青海地区流体地球化学背景特征     

刘磊  张朋涛  李霞  赵玉红  冯丽丽  苏维刚 《地震地磁观测与研究》2021,42(2):186-187

  相似文献   

台阵地震计程控化正弦标定系统设计     

郭磊  白珊珊  李从庆  轩倩倩 《地震地磁观测与研究》2021,42(4):163-168

为满足台阵地震计标定要求,通过对程控化标定测控仪和标定测控软件的研究,采用一种适用于台阵地震计的程控化正弦标定方法,对中国地震局地球物理勘探中心负责管理的台阵地震计进行标定。台阵地震计标定实验结果显示,采用程控化正弦标定方法,在缩短标定时长、提高标定效率方面具有显著效果。  相似文献   

连云港地震台BBVS-120、CTS-1E型地震计系统性能对比     

立凯  秦磊  曾智  孙雷 《地震地磁观测与研究》2021,43(1):106-110

通过对连云港地震台BBVS-120、CTS-1E型地震计台基噪声功率谱分析,正弦标定和脉冲标定计算分析,近震和远震震级对比分析,研究在实际工作中2种地震计性能差异,对比观测数据质量,检验稳定性,以期为地震监测及相关研究工作提供依据。  相似文献   

基于地震属性融合技术的火山通道识别研究     

曹磊  蔡峰 《地球物理学进展》2021,36(2):559-564

长岭龙凤山火山岩为多机构、多期次喷发叠合分布的一套火山岩地层,火山通道识别是成藏分析和油气运移等研究工作的基础,同时也影响储量计算和开发井的部署.针对深层地震资料品质较差,且难以对火山通道进行准确刻画的问题,开展针对火山通道的地震属性优选.该地区火山岩具有"低频强振幅"的特点,通过地震属性优选,提取10 Hz单频体、纹理对比属性和最大振幅地震属性,平面上采用三者RGB融合方法识别并落实火山通道边界,剖面上采用10 Hz单频体、纹理对比属性和地震数据体三者HSV融合突出火山通道纵向展布.通过地震属性融合在碎屑岩里识别强振幅,在火山岩里识别低频能量,在一定程度上抑制其他岩相的影响,最终实现长岭龙凤山地区火山通道的准确刻画.  相似文献   

腮腺良性肿瘤容积穿梭CT灌注时间-密度曲线特征分析          下载免费PDF全文

杨振兴  郝粉娥  赵磊  杨晓光  刘挨师 《CT理论与应用研究》2021,30(5):575-582

目的:探讨容积穿梭CT灌注时间-密度曲线特征结合形态学参数对腮腺良性肿瘤鉴别诊断的价值。方法:收集我院拟诊腮腺肿瘤患者100例,术前均行容积穿梭CT灌注成像检查,术后经手术病理证实。将所得影像数据传送至工作站及pacs系统,观察分析不同病理类型腮腺肿瘤的形态学参数（位置、大小、密度、边界、颈部淋巴结、增强扫描强化幅值）及时间-密度曲线（TDC）类型,计数资料比较采用χ2检验,计量资料符合正态分布采用两独立样本t检验,不符合正态分布的采用秩和检验,检验水准α=0.05。结果:腮腺良性肿瘤（多行性腺瘤、腺淋巴瘤、基底细胞瘤及肌上皮瘤）间的形态学参数无统计学差异;时间-密度曲线类型差异有统计学差异。结论:CT灌注时间-密度曲线特征结合形态学参数对腮腺良性肿瘤的鉴别诊断有重要价值,为患者术式的选择有重要指导意义。   相似文献   

基于机器学习的地震动特征提取与模拟以2021年云南漾濞6.4级地震为例          下载免费PDF全文

靳超越  胡进军  胡磊  王中伟 《世界地震工程》2021,(4):073-80

随着地震动数据数量的增长和质量的提高,将基于数据驱动的机器学习方法应用到地震动模拟中有重要意义。以2021年5月21日云南漾濞M_S6.4地震为例,利用主成分析方法从前震及余震地震动记录中提取特征母波时程,将地震动三要素作为模拟误差约束,在求解母波的线性组合系数时使用多目标优化算法寻优,最终找到帕累托最优解作为模拟目标台站记录时的组合系数,得到模拟地震动时程。结果表明:主成分析法在对实际地震动记录进行特征提取后,得到的特征母波时程可以在一定程度上保留原始数据的主要信息;考虑幅值、频谱和持时这三要素的角度去控制模拟误差,可以使得模拟的地震动时程更加接近真实记录。提出的基于特征提取的地震动模拟方法可以为基于小震数据合成大震地震动提供参考。  相似文献   

Statistics of long-crested extreme waves in single and mixed sea states     

Wang  Lei  Li  Jinxuan  Liu  Shuxue  Ducrozet  Guillaume 《Ocean Dynamics》2021,71(1):21-42

Ocean Dynamics - Most of the studies on extreme waves are focused on the systems with single-peak wave spectra. However, according to the statistics of occurrence, the bimodal spectral system is...  相似文献   

The Responses of the Deformable Earth to Different Driving Forces     

Han-wei Zhang  Qiong-xian Tie  Lei Yang 《Chinese Astronomy and Astrophysics》2008,32(2):209-215

The spatial and temporal variations of the Earth deformation and the gravitational field are important both in the theoretical research and in the construction of geospatial database. The Earth deforms due to various mechanisms and the deformation further induces changes in the gravitational potential of the Earth, i.e. the deformation-induced additional potential or the Euler gravitational increment. Based on the theory of vector spherical harmonics, we discuss in this paper the Earth deformation and gravitational increment resulting from the tidal force, loading force and the stress of the Earth's surface. We write out the expression for the Euler gravitational potential increment and the relations between different Love numbers. These are all important points in the research on Earth deformation.  相似文献   

Calculation of the Intensity Ratio and Intrinsic Redshift Ratio of the Cerenkov Iron K_α and K_β Lines and Its Possible Application in the Study of AGNs     

Dang-bo Liu  Lei Chen  Jun-han You 《Chinese Astronomy and Astrophysics》2008

We have pointed out that, when thermal relativistic electrons with an isotropic velocity distribution move through a region of dense gas or impinge upon its surface, the Cerenkov effect will produce a particular kind of atomic or ionic emission line, which we have called the “Cerenkov line-like radiation”. This prediction for the optical wavebands has been verified by laboratory experiments. In this paper, we extend this line-like radiation theory to the X-ray waveband and give the basic formulae for calculating the intensity ratio and intrinsic redshift ratio of the Cerenkov iron K_α and K_β lines, for different ionization orders of iron. Potential application of this calculated result may be found in the study of AGNs. The recent observations of NGC3783 show that besides the iron K_α line at ∼6.4 keV, there is also a very strong iron Kβ line at ∼7.0 keV, and that the ratio of equivalent widths between the two is anomalous: EWK_α/EWK_β ≈ 3.43. It is difficult to explain this by the conventional mechanism of “photoelectric absorption-fluorescence emission”. We suggest that the mechanism of Cerenkov line-like radiation can provides a way of solving this puzzle. Besides, we expect that the calculated intrinsic redshift ratio of Cerenkov iron K_α and K_β lines could be tested in future observations. If our suggestion is further supported by observations, then our view on the physical environment around the central massive black hole of an AGN will be greatly modified: the activity becomes more energetic and violent, and the gas, much denser than previously thought.  相似文献   

The Effect of AGN and SNe Feedback on Star Formation, Reionization and the Near Infrared Background     

Lei Wangt Ji-Rong Mao Shou-Ping Xiang Ye-Fei Yuan 《中国天文和天体物理学报》2008,8(6)

Feedback from supernovae (SNe) and from active galactic nuclei (AGN) accom-panies the history of star formation and galaxy evolution. We present an analytic model to explain how and when the SNe and AGN exert their feedback effects on the star formation and galaxy evolution processes. By using SNe and AGN kinetic feedback mechanisms based on the Lambda Cold Dark Matter (LCDM) model, we explore how these feedback mecha-nisms affect the star formation history (SFH), the Near-Infrared Background (NIRB) flux and the cosmological reionization. We find the values of the feedback strengths, ∈AGN =1.0+0.50.3and ∈SN=0.04+0.02-0.02, can provide a reasonable explanation of most of the observational re-suits, and that the AGN feedback effect on star formation history is quite different from the SNe feedback at high redshifts. Our conclusions manifest quantitatively that these feedback effects decrease star formation rate density (SFRD) and the NIRB flux (in 1.4 - 4.0μm), and postpone the time of completion of the cosmological reionization.  相似文献