Seismic modeling plays an important role in geophysics and seismology for estimating the response of seismic sources in a given medium. In this work, we present a MATLAB-based package, FDwave3D, for synthetic wavefield and seismogram modeling in 3D anisotropic media. The seismic simulation is carried out using the finite-difference method over the staggered grid, and it is applicable to both active and passive surveys. The code package allows the incorporation of arbitrary source mechanisms and offers spatial derivative operators of accuracy up to tenth-order along with different types of boundary conditions. First, the methodological aspects of finite-difference method are briefly introduced. Then, the code has been tested and verified against the analytical solutions obtained for the homogeneous model. Further, the numerical examples of layered and overthrust models are presented to demonstrate its reliability.
提高地震数据分辨率是地震勘探中获得高质量数据的关键,而分辨率与信噪比的相互制约关系是高分辨率处理的根本问题。本文基于反褶积的基本原理,采用压缩子波的方法,对原始地震数据进行高频拓展法(High Frequency Expanding,HFE)处理。通过测试子波压缩参数,分析研究可选参数对地震资料分辨率和保真度的影响,确定最佳处理参数,并应用于实际地震资料处理中。应用结果表明,HFE处理后的地震资料,其品质得到了明显的改善,处理后的剖面弱反射带层间细节反射更为丰富,横向变化清晰,频带变宽,分辨率得到了很大提高。 相似文献
Two large stable solar filaments were used as test tracers to determine the apparent synodic rotation rate as a function of the central meridian distance for several filaments' segments at different heights. An analytic fitting procedure was applied to determine simultaneously the real synodic rotation rate and the height of the traced filament segments. The determined heights were compared with the values obtained from the widths of filament contours on the solar disk and with the values obtained by direct measurements at the solar limb. Furthermore, the obtained rotation rates and heights of the filaments' segments close to the filaments' pivot points were compared with the values obtained using two successive central meridian passages. Finally, sources and scales of errors were investigated and possible implications on the previous studies of the solar differential rotation were considered. 相似文献