Imaging Convection and Magnetism in the Sun
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Beschreibung
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.
Reviews the major successes of helioseismology as well as outstanding challenges that are still faced today Includes a detailed discussion of the latest computational methodologies Contains a section on solutions First book on helioseismology that covers a wide range of topics Reviews some of the major successes of helioseismology while focusing on the outstanding challenges that are still faced today Discusses and draws from methods widely used in terrestrial seismology Includes a detailed discussion of the latest relevant computational methodologies Ties together the inverse and forward problems using computation Includes supplementary material: sn.pub/extras
Autor*in
Shravan Hanasoge
Themen in »Imaging Convection and Magnetism in the Sun«
Constrained optimization Helioseismology Homogenization Inverse problems Magnetohydrodynamics Numerical Methods Wave propagation in random media fluid- and aerodynamics