Understanding the Adjoint Method in Seismology: Theory and Implementation in the Time Domain

Rafael Abreu
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Abstract

The adjoint method is a popular method used for seismic (full-waveform) inversion today. The method is considered to give more realistic and detailed images of the interior of the Earth by the use of more realistic physics. It relies on the definition of an adjoint wavefield (hence its name) that is the time reversed synthetics that satisfy the original equations of motion. The physical justification of the nature of the adjoint wavefield is, however, commonly done by brute force with ad hoc assumptions and/or relying on the existence of Green's functions, the representation theorem and/or the Born approximation. Using variational principles only, and without these mentioned assumptions and/or additional mathematical tools, we show that the time reversed adjoint wavefield should be defined as a premise that leads to the correct adjoint equations. This allows us to clarify mathematical inconsistencies found in previous seminal works when dealing with visco-elastic attenuation and/or odd-order derivative terms in the equation of motion. We then discuss some methodologies for the numerical implementation of the method in the time domain and to present a variational formulation for the construction of different misfit functions. We here define a new misfit travel-time function that allows us to find consensus for the long-standing debate on the zero sensitivity along the ray path that cross-correlation travel-time measurements show. In fact, we prove that the zero sensitivity along the ray-path appears as a consequence of the assumption on the similarity between data and synthetics required to perform cross-correlation travel-time measurements. When no assumption between data and synthetics is preconceived, travel-time Frechet kernels show an extremum along the ray path as one intuitively would expect.
了解地震学中的邻接法:时域理论与实施
邻接法是当今用于地震(全波形)反演的一种流行方法。人们认为,该方法通过使用更逼真的物理学原理,可提供更真实、更详细的地球内部图像。它依赖于邻接波场的定义(因此而得名),即满足原始运动方程的时间反转合成波场。然而,对邻接波场性质的物理论证通常是通过临时假设和/或依靠格林函数的存在、表示定理和/或博尔纳近似法来完成的。我们仅使用变分原理,而不使用上述假设和/或额外的数学工具,就证明了时间反转的邻接波场应被定义为导致正确邻接方程的前提。这使我们能够澄清以前的开创性著作在处理运动方程中的粘弹性衰减和/或奇数阶导数项时发现的数学不一致之处。我们讨论了在时域中数值实现该方法的一些方法,并提出了构建不同误拟合函数的变分公式。在此,我们定义了一种新的误差旅行时间函数,它使我们能够就长期以来关于交叉相关旅行时间测量所显示的沿射线路径的零灵敏度的争论达成共识。事实上,我们证明了射线路径上的零灵敏度是进行交叉相关旅行时间测量所需的数据与合成物之间相似性假设的结果。如果不预先假定数据和合成物之间的相似性,那么旅行时间弗雷谢特核就会像人们直觉上所期望的那样,在射线路径上出现一个极值。
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