F-mode sensitivity kernels for flows
Astrophysics
2007-05-23 v1
Abstract
We compute f-mode sensitivity kernels for flows. Using a two-dimensional model, the scattered wavefield is calculated in the first Born approximation. We test the correctness of the kernels by comparing an exact solution (constant flow), a solution linearized in the flow, and the total integral of the kernel. In practice, the linear approximation is acceptable for flows as large as about 400 m/s.
Keywords
Cite
@article{arxiv.astro-ph/0612475,
title = {F-mode sensitivity kernels for flows},
author = {J. Jackiewicz and L. Gizon and A. C. Birch},
journal= {arXiv preprint arXiv:astro-ph/0612475},
year = {2007}
}
Comments
4 pages, 3 figures. Proceedings of SOHO18/GONG 2006/HELAS I. Beyond the Spherical Sun: A new era of helio- and asteroseismology. Sheffield, England. August, 2006