Solving the forward problem of helioseismology in the frequency domain
GIZON, Laurent
Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
Institut für Astrophysik [Göttingen]
Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
Institut für Astrophysik [Göttingen]
BARUCQ, Hélène
Advanced 3D Numerical Modeling in Geophysics [Magique 3D]
Laboratoire de Mathématiques et de leurs Applications [Pau] [LMAP]
Advanced 3D Numerical Modeling in Geophysics [Magique 3D]
Laboratoire de Mathématiques et de leurs Applications [Pau] [LMAP]
DURUFLÉ, Marc
Advanced 3D Numerical Modeling in Geophysics [Magique 3D]
Institut de Mathématiques de Bordeaux [IMB]
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Advanced 3D Numerical Modeling in Geophysics [Magique 3D]
Institut de Mathématiques de Bordeaux [IMB]
GIZON, Laurent
Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
Institut für Astrophysik [Göttingen]
Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
Institut für Astrophysik [Göttingen]
BARUCQ, Hélène
Advanced 3D Numerical Modeling in Geophysics [Magique 3D]
Laboratoire de Mathématiques et de leurs Applications [Pau] [LMAP]
Advanced 3D Numerical Modeling in Geophysics [Magique 3D]
Laboratoire de Mathématiques et de leurs Applications [Pau] [LMAP]
DURUFLÉ, Marc
Advanced 3D Numerical Modeling in Geophysics [Magique 3D]
Institut de Mathématiques de Bordeaux [IMB]
Advanced 3D Numerical Modeling in Geophysics [Magique 3D]
Institut de Mathématiques de Bordeaux [IMB]
BIRCH, C. Aaron
Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
CHABASSIER, Juliette
Laboratoire de Mathématiques et de leurs Applications [Pau] [LMAP]
Advanced 3D Numerical Modeling in Geophysics [Magique 3D]
Laboratoire de Mathématiques et de leurs Applications [Pau] [LMAP]
Advanced 3D Numerical Modeling in Geophysics [Magique 3D]
HANSON, Cristopher
Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
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Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
Idioma
en
Communication dans un congrès
Este ítem está publicado en
THE 12TH INTERNATIONAL CONFERENCE ON MATHEMATICAL AND NUMERICAL ASPECTS OF WAVE PROPAGATION, 2015-07-20, Karlsruhe.
Resumen en inglés
Solar acoustic waves are continuously excited by turbulent convection (a random process). The forward problem of local helioseismology was specified at the Waves 2013 conference: computing the cross-covariance of the wave ...Leer más >
Solar acoustic waves are continuously excited by turbulent convection (a random process). The forward problem of local helioseismology was specified at the Waves 2013 conference: computing the cross-covariance of the wave field between any two locations on the solar surface. Here we solve the problem in the frequency domain using the finite element solver Montjoie. One of the specificities of propagation/scattering problems in the Sun is the very sharp decrease of sound speed and density with radius near the surface. We show that the problem simplifies considerably under the assumption that the co-variance function of the source of excitation is proportional to the attenuation.< Leer menos
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Importado de HalCentros de investigación