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Imaging Convection and Magnetism in the Sun

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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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Detail Information

Series Title

-

Call Number

004 HAN i

Publisher

: ., 2015

Collation

XVII, 131

Language

English

ISBN/ISSN

978-3-319-27328-0

Classification

004

Content Type

text

Media Type

computer

Carrier Type

online resource

Edition

-

Subject(s)

Computational Science and Engineering

Specific Detail Info

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Statement of Responsibility

Shravan Hanasoge

Other Information

Cataloger

Khusnun

Source

-

Validator

-

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