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Gung Yuancheng, Hsu Ya-Ting, Chiao Ling-Yun, Obayashi Masayuki, . (2009). Multiscale waveform tomography with two-step model parameterization
. J. Geophys. Res., 114(B11), B11301–.
Abstract: In geophysical tomography, a proper model parameterization scheme for forward modeling is not necessarily a suitable one for the inversion stage, and vice versa. To take full advantage of the merits of parameterization in both stages, we propose a two-step model parameterization approach, in which different model bases for forward computation and inversion are adopted and the basis change is achieved by applying a spatial projection directly to the sensitivity matrix. We demonstrate this approach through an experimental study of waveform tomography for the Pacific upper mantle shear wave structure using first-orbit long-period Rayleigh waves. In the forward modeling, a normal-mode-based nonlinear asymptotic coupling theory is used for the computation of the synthetics and sensitivity matrix, and the model is parameterized in terms of spherical harmonics which provide efficient analytical solutions for path integrals in the forward modeling. Prior to the inversion, the model basis of the sensitivity matrix is transformed to local functions within the study region. After mapping, only local bases around the data sampling path receive effective sensitivities. Accordingly, the computation cost in the inversion is significantly reduced. Furthermore, the two-step model parameterization also adds flexibility to the inversion schemes. In particular, a wavelet-based multiscale inversion is implemented, and its results are compared to simple damping solutions. The general concept and applications of the two-step model parameterization are not restricted to the forwarding modeling technique or model parameterization schemes employed in this experimental study. This approach benefits any inverse problems wherever transformation of model bases helps to better constrain the results.
Keywords: multiscale tomography, two-step model parameterization, nonlinear asymptotic coupling theory, 3260 Mathematical Geophysics: Inverse theory, 7270 Seismology: Tomography, 7255 Seismology: Surface waves and free oscillations,
Programme: 133
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Chessa J.P., Peterscu I., Bentahir M., Van Beeumen J. & Gerday C. (2000). Purification, physico-chemical characterization and sequense of a heat labile alkaline metalloprotease isolated from a psychrophilic Pseudomonas species. Biochim. Biophys. Acta, 1479, 265–274.
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. (1999). Changes in depth utilization in relation to the breeding stage: a case study with the king penguin aptendytes patagonicus. Marine ornithology, 27, 43–47.
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Hamilton J-Ch, Charlassier R, Cressiot C, Kaplan J, Piat M, Rosset C, . (2008). Sensitivity of a bolometric interferometer to the cosmic microwave backgroud power spectrum
. A&A, 491(3), 923–927.
Abstract: Context. The search for B-mode polarization fluctuations in the Cosmic Microwave Background is one of the main challenges of modern cosmology. The expected level of the B-mode signal is very low and therefore requires the development of highly sensitive instruments with low systematic errors. An appealing possibility is bolometric interferometry. Aims. We compare in this article the sensitivity on the CMB angular power spectrum achieved with direct imaging, heterodyne and bolometric interferometry. Methods. Using a simple power spectrum estimator, we calculate its variance leading to the counterpart for bolometric interferometry of the well known Knox formula for direct imaging. Results. We find that bolometric interferometry is less sensitive than direct imaging. However, as expected, it is finally more sensitive than heterodyne interferometry due to the low noise of the bolometers. It therefore appears as an alternative to direct imagers with different and possibly lower systematic errors, mainly due to the absence of an optical setup in front of the horns.
Programme: 915
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