【24h】

Deconvolution of the PSF of a Seismic Lens

机译:地震透镜的PSF的反卷积

获取原文
获取原文并翻译 | 示例

摘要

We show that if seismic data d is related to the migration image by m_(mig) = L~Td, then m_(mig) is a blurred version of the actual reflectivity distribution m, i.e., m_(mig) = [L~TL]m. Here L is the acoustic forward modeling operator under the Born approximation where d = Lm. The blurring operator [L~TL], or point spread function, distorts the image because of defects in the seismic lens, i.e., small source-receiver recording aperture and irregular/coarse geophone-source spacing. These distortions can be partly suppressed by applying the deblurring operator [L~TL] to the migration image to get m = [L~TL] m_(mig). This deblurred image is known as a least squares migration (LSM) image if [L~TL]~(-1) L~T is applied to the data d using a conjugate gradient method, and is known as a migration deconvolved (MD) image if [L~TL] is directly applied to the migration image m_(mig) in (k_x, k_y, z) space. The MD algorithm is an order-of-magnitude faster than LSM, but it employs more restrictive assumptions. We also show that deblurring can be used to filter out coherent noise in the data such as multiple reflections. The procedure is to, e.g., decompose the forward modeling operator into both primary and multiple reflection operators d = (L_(prim) + L_(mult))m, invert for m, and find the primary reflection data by d_(prim) = L_(prim)m. This method is named least squares migration filtering (LSMF). The above three algorithms (LSM, MD and LSMF) might be useful for attacking problems in optical imaging.
机译:我们表明,如果地震数据d通过m_(mig)= L〜Td与迁移图像相关,则m_(mig)是实际反射率分布m的模糊版本,即m_(mig)= [L〜TL ] m。这里L是在Born近似下的声学前向建模算子,其中d = Lm。模糊运算符[L〜TL]或点扩展函数由于地震透镜中的缺陷(即,较小的源接收器记录孔径和不规则/粗大的检波器-源间隔)而使图像失真。通过对迁移图像应用去模糊算子[L〜TL]以获得m = [L〜TL] m_(mig),可以部分抑制这些失真。如果使用共轭梯度方法将[L〜TL]〜(-1)L〜T应用于数据d,则该去模糊图像称为最小二乘偏移(LSM)图像,并且称为偏移反卷积(MD)如果[L〜TL]直接应用于(k_x,k_y,z)空间中的迁移图像m_(mig),则为该图像。 MD算法比LSM快一个数量级,但是采用了更多限制性假设。我们还表明,去模糊可用于滤除数据中的相干噪声,例如多次反射。该过程是,例如,将前向建模算子分解为主反射算子和多重反射算子d =(L_(prim)+ L_(mult))m,求m倒数,然后通过d_(prim)=找到主反射数据。 L_(prim)m。此方法称为最小二乘迁移过滤(LSMF)。以上三种算法(LSM,MD和LSMF)可能有助于解决光学成像中的问题。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号