Buch, Englisch, 131 Seiten, Format (B × H): 155 mm x 235 mm, Gewicht: 2409 g
Buch, Englisch, 131 Seiten, Format (B × H): 155 mm x 235 mm, Gewicht: 2409 g
Reihe: SpringerBriefs in Mathematics
ISBN: 978-3-319-27328-0
Verlag: Springer International Publishing
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.
Zielgruppe
Research
Autoren/Hrsg.
Fachgebiete
- Naturwissenschaften Astronomie Sonnensystem: Sonne und Planeten
- Mathematik | Informatik Mathematik Numerik und Wissenschaftliches Rechnen Numerische Mathematik
- Mathematik | Informatik Mathematik Numerik und Wissenschaftliches Rechnen Angewandte Mathematik, Mathematische Modelle
- Geowissenschaften Geologie Vulkanologie, Seismologie
Weitere Infos & Material
Introduction.- Wave Equation Solver.- Adjoint Optimization.- Adjoint Optimization.- Full Waveform Inversion.- Perspective.- Appendices.- References.
