Imaging Convection and Magnetism in the Sun

Nonfiction, Science & Nature, Science, Earth Sciences, Computers, Advanced Computing, Computer Science
Cover of the book Imaging Convection and Magnetism in the Sun by Shravan Hanasoge, Springer International Publishing
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Author: Shravan Hanasoge ISBN: 9783319273303
Publisher: Springer International Publishing Publication: December 24, 2015
Imprint: Springer Language: English
Author: Shravan Hanasoge
ISBN: 9783319273303
Publisher: Springer International Publishing
Publication: December 24, 2015
Imprint: Springer
Language: English

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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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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