Seismic random noise attenuation and signal-preserving by multiple directional time-frequency peak filtering     

《Comptes Rendus Geoscience》2015,347(1):2-12

Time-frequency peak filtering (TFPF) is an effective method for seismic random noise attenuation. The linearity of the signal has a significant influence on the accuracy of the TFPF method. The higher the linearity of the signal to be filtered is, the better the denoising result is. With this in mind, and taking the lateral coherence of reflected events into account, we do TFPF along the reflected events to improve the degree of linearity and enhance the continuity of these events. The key factor to realize this idea is to find the traces of the reflected events. However, the traces of the events are too hard to obtain in the complicated field seismic data. In this paper, we propose a Multiple Directional TFPF (MD–TFPF), in which the filtering is performed in certain direction components of the seismic data. These components are obtained by a directional filter bank. In each direction component, we do TFPF along these decomposed reflected events (the local direction of the events) instead of the channel direction. The final result is achieved by adding up the filtering results of all decomposition directions of seismic data. In this way, filtering along the reflected events is implemented without accurately finding the directions. The effectiveness of the proposed method is tested on synthetic and field seismic data. The experimental results demonstrate that MD–TFPF can more effectively eliminate random noise and enhance the continuity of the reflected events with better preservation than the conventional TFPF, curvelet denoising method and F–X deconvolution method.  相似文献   

小波框架的彩色图像泊松去噪     

高涛  何秀丽 《南京气象学院学报》2020,12(5):614-618

噪声是影响图像质量的重要因素,噪声的存在导致图像的某些特征细节不能被辨识以及图像的信噪比下降,所以图像去噪是图像处理中的一个重要问题.本文提出了基于小波框架的彩色图像的泊松去噪模型.在该模型中,赋权的l²项作为保真项,包含小波框架的l¹项作为正则项.同时,又提出了解决该模型的重新赋权的split Bregman算法.最后,利用仿真实验以及PSNR（峰值信噪比）指标对该模型的去噪效果进行评估,评估结果表明该算法可行、有效.  相似文献   

确定风廓线雷达功率谱噪声功率方法   总被引：5，自引：3，他引：2       下载免费PDF全文

何平  李柏  吴蕾  高玉春 《应用气象学报》2013,24(3):297-303

风廓线雷达以测风为主要目的设计,没有充分考虑强度的定量测量。如果能够实现强度定量测量将大大扩展风廓线雷达的应用范围。首要的扩展应用就是可以获取雨滴谱分布、解决降水定量测量准确性问题。若实现强度定量测量,需要解决的一个关键技术问题是如何由其功率谱数据准确计算噪声功率。该文根据风廓线雷达功率谱估计方法、依据噪声频域统计特性,提出了一种计算风廓线雷达功率谱噪声功率的方法,并利用风廓线雷达实测功率谱数据进行检验。检验结果表明:即便在有降水或存在地物时,该方法仍可以准确、快速分辨出噪声功率谱, 且客观有效。  相似文献   

Model of wind-generated ambient noise in stratified shallow water   总被引：1，自引：0，他引：1  

林建恒  高天赋 《中国海洋湖沼学报》2005,23(2):144-151

In order to build a rapid ocean ambient noise model adapted for a stratified shallow water, a hybrid model of normal mode method (for far field) and ray method (for near field) is suggested which combines the advantages of both methods. Since the near field of wind-generated noise is not sensitive to the sound speed profile, the sound speed profile is regarded as a constant; which makes the model rapid and accurate. The simulation results are in agreement with those of the wave model.  相似文献   

高稳定性数字钟的分析与实现     

HUANG Peicheng 《中国科学院上海天文台年刊》2004,(1)

介绍一种高稳定、低功耗、多功能、小型化的数字钟 ,由数字钟插入相位噪声引起的 1pps输出信号相位抖动为 5 .3ps,前沿上升时间为 4 .6ns ,指标测量通过 2m长 5 0Ω高频同轴电缆并接 5 0Ω电阻性负载 ,输入信号为 10MHz正弦波信号 ,移相精度为 10 0ns,同步精度≤ 10 0ns,通过RS 2 32接口每秒一次的速率以ASCII码格式输出时间信息 (年、月、日、时、分、秒 ) ,在接数显钟面时其功耗为2W ,不接数显钟面时为 1.2W。  相似文献   

On the analysis of light curves in asteroseismology     

David L. Mary 《Journal of Astrophysics and Astronomy》2005,26(2-3):283-292

We provide a detailed introduction to the main problems arising when analyzing light curves in asteroseismology. Attention is first paid to the signal model delivered by the pulsating stars and to the noise sources corrupting this model in photometric observations. The main pitfalls and ambiguities occurring in Fourier analysis are summarized and illustrated. Some classical, Least Squares (LS) based methods for spectrum analysis are analyzed and commented on from the point of view of ill-posed problems. The insight that can be gained from such analyses is discussed.  相似文献   

Is there a black hole among the black-hole candidates?     

Wolfgang Kundt  Daniel Fischer 《Journal of Astrophysics and Astronomy》1989,10(1):119-138

None of the tentative black-hole identifications has remained without serious difficulties. As a class, the black-hole candidates differ in no obvious property from neutron-star binaries other than in their estimated high mass. We favour an interpretation of the black-hole candidates as binary neutron stars surrounded by a more or less massive accretion disc  相似文献   

分形随机漫步噪声及相关函数     

韩英  符养 《地球科学与环境学报》2003,25(3):81-83

讨论了在地学、工程测量研究领域常见的随机漫步噪声,从理论上将经典布朗运动随机过程(随机漫步噪声)推广到分形布朗运动随机过程,并导出分形布朗运动随机过程的相关函数。  相似文献   

Assessing the Vibrational Frequencies of the Holweide Hospital in the City of Cologne (Germany) by Means of Ambient Seismic Noise Analysis and FE modelling     

Stefano?ParolaiEmail author  Andreas?F?cke  Sandra?M.?Richwalski  Lothar?Stempniwski 《Natural Hazards》2005,34(2):217-230

Ambient seismic noise measurements were conducted inside the Holweide Hospital (Cologne) for checking whether its frequencies of vibration fall into the range where soil amplification is expected. If this is the case, damage might increase in case of an earthquake due to an amplified structural response of the building. Two different techniques were used: the ratio between the horizontal and vertical components of the spectra recorded at stations located inside the building and the ratio between the corresponding components of the spectra recorded simultaneously inside the building and at a reference station placed outside. While the former method might be preferred because of less equipment involved, the latter has the advantage of producing more stable results and deleting automatically the influence of the sedimentary cover, which might obscure some eigenfrequencies of vibration of the building. An independently performed finite-element analysis of the hospital showed a good correlation between measured and calculated eigenmodes.  相似文献   

A simplified method for simulation of strong ground motion using finite rupture model of the earthquake source     

A.?JoshiEmail author  S.?Midorikawa 《Journal of Seismology》2004,8(4):467-484

We present a simplified method to simulate strong ground motion for a realistic representation of a finite earthquake source burried in a layered earth. This method is based on the stochastic simulation method of Boore (Boore, D. M., 1983, Bull. Seism. Soc. Am. 73, 1865–1894) and the Empirical Greens Function (EFG) method of Irikura (Irikura, K., 1986, Proceedings of the 7th Japan Earthquake symposium, pp. 151–156). The rupture responsible for an earthquake is represented by several subfaults. The geometry of subfaults and their number is decided by the similarity relationships. For simulation of ground motion using the stochastic simulation technique we used the shapping window based on the kinetic source model of the rupture plane. The shaping window deepens on the geometry of the earthquake source and the propagation characteristics of the energy released by various subfaults. The division of large fault into small subfaults and the method for accounting their contribution at the surface is identical to the EGF. The shapping window has been modified to take into account the effect of the transmission of energy released form the finite fault at various boundaries of the layered earth model above the source. In the present method we have applied the correction factor to adjust slip time function of small and large earthquakes. The correction factor is used to simulate strong motion records having basic spectral shape of ² source model in broad frequency range. To test this method we have used the strong motion data of the Geiyo earthquake of 24th March 2001, Japan recorded by KiK network. The source of this earthquake is modelled by a simple rectangular rupture of size 24 × 15 km, burried at a depth of 31 km in a multilayered earth model. This rupture plane is divided into 16 rectangular subfaults of size 6.0 × 3.75 km each. Strong motion records at eight selected near-field stations were simulated and compared with the observed records in terms of the acceleration and velocity records and their response spectrum. The comparison confirms the suitability of proposed rupture model responsible for this earthquake and the efficacy of the approach in predicting the strong motion scenario of earthquakes in the subduction zone. Using the same rupture model of the Geiyo earthquake, we compared the simulated records from our and the EGF techniques at one near-field station. The comparison shows that this technique gives records which matches in a wide frequency range and that too from simple and easily accessible parameters of burried rupture.  相似文献