水星磁尾电流片的磁场结构分布特征进行了统计分析.为探究磁场结构分布随水星径向距离的变化,电流片划分为近磁尾（-1.5RM > X > -2.0RM）和远磁尾（-2.0RM > X > -2.5RM）两个区域.所得结果表明：（1）无论是近磁尾还是远磁尾,电流片中的磁场都以+Bz分量为主,磁场方向几乎与磁赤道面垂直.（2）相比近磁尾,远磁尾电流片中磁场强度、Bz分量较弱,By分量较强,而且-Bz信号出现概率相对较大,这表明电流片中磁活动相对容易在远磁尾中发生.（3）磁场强度以及Bz分量在晨昏方向上的分布存在晨昏不对称性——在方位角120°~190°范围内相对较弱.弱Bz数据点（Bz<5 nT）也在昏侧（Y>0）发生较为频繁.（4）与Bz分布相反,磁场强By分量（|By|>5 nT）倾向于在晨侧（Y<0）发生.统计分析还表明,磁场By分量与行星际磁场By分量并无明显的相关性.对比地球磁尾电流片,我们对水星磁尾电流片Bz分量、强By分量的晨昏不对称起源机制作了探讨分析. 相似文献
3.
利用Cluster卫星数据,选取2001—2010年期间的616个极尖区穿越事件,研究了行星际磁场（IMF）的大小和方向对极尖区位形的影响.结果表明：当Bz为北向时,随着Bx负向的增大,极尖区的磁不变纬度向高纬方向（极区）移动;当Bz为南向时,随着Bx负向增大,极尖区的磁不变纬度略微向低纬度方向（赤道）移动.Bx正向增大时,极尖区并没有明显移动.Bx对极尖区影响在南半球较为显著,在北半球没有明显规律性变化.此外,随着行星际磁场锥角的增大（>90°）,极尖区也随之向高纬移动.当Bz南向时,随着By的负向增大,极尖区在北半球向晨侧移动,在南半球向昏侧移动.而当Bz南向增加时,南北半球两个极尖区的磁不变纬度都朝赤道方向移动;但北向Bz时几乎没有移动. 相似文献
4.
5.
以场源为分类原则,地电场E由自然电场ESP和大地电场ET构成.ESP起源于地下介质物理、化学作用,通常其变化及稳定性具有明显的局部场地特征;ET起源于空间电流系和潮汐力,在日变波形、频谱特征上表现出广域性.在形成微观机理方面,ESP和ET能够具有部分相同的机理过程.2008—2013年,在南北地震带附近13个代表性场地,多数ESP不具有清晰的年变波形,其稳定性也受区域、场地、方位、构造活动等因素影响.在这些地区,ESP较平稳的持续升降、快速跃变、突跳等现象常见,同一主断裂带附近或局部区域内,这些大幅变化的趋势转折点多具有时间同步或准同步性,同一时段数据稳定性可能类似,但形态变化存在场地因素而不具相关性.ESP较平稳期间,应用潮汐地电场频谱特征计算的裂隙水主体渗流方位α易处于相对稳定状态,而在其剧烈变化期间的α常会明显变化.以潮汐地电场频谱特征逐日计算α值,可能揭示场地裂隙、裂隙水渗流、主压应力的逐日变化信息,进而可解析ESP、ET宏观变化的微观机理过程. 相似文献
6.
准确的磁场测量对深入研究空间等离子体环境具有重要意义.星载磁通门磁强计的磁补偿随时间缓慢变化,因此,需要对其进行常规的在轨标定.现有的在轨标定方法都依赖于磁扰动或磁结构事件的筛选,导致标定结果的频次受限于事件的筛选,且差的事件还会增大计算误差.为此,本文研发出一种不依赖于磁场事件筛选的在轨标定新方法.根据行星际磁场强度的取值范围,我们可建构一个磁补偿取值空间.不同的磁补偿值会影响行星际磁场的阿尔芬特性;于是,我们通过在磁补偿空间中找到使被调整之后的行星际磁场的阿尔芬特性最强的点作为磁补偿值的最优解.测试结果表明,我们的新方法可以利用1～4 h时长的行星际磁场数据获得误差小于0.1 nT的标定结果. 相似文献
7.
本文基于二维三分量可压缩磁流体动力学模拟，数值研究由于磁力线足点在光球层的剪切运动引起日冕电流片中的磁场重联过程。结果表明，磁力线足点的剪切运动作为引起强迫磁场重联的一种触发机制，将加速磁场重联的发展和磁岛的合并过程。结合不稳定性导致等离子体急剧加速，在β∞＝０．１的情况下其加速度达到０．３４νＡ∞／τＡ，等离子体的最大下落速度可达１．９０νＡ∞，大于纯电阻撕裂模情况。还讨论了β∞值对这种磁场重联过程的影响。β∞值越小，磁场重联和磁岛合并过程发展得越快。 相似文献
8.
核磁共振测井在火成岩地层应用的适应性分析 总被引：1，自引：0，他引：1
火成岩岩石具有高磁化率特征,与沉积岩差别明显,岩石的高磁化率会对核磁共振信号产生显著影响,开展核磁共振测井在火成岩地层应用的适应性分析研究,为广泛使用核磁共振测井用于火成岩储层评价提供参考.采用理论模拟、实验分析及实际测井资料相结合的方法,分析了高磁化率岩石的核磁共振响应特征.分析结果表明,火成岩岩石具有很高的磁化率,从酸性火成岩到基性火城岩,岩石的磁化率一般是逐渐增大的.高磁化率岩石孔隙内部会产生强梯度磁场,孔隙内部的磁场梯度越强,核磁共振的T2谱前移越明显,核磁信号衰减幅度也越大,核磁分析孔隙度与常规分析的孔隙度误差也越大;相同岩石磁化率情况下,岩石孔径越小,岩石孔隙内部磁场梯度越强,核磁信号衰减越大,核磁共振测井计算的孔隙度也越低.因此,核磁共振测井与岩性有关系,核磁共振测井会受到高磁化率岩石的显著影响.核磁共振测井在部分火成岩,尤其在中基性火成岩和小孔径火成岩储层中应用具有很大的局限性. 相似文献
9.
2004年8月3日近地TC-1卫星在磁尾XGSM~－12RE的等离子体片内,观测到了伴随着高速流的低于离子回旋频率的波,即超低频波(ULF,Ultra Low Frequency).该波垂直分量的振幅在高速流及其振荡减速期间大致相当;而平行分量振幅在高速流时明显大于其振荡减速时. 利用一个扰动双流模型对完全磁化离子横场漂移驱动的电磁不稳定性计算后,预测结果表明:(1)对于垂直分量来说,横场漂移速度与Alfvén速度的比值影响不稳定性增长率和激发波频率,随其比值增加,增长率变大,激发波频率从负值增加到正值.(2)对于平行分量来说,温度各向异性时等离子体热速度与Alfvén速度比值只影响不稳定性增长率和激发波频率,未改变不稳定性模类别;而温度各向同性时离子横场漂移速度与Alfvén速度比值既影响不稳定性模的种类及其分支,又影响激发波频率.进一步将卫星观测到的等离子体密度、温度、整体流速和磁场代入模型方程,进行数值计算与上述预测结果对比后发现:卫星观测中垂直分量的功率谱密度(PSD,Power Spectrum Density)增强时间和频段与理论模型中由β//、β⊥和v⊥/VA引起不稳定性激发的波一致;卫星观测中平行分量的功率谱密度增强时间与理论模型基本相符,但是前者的频率明显地低于后者.因此,除了需考虑平行磁场的离子整体流速对不稳定性激发波频率的可能影响,还需要统计上进一步核实伴随有高速流的ULF波与不稳定性的相关性. 相似文献
10.
研究金属套管对低频电磁场各分量透射信号和反射信号的影响规律对采用过套管电磁感应测井技术监测生产过程中的流体移动具有重要价值.采用柱状成层各向异性介质中的并矢Green函数模拟当发射源在套管内、接收器分别在套管内和套管外时多分量电磁感应的响应,并系统分析了金属套管对透射磁场和反射磁场各主分量的影响规律.计算结果表明,无论是透射场还是反射场,由于所采用的频率较低,金属套管对每个分量信号的影响可以与地层对该分量信号的影响分开.在低频段,磁性金属套管对磁场各分量仍存在稳定的反射,但不同分量被反射的程度不同,受套管磁屏蔽作用大的分量(如ρρ分量)被反射的程度高于受套管磁屏蔽作用小的分量(如zz分量).随着频率的升高,反射磁场的强度逐渐增大并最终达到饱和,信号被全反射.磁性金属套管的存在导致透射磁场各分量出现不同程度的幅度衰减和相位延迟,受套管磁屏蔽作用大的分量的幅度衰减程度大.在固定套管参数和频率的情况下,磁性套管对透射磁场不同分量的影响程度虽然不同但是恒定,其所导致的各分量的幅度衰减和相位延迟与线圈系位置和地层电参数无关.在低频段,套管外透射场的各分量处于准静态,其幅度和相位均不随频率而改变,受套管磁屏蔽作用大的分量的幅度随套管磁导率和厚度的不同而存在明显变化.当频率超过某一临界值后,套管的影响逐渐从以静态屏蔽为主转到以趋肤效应为主,导致透射场幅度的衰减和相位的延迟,套管的厚度越大、套管的电导率和相对磁导率值越大,所对应的频率临界值越小. 相似文献
11.
Thermal instabilities in the form of oscillatory magnetoconvection representing diffusively modified Alfvén waves in an electrically-conducting Bénard fluid layer of rigid walls in the presence of a vertical magnetic field are investigated. Emphasis of the article is on the transition from a nearly undamped Alfvén wave to diffusively modified Alfvén waves, and on the effect of physically realisable magnetic field boundary conditions on magnetoconvection. It is found that the extra magnetic dissipation in the magnetic Hartmann boundary layers can enhance oscillatory magnetoconvection in the form of strongly modified Alfvén waves. Oscillatory magnetoconvection produced solely by the Alfvén wave mechanism can be the most unstable mode even in the presence of a strong viscous effect. This article also represents the first study on the effect of an electrically conducting wall on magnetoconvection which is associated with a nonlinear eigenvalue problem. We find that the electrically perfectly conducting condition does not yield a good approximation for magnetoconvection with an electrically highly conducting wall. The size of oscillation frequency with an electrically highly conducting wall can be more than a factor of 2 larger than that obtained using the perfectly conducting condition. 相似文献
12.
《Journal of Atmospheric and Solar》2000,62(4):311-322
A Pc1/IPDP event recorded by the Finnish search coil magnetometers on 15 December 1984 was analyzed in a companion paper (Mursula et al., 2000. Non-stationary Alfvén resonator: new results on Pc1 pearls and IPDP events. J. Atmos. Solar-Terr. Phys. 62(4), 299–309) using numerical simulations of the ionospheric Alfvén resonator (IAR). EISCAT incoherent scatter radar data were used to determine the vertical profiles of ionospheric plasma parameters. In this paper, the detailed altitude profiles of several wave characteristics at the IAR eigenfrequency are computed up to 1000 km height, including, e.g., the real normalized amplitude of the magnetic wave field component, ellipticity and orientation of the polarization ellipse in the horizontal plane. We also calculate the altitude profile of the energy flux density (Poynting vector). These features illustrate in detail the ionospheric effects on the wave spectral structure in a non-stationary IAR, and their significance in the formation of the Pc1/IPDP signal on the ground. 相似文献
13.
N. A. Zolotukhina 《Geomagnetism and Aeronomy》2009,49(4):438-449
It has been indicated that the magnetic field variations, registered by the geostationary satellites in the range 150–600 s after 14 SI/SC events, include transverse wave components that show the spectral—polarization properties of standing Alfvén waves. The amplitude of these waves increases with increasing pulse amplitude, the period increases with decreasing magnetic field magnitude, and the rotation direction and magnetic field vector orientation reverse their signs near the noon and midnight meridians. 相似文献
14.
《Journal of Atmospheric and Solar》2000,62(4):231-238
A self-consistent model for the generation of Pc 1 pearl emissions based on the nonlinear coupling between the magnetospheric and ionospheric resonators for Alfvén waves is considered. Formation of pearls is attributed to the pulsating regime of the Alfvén sweep maser with nonlinear selective mirrors. Such mirrors are formed by the conjugate ionospheres: their reflection coefficient has an oscillatory frequency dependence due to eigenmodes of the ionospheric Alfvén resonator. Nonlinear magnetosphere/ionosphere feedback is provided by the dependence of the value and frequency of the reflection maxima on the flux of energetic protons precipitated into the ionospheres in the course of Alfvén wave generation in the magnetosphere. A nonlinear soliton-like solution of this model is found which corresponds to a single wave packet having the positive frequency drift and oscillating between the conjugate ionospheres. Properties of this solution are shown to explain many observational characteristics of Pc 1 pearls, such as their morningside predominance, correlation with low magnetic activity, spatio-temporal and spectral patterns. 相似文献
15.
仪器定向误差对地磁日变化记录 准确度的影响研究 总被引：1，自引：1，他引：0
基于红山地磁台磁通门磁力仪GM4-2记录的日变化数据, 提出了一种减小仪器定向误差的方法, 即D要素磁轴零场漂移S0校正法. 首先基于零场漂移S0测量原理, 试制测量工具无磁旋转平台, 并对磁力仪GM4-2零场漂移S0值进行测量, 得出该值约为1024.7 nT; 然后在重新定向时对该数值进行误差校正; 最后将较正后的零场漂移S0值应用到理论日变化数据和定向后的实际日变化数据中. 结果表明, D要素磁轴零场漂移S0是产生定向误差的主要因素, 经过零场漂移S0校正后的日变化数据与理论日变化数据一致, 消除了由定向误差所造成的日变化畸变, 从而能更真实地反映地磁场变化. 相似文献
16.
The behaviour of the magnetic field variations over the North China-Korea coastal region is studied with the aid of a scaled laboratory analogue model. The model source frequencies simulate naturally occurring geomagnetic variations of 3–60 min periods. In-phase and quadrature magnetic Bx, By and Bz field measurements for the modelled region are presented for E- and B-polarizations. Large anomalous in-phase and quadrature model magnetic fields are observed over the Korea-Japan strait for E-polarization and over the Bohai strait for B-polarization due to current channelling through the straits. Large responses of the peninsulas in the shallow coastal areas occur at short periods but decrease abruptly with increasing period. In general, the effects of peninsulas, straits, bays and irregularities in the coastlines play an important role in the magnetic field responses both on-shore and off-shore for this complex North China-Korea coastal region. Model and field site induction arrows are compared for three sites west of Bohai Bay. 相似文献
17.
E. N. Parker 《地球物理与天体物理流体动力学》2013,107(1-4):1-12
Abstract The propagation of Alfvén waves along a uniform horizontal field in a highly conducting incompressible fluid, subject to the convective forces produced by a uniform vertical temperature gradient, is treated in a Boussinesq approximation. It is shown that there are exact solutions with large amplitude but restricted form. Their restricted form means that an arbitrary disturbing force produces other motions as well as Alfvén waves. An arbitrary initial disturbance of small amplitude produces waves whose state of polarization varies along the direction of propagation. For large amplitudes, however, any mixtures of polarization states causes scattering into new modes. 相似文献