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Imaging Convection and Magnetism in the Sun electronic resource by Shravan Hanasoge.

By: Hanasoge, Shravan [author.]Contributor(s): SpringerLink (Online service)Material type: TextTextSeries: SpringerBriefs in MathematicsPublication details: Cham : Springer International Publishing : Imprint: Springer, 2015Edition: 1st ed. 2015Description: XVII, 131 p. 48 illus., 22 illus. in color. online resourceContent type: text Media type: computer Carrier type: online resourceISBN: 9783319273303Subject(s): mathematics | Geotechnical Engineering | Applied mathematics | Engineering mathematics | Computer mathematics | Fluids | Mathematics | Computational Science and Engineering | Geotechnical Engineering & Applied Earth Sciences | Fluid- and Aerodynamics | Appl.Mathematics/Computational Methods of Engineering | Applications of MathematicsDDC classification: 004 LOC classification: QA71-90Online resources: Click here to access online
Contents:
Introduction -- Wave Equation Solver -- Adjoint Optimization -- Adjoint Optimization -- Full Waveform Inversion -- Perspective -- Appendices.- References.
In: Springer eBooksSummary: This book reviews the field of helioseismology and its outstanding challenges and also offers a detailed discussion of the latest computational methodologies. The focus is on the development and implementation of techniques to create 3-D images of convection and magnetism in the solar interior and to introduce the latest computational and theoretical methods to the interested reader. With the increasing availability of computational resources, demand for greater accuracy in the interpretation of helioseismic measurements and the advent of billion-dollar instruments taking high-quality observations, computational methods of helioseismology that enable probing the 3-D structure of the Sun have increasingly become central. This book will benefit students and researchers with proficiency in basic numerical methods, differential equations and linear algebra who are interested in helioseismology.
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Introduction -- Wave Equation Solver -- Adjoint Optimization -- Adjoint Optimization -- Full Waveform Inversion -- Perspective -- Appendices.- References.

This book reviews the field of helioseismology and its outstanding challenges and also offers a detailed discussion of the latest computational methodologies. The focus is on the development and implementation of techniques to create 3-D images of convection and magnetism in the solar interior and to introduce the latest computational and theoretical methods to the interested reader. With the increasing availability of computational resources, demand for greater accuracy in the interpretation of helioseismic measurements and the advent of billion-dollar instruments taking high-quality observations, computational methods of helioseismology that enable probing the 3-D structure of the Sun have increasingly become central. This book will benefit students and researchers with proficiency in basic numerical methods, differential equations and linear algebra who are interested in helioseismology.

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