F-mode sensitivity kernels for flows

Details F-mode sensitivity kernels for flows F-mode sensitivity kernels for flows

2006-12-17

arxiv.org/abs/astro-ph/0612475v1

ESA-SP 624, 2006

Astronomy and Astrophysics

Astrophysics

4 pages, 3 figures. Proceedings of SOHO18/GONG 2006/HELAS I. Beyond the Spherical Sun: A new era of helio- and asteroseismolog

Scientific paper

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.

Affiliated with

Also associated with

No associations

Rating

F-mode sensitivity kernels for flows does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with F-mode sensitivity kernels for flows, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and F-mode sensitivity kernels for flows will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-609424