F-mode sensitivity kernels for flows

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dc.creatorJackiewicz, J.
dc.creatorGizon, L.
dc.creatorBirch, A. C.
dc.date2006-12-17
dc.date.accessioned2026-07-07T07:35:29Z
dc.date.available2026-07-07T07:35:29Z
dc.descriptionWe 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.
dc.description4 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
dc.identifierhttps://arxiv.org/abs/astro-ph/0612475
dc.identifierhttp://arxiv.org/abs/astro-ph/0612475
dc.identifierESA-SP 624, 2006
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/120110
dc.subjectAstrophysics
dc.titleF-mode sensitivity kernels for flows
dc.typetext

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