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Imaging convection and magnetism in the sun

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 t...

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Detalles Bibliográficos
Autor principal: Hanasoge, Shravan
Lenguaje:eng
Publicado: Springer 2015
Materias:
Acceso en línea:https://dx.doi.org/10.1007/978-3-319-27330-3
http://cds.cern.ch/record/2120274
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author Hanasoge, Shravan
author_facet Hanasoge, Shravan
author_sort Hanasoge, Shravan
collection CERN
description 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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institution Organización Europea para la Investigación Nuclear
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spelling cern-21202742021-04-21T19:55:48Zdoi:10.1007/978-3-319-27330-3http://cds.cern.ch/record/2120274engHanasoge, ShravanImaging convection and magnetism in the sunMathematical Physics and MathematicsThis 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.Springeroai:cds.cern.ch:21202742015
spellingShingle Mathematical Physics and Mathematics
Hanasoge, Shravan
Imaging convection and magnetism in the sun
title Imaging convection and magnetism in the sun
title_full Imaging convection and magnetism in the sun
title_fullStr Imaging convection and magnetism in the sun
title_full_unstemmed Imaging convection and magnetism in the sun
title_short Imaging convection and magnetism in the sun
title_sort imaging convection and magnetism in the sun
topic Mathematical Physics and Mathematics
url https://dx.doi.org/10.1007/978-3-319-27330-3
http://cds.cern.ch/record/2120274
work_keys_str_mv AT hanasogeshravan imagingconvectionandmagnetisminthesun