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Imaging Convection and Magnetism in the Sun

  • Shravan Hanasoge
Book

Part of the SpringerBriefs in Mathematics book series (BRIEFSMATH)

Table of contents

  1. Front Matter
    Pages i-xvii
  2. Shravan Hanasoge
    Pages 1-19
  3. Shravan Hanasoge
    Pages 21-45
  4. Shravan Hanasoge
    Pages 47-73
  5. Shravan Hanasoge
    Pages 75-103
  6. Shravan Hanasoge
    Pages 105-107
  7. Back Matter
    Pages 109-131

About this book

Introduction

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.

Keywords

Constrained optimization Helioseismology Homogenization Inverse problems Magnetohydrodynamics Numerical Methods Wave propagation in random media

Authors and affiliations

  • Shravan Hanasoge
    • 1
  1. 1.Department of Astronomy and AstrophysicsTata Institute of Fundamental ResearchMumbaiIndia

Bibliographic information

  • DOI https://doi.org/10.1007/978-3-319-27330-3
  • Copyright Information The Author 2015
  • Publisher Name Springer, Cham
  • eBook Packages Mathematics and Statistics
  • Print ISBN 978-3-319-27328-0
  • Online ISBN 978-3-319-27330-3
  • Series Print ISSN 2191-8198
  • Series Online ISSN 2191-8201
  • Buy this book on publisher's site