Buch, Englisch, Band 154, 744 Seiten, Format (B × H): 175 mm x 250 mm, Gewicht: 1433 g
Buch, Englisch, Band 154, 744 Seiten, Format (B × H): 175 mm x 250 mm, Gewicht: 1433 g
Reihe: International Series of Monographs on Physics
ISBN: 978-0-19-964174-1
Verlag: ACADEMIC
Ongoing studies in mathematical depth, and inferences from `helioseismological' observations of the internal solar rotation have shown up the limitations in our knowledge of the solar interior and of our understanding of the solar dynamo, manifested in particular by the sunspot cycle, the Maunder minimum, and solar flares. This second edition retains the identical overall structure as the first edition, but is designed so as to be self-contained with the early
chapters presenting the basic physics and mathematics underlying cosmical magnetohydrodynamics, followed by studies of the specific applications appropriate for a book devoted to a central area in astrophysics.
Zielgruppe
Graduate students and researchers in theoretical astrophysics and plasma physics, as well as observers and experimentalists.
Autoren/Hrsg.
Fachgebiete
Weitere Infos & Material
1: Introduction
2: Theoretical basis
3: Applications
4: Magnetism and convection
5: Magnetic fields in stellar interiors
6: Dynamo processes in stars
7: Stellar winds: magnetic braking
8: Late-type stars
9: The early-type magnetic stars
10: Pre-main sequence stars
11: Magnetism and star formation I
12: Magnetism and star formation II
13: Pulsar electrodynamics I
14: Pulsar electrodynamics II
Index




