Sensitivity of solar f-mode travel times to internal flows

Details Sensitivity of solar f-mode travel times to internal flows Sensitivity of solar f-mode travel times to internal flows

2006-08-28

arxiv.org/abs/astro-ph/0608604v1

ESA-SP 617, 2006

Astronomy and Astrophysics

Astrophysics

Conference proceedings of SOHO 17, 7-11 May, 2006, Giardini Naxos, Italy. 4 pages

Scientific paper

We compute f-mode travel-time sensitivity kernels for flows. Using a two-dimensional model, we show that it is important to account for several systematic effects, such as the foreshortening and the projection of the velocity vector onto the line of sight. Correcting for these effects is necessary before any data inversion is attempted away from the center of the solar disk.

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