Abstract
We outline a method that enables the efficient computation of exact Fréchet sensitivity kernels for a non-gravitating 3-D spherical earth model. The crux of the method is a 2-D weak formulation for determining the 3-D elastodynamic response of the earth model to both a moment-tensor and a point-force source. The sources are decomposed into their monopole, dipole and quadrupole constituents, with known azimuthal radiation patterns. The full 3-D response and, therefore, the 3-D waveform sensitivity kernel for an arbitrary source-receiver geometry, can be reconstructed from a series of six independent 2-D solutions, which may be obtained using a spectral-element or other mesh-based numerical method on a 2-D, planar, semicircular domain. This divide-and-conquer, 3-D to 2-D reduction strategy can be used to compute sensitivity kernels for any seismic phase, including grazing and diffracted waves, at relatively low computational cost. © 2007 The Authors Journal compilation © 2007 RAS.
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CITATION STYLE
Nissen-Meyer, T., Dahlen, F. A., & Fournier, A. (2007). Spherical-earth Fréchet sensitivity kernels. Geophysical Journal International, 168(3), 1051–1066. https://doi.org/10.1111/j.1365-246X.2006.03123.x
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