Spatial structure of the magnetic field induced by an infrasonic wave in the oceanic waveguide

The magnetic field generated by an acoustic wave propagating in the oceanic waveguide has been considered. The effect of the self-induction factor on the spatial structure of this field has been studied. It has been indicated that there exists a frequency range where it is necessary to take into consideration self-induction. It has been indicated that the induced field is most substantial at frequencies when only the first normal mode exists. The dependences of the induced field on the depth, frequency, and geomagnetic field direction have been obtained and analyzed for this frequency range.     

磁尾等离子体片中周期性高速流相伴随磁场超低频波

本文利用Cluster卫星2004年11月8日的观测数据,分析了磁尾等离子体片中与地向周期性高速离子流相伴随的ULF波.结果显示周期性高速流的速度波动与磁场和温度中的ULF波同时出现、同时增强、同时消失,而且波动的频率都集中在60~70 mHz.这说明磁场和温度ULF波与周期性高速流密切相关,周期性高速流是ULF波产生的来源.高速流波动的相位与磁场波动的相位大致反相关,与热离子温度波动的相位正相关,同时磁场波动与热离子温度波动呈相位反相关的特性.最小方差法分析的结果显示虽然波传播方向有地向分量,但其主要传播方向是向等离子体片中心传播,并与周期性高速流速度方向垂直.以上观测说明是高速流的周期性变化产生了磁场在Pi1频率范围内的ULF波.     

声波远探测中偏心声源的辐射以及接收波场研究

通过最速下降积分法获得了充液井孔中偏心点声源激发的井外波场的远场渐近解;利用互易性获得井外存在反射体时井内偏心接收的波场渐近解,渐近解结果与有限差分的结果吻合;分析了声源频率、偏心距离以及方位角对波场辐射与接收的影响.计算发现：声源频率是影响井外波场的主导因素,声源频率较低时,偏心点声源激发的远场波场与偏心距离无关,可以将偏心点声源视为中心声源;声源频率较高时,偏心点声源激发的远场波场与中心声源之间存在不可忽略的差异,且频率越高、偏心距离越大,差异越大.计算还发现：采用偏心声源与偏心接收时,辐射波场与接收波场的幅度都具有方位角依赖性.最后我们给出利用反射波幅度变化来消除反射体方位角180°不确定性的算例.     

土中Love波弥散特性

利用有限单元法及解析法建立和求解了土中Love波特征方程以及位移计算公式．计算结果表明,这一计算方法比纯解析法优越,可以用来分析均质和非均质上中Love波弥散性．本文利用这一方法详细讨论了Love波在上软下硬地基及软夹层地基中的传播特性和弥散特性．上软下硬地基Love波具有弥散性,土层的剪切波及厚度对Love波弥散曲线影响较大,而质量密度的相对变化对Love彼弥散曲线影响较小．软夹层地基中低频时Love波以第一模态波为主,现场所测为第一模态波波速;高频时存在多个高模态波,土中传播的波为这几个高模态波的叠加波,现场所测波速随两传感器的位置不同而有波动．     

粘弹性VTI介质地震波模拟特征分析

本文首先利用有限差分法分别对弹性和粘弹性VTI介质进行地震波传播数值模拟,并针对波场快照和波场记录特征,分析不同品质因子组合对波场能量衰减和频率吸收作用的影响.结果表明：对应于膨胀滞弹性形变的品质因子变化主要影响qP波的能量衰减;对应于剪切滞弹性形变的品质因子变化主要影响qSV波的能量衰减;对于qSH波,两个品质因子分别对应于垂直和水平方向的能量衰减;品质因子较小时,qSV波和qSH波的频率向低频方向移动,qP波频率变化不明显.     

通量堆积和偶极化过程中的超低频波动

2004年9月17日TC-1卫星在近地磁尾夜侧观测到一次伴随有通量堆积和偶极化过程的典型亚暴事件.本文利用离散小波分析和FFT分析方法对本次事件中4 s精度的FGM和HIA数据进行分析,以了解通量堆积过程和偶极化过程中的低频波特性.分析结果表明,通量堆积过程和偶极化过程中场和粒子有明显的不规则低频波动,主要波动频率范围为4~15 mHz,和Pi-2脉动一致.通量堆积过程中磁场各个分量的低频波动和偶极化过程中的低频波动有明显不同,表明这两个物理过程可能存在不同的波动机制.在通量堆积过程和偶极化过程中,平行磁场方向上温度和速度的波动和垂直方向上温度和速度的波动有明显区别,平行磁场方向上温度和速度的波动有较好的相关性,且热离子密度的波动和平行磁场方向上的波动有较好的相关性,表明存在快模压缩波.TC-1卫星的观测显示通量堆积过程中磁场By分量有明显增长.我们的分析结果表明ULF波与By分量的增长有密切关系,从而可能对亚暴膨胀相的触发有重要影响.     

Small-scale heterogeneities below the Lanzhou CTBTO seismic array,from seismic wave field fluctuations

Seismic wave field fluctuations below Lanzhou Comprehensive Test Ban Treaty Organization seismic array are determined and interpreted to describe the scattering characteristics of the crust beneath the northeastern margin of Qinghai–Tibet plateau in China. The frequency-dependent intensities of the mean and fluctuation wave fields are analyzed for 21 deep (206–632 km depth) teleseismic events. The observed wave field fluctuations in the frequency range 0.5–2.5 Hz can be explained by the scattering of the teleseismic P wave front at random media-type structures. The stable and narrow range of the fluctuation parameters from these teleseismic events indicates evidence for scattered seismic phases which are generated inside the crust. The reasonable structural models contain heterogeneities with 1–3% velocity fluctuations and 2.4–8.2 km correlation lengths in the crust with 53 km thickness.     

从空间飞行器注入电离层的调制电子束产生的电磁波辐射

调制电子束入射进电离层等离子体中会激发电磁波辐射,根据不同试验条件和等离子体状态,激发电磁波的机制也不一样.本文主要讨论半无界稀薄调制电子束沿地球磁场力线从空间飞行器入射到电离层等离子体产生的电磁波辐射,其相应的辐射机理是由于束的纵向约束而产生的电磁波辐射.理论分析和数值计算结果显示,在满足切伦柯夫（Cerenkov）共振条件时,哨声波前向辐射方向图有一个尖锐的峰值,且随着电子束弛豫长度的增加,辐射功率值也相应增大,表明可以通过对电子束的适当调制增强电子束激发的电磁波辐射强度.     

Infrasonic wave magnetic field in the oceanic waveguide

The magnetic field generated by an acoustic wave, propagating in the oceanic wave guide, has been considered. It has been indicated that the induced field is most substantial at frequencies when only the first normal mode exists. The dependences of the induced field component on the depth, frequency, and direction of the geomagnetic field have been obtained in this frequency band. The possibility of determining coordinates of a strong underwater earthquake using the acoustic field magnetic field has been considered.     

非对称圆弧片状声源在井旁地层中产生的声场

提出了一种可用于随钻三维反射声波成像测井的圆弧片状声源,推导了该声源声学性质在波数-频率域内的数学描述,并利用实轴积分的方法对该声源在井旁地层中产生的声场进行求解,考察了声源的线度、频率等因素对该声源向地层中辐射的声场的影响.研究结果表明,特定尺寸和特定频率下的圆弧片状声源产生的纵波场的水平和垂直指向性图中仅具有一个明显的主瓣,且主瓣三分贝角宽较窄,方位分辨率较高,指向性良好,适用于随钻三维反射成像测井;SV波场和SH波场的指向性图中存在两个或者多个角瓣,SV波场在垂直于井轴方向上辐射的能量为0,另外在井中发射和接收的反射SH波场和SV波场会相互干扰,所以难以利用SV波场和SH波场进行三维反射声波成像;声源的线度和频率等因素对其辐射声场影响较大,考虑到激励效率和方位分辨率等因素,对于本文描述的井孔模型,选择圆周角在75°和90°之间, 主频为12 kHz左右的声源是合适的.     

多道瞬态瑞雷波技术在公路采空塌陷区探测中应用

地下采空塌陷区岩体结构具有明显的结构不连续、松散、断裂、空洞等异常结构特征,本文在分析公路采空塌陷区地球物理场特征的基础上,详细讨论了应用多道瞬态瑞雷波技术探测采空塌陷区的可行性以及相关技术,深入分析基于瑞雷波波场特征、频谱结构、能量衰减、频散特征、相速度以及多阶模等特征探测和评价地层结构的均匀性、地下空洞及异常结构体等地下障碍物的存在及其空间分布的解释标志.滚动式多道瑞雷波探测技术可以有效地探测地下采空区、软弱结构体等异常结构体的赋存状态及空间分布.     

软地层横波速度的偶极随钻测井反演

在电缆测井中,可以利用偶极声场中的弯曲波反演软地层的横波速度.然而,在随钻声波测井(LWD)中,钢制钻铤的存在使得井孔结构变得复杂,同时改变了井孔声场,弯曲波也变得难以测定.此外,弯曲波与钻铤波耦合在一起,使得地层横波速度的反演变得困难.本文计算分析了随钻声场的频散曲线和激发曲线,注意到了偶极舒尔特波在较宽频带内速度频散很弱,特别是在本文研究的软地层情况下,偶极舒尔特波速度在3至25kHz的频率范围内几乎为一个常值,并且该值与地层横波速度存在一一对应关系.舒尔特波速度远小于其他模式波速度,与其他模式波在时域上易分离.相对于其他地层参数,舒尔特波对地层横波速度十分敏感.因此,它可以用来反演软地层的横波速度.     

孔隙地层轻质水泥套管井中偶极弯曲波的激发与传播特性

针对软地层套管井中弯曲波频散移向高频,以致超出了现行偶极声波测井仪器的激发频带的问题,本文在井外为孔隙地层时,采用Biot模型对套管井多极源激发的声波场进行了理论推导,对套管井偶极弯曲波的频散特性进行了数值模拟,考察了高密度水泥(或快速水泥)和低密度水泥(或轻质水泥)情况下的弯曲波频散,分析了不同水泥环对弯曲波主频散区和激发谱偏移的影响,重点对轻质水泥套管井中偶极源激发的模式波频散与激发谱及临界折射P、S波激发特性进行了研究,并考察了渗透率、孔隙度对弯曲波频散及衰减的影响,利用实轴积分法计算了偶极声源激发的时域全波波形.分析对比结果表明,在快速水泥情况下弯曲波频散曲线随着地层特征横波速度的减小会迅速向高频移动,随着快速水泥向轻质水泥变化,弯曲波频散曲线向高频移动将会减缓,对于特征横波速度低于1400m·s~(-1)的软地层,偶极弯曲波基础模式主频散区(或截止频率)可以由原来13kHz向低频移动至4kHz;在轻质水泥套管井中,无论是硬地层还是软地层,在目前偶极声波测井仪器声源主频激发下,接收波形中弯曲波均占主导地位.     

WIND observations of coherent electrostatic waves in the solar wind

The time domain sampler (TDS) experiment on WIND measures electric and magnetic wave forms with a sampling rate which reaches 120 000 points per second. We analyse here observations made in the solar wind near the Lagrange point L1. In the range of frequencies above the proton plasma frequency f_pi and smaller than or of the order of the electron plasma frequency f_pe, TDS observed three kinds of electrostatic (e.s.) waves: coherent wave packets of Langmuir waves with frequencies f ≃ f_pe, coherent wave packets with frequencies in the ion acoustic range f_pi ≥ f ≥ f_pe, and more or less isolated non-sinusoidal spikes lasting less than 1 ms. We confirm that the observed frequency of the low frequency (LF) ion acoustic wave packets is dominated by the Doppler effect: the wavelengths are short, 10 to 50 electron Debye lengths λ_D. The electric field in the isolated electrostatic structures (IES) and in the LF wave packets is more or less aligned with the solar wind magnetic field. Across the IES, which have a spatial width of the order of ≃25_D, there is a small but finite electric potential drop, implying an average electric field generally directed away from the Sun. The IES wave forms, which have not been previously reported in the solar wind, are similar, although with a smaller amplitude, to the weak double layers observed in the auroral regions, and to the electrostatic solitary waves observed in other regions in the magnetosphere. We have also studied the solar wind conditions which favour the occurrence of the three kinds of waves: all these e.s. waves are observed more or less continuously in the whole solar wind (except in the densest regions where a parasite prevents the TDS observations). The type (wave packet or IES) of the observed LF waves is mainly determined by the proton temperature and by the direction of the magnetic field, which themselves depend on the latitude of WIND with respect to the heliospheric current sheet.     

一种多波宽频地震数据采集设计与仪器实现关键技术

随着多波多分量技术的发展,宽频数据采集逐渐成为地震勘探的发展趋势.通过高保真获取全波场信息,并尽可能保留高频有效成分,进而利用多种波场信息相互验证和补充,是提高地震勘探精度的有效方法.受仪器带宽限制,常规设备在高频段很难同时保持高分辨率和大动态范围特征,在多波地震采集时,极容易出现分辨率不足和限幅失真等现象,极大影响多波多分量方法的实际应用效果.鉴于此,本文给出一种利用积分器、高频ADC、DAC和抽取滤波器构成的低成本宽频数据采集方法.通过构造环路滤波器(调制器),对高频ADC输出数据中的量化噪声二次整形,并配合抽取滤波,对带外噪声进行有效压制.实际测试表明,通过精细电路结构设计,采集站有效分辨率可达24位(采样率为2 kHz),动态范围超过140 dB,SNR达142 dB.相比传统设备,其采集数据在5～25 Hz的低频段和100 Hz以上的高频段都具有更加丰富的有效信息,非常适合多波多分量数据采集.     

随钻声波测井FDTD模拟及钻铤波传播特性研究

幅度大的钻铤波掩盖地层信号是困扰随钻声波测井技术的难题,认识钻铤波特性对于消除或有效降低钻铤波至关重要.记录岩石动电效应引起电磁场的随钻动电测井,被认为有望彻底解决钻铤波干扰问题.本文采用有限差分法,模拟不同钻铤、不同井孔结构的随钻声场,对比分析了单极源钻铤波的传播特性,阐明存在伴随钻铤波动电信号的原因.结果表明:钻铤声波在沿钻铤传播时向外部介质辐射能量,透过井壁进入地层的具有视钻铤波速度的声波,与地层纵横波一样可发生动电转化,因而可导致随钻动电测井时产生钻铤波速度的电磁信号.计算还表明,高频情况下,随钻声波测井钻铤波呈现两阶模式:具有低频截止频率的高阶钻铤波幅度较小,其速度略低于钻铤纵波速度;无截止频率的低阶钻铤波幅度较大,其波速在高频时甚至低于钻铤横波速度.这种频散特性和多阶模式特性,是径向多分层开波导结构的导波属性.     

Implementation of viscoelastic mud-induced energy attenuation in the third-generation wave model,SWAN

The interaction of waves with fluid mud can dissipate the wave energy significantly over few wavelengths. In this study, the third-generation wave model, SWAN, was advanced to include attenuation of wave energy due to interaction with a viscoelastic fluid mud layer. The performances of implemented viscoelastic models were verified against an analytical solution and viscous formulations for simple one-dimensional propagation cases. Stationary and non-stationary test cases in the Surinam coast and the Atchafalaya Shelf showed that the inclusion of the mud-wave interaction term in the third-generation wave model enhances the model performance in real applications. A high value of mud viscosity (of the order of 0.1 m²/s) was required in both field cases to remedy model overestimation at high frequency ranges of the wave spectrum. The use of frequency-dependent mud viscosity value improved the performance of model, especially in the frequency range of 0.2–0.35 Hz in the wave spectrum. In addition, the mud-wave interaction might affect the high frequency part of the spectrum, and this part of the wave spectrum is also affected by energy transfer from wind to waves, even for the fetch lengths of the order of 10 km. It is shown that exclusion of the wind input term in such cases might result in different values for parameters of mud layer when inverse modeling procedure was employed. Unlike viscous models for wave-mud interaction, the inverse modeling results to a set of mud parameters with the same performance when the viscoelastic model is used. It provides an opportunity to select realistic mud parameters which are in more agreement with in situ measurements.     

Radio emission spectrum from an interplanetary shock front

The characteristics of low-damping high-frequency waves in hot magnetized solar and stellar coronal plasmas under the conditions when the electron gyrofrequency ω_He is equal to or higher than the electron plasma frequency ω_pe have been analyzed using the numerical solution of the dispersion equation. It is shown that the wave branches corresponding to the Z mode and ordinary waves approach each other when the magnetic field increases and become almost indistinguishable in a wide frequency range at all angles between the wave vector and magnetic field. A branch with anomalous dispersion appears at angles close to 90°. A new interpretation of broadband pulsations and spikes is suggested on the basis of the results.     

High-frequency waves in hot magnetized solar and stellar coronal plasmas

The characteristics of low-damping high-frequency waves in hot magnetized solar and stellar coronal plasmas under the conditions when the electron gyrofrequency ω_He is equal to or higher than the electron plasma frequency ω_pe have been analyzed using the numerical solution of the dispersion equation. It is shown that the wave branches corresponding to the Z mode and ordinary waves approach each other when the magnetic field increases and become almost indistinguishable in a wide frequency range at all angles between the wave vector and magnetic field. A branch with anomalous dispersion appears at angles close to 90°. A new interpretation of broadband pulsations and spikes is suggested on the basis of the results.     

微动探测方法软件的实现

利用微动进行勘探无需振动源,方便快捷、对环境没有干扰,是一种很有发展前景的勘探方法。针对微动探测数据处理的需求,开发研制了一套可视化微动探测处理分析软件系统MSMSPAC。该软件采用C~#语言开发,主要功能包括台阵设计、台阵方位角分布分析、数据格式转换、微动有效数据段挑选、数据滤波、重采样、参数计算及频散曲线提取、编辑、合并、项目管理等功能。软件系统界面友好,操作简便。