Ryutova Physics of Magnetic Flux Tubes

2. Auflage 2018
ISBN: 978-3-319-96361-7
Verlag: Springer International Publishing
Format: PDF
Kopierschutz: 1 - PDF Watermark

E-Book, Englisch, Band 455, 747 Seiten, eBook

Reihe: Astrophysics and Space Science Library

This book presents the physics of magnetic flux tubes, including their fundamental properties and collective phenomena in an ensemble of flux tubes. The physics of magnetic flux tubes is vital for understanding fundamental processes in the solar atmosphere that are shaped and governed by magnetic fields. The concept of magnetic flux tubes is also central to various magnetized media ranging from laboratory plasma and Earth's magnetosphere to planetary, stellar and galactic environments. The book covers both theory and observations. Theoretical models presented in analytical and phenomenological forms that are tailored to practical applications. These are welded together with empirical data extending from the early pioneering observations to the most recent state-of-the-art data. This new edition of the book is updated and contains a significant amount of new material throughout as well as four new chapters and 48 problems with solutions. Most problems make use of original papers containing fundamental results. This way, the original paper, often based on complex theory, turns into a convenient tool for practical use and quantitative analysis.

Zielgruppe

Research

Autoren/Hrsg.

Ryutova, Margarita

Inhaltsverzeichnis

Preface.- The Sun’s Magnetic Fields.- A Quick Look on Small-Scale Flux Tubes.- Intrinsic Properties of Flux Tubes – Wave Phenomena.- Effects of Flux Tube Inhomogeneities and  Weak Nonlinearity.- Flux Tube Dynamics in the Presence of Mass Flows.- Collective Phenomena Ensembles of Flux Tubes.- Effects of Magnetic Flux Tubes in Helioseismology.- Wave Phenomena in Dense Conglomerate of Flux Tubes.- Nonlinear Wave Phenomena in Dense Conglomerate of Flux Tubes.- Magnetosonic Streaming.- Moving Magnetic Features (MMFs).- Reconnection of Flux Tubes – Specifics of High Plasma ß.- Post-Reconnection Processes – Shocks, Jets and Microflares.- Photospheric Network as Energy Source for Quiet-Sun Corona.- Response of the Corona to Magnetic Activity in Underlying Plage Regions.- Electrodynamic Coupling of Active Region Corona with the Photosphere.- Fine Structure of Penumbrae: Formation and Dynamics.- Bow Shocks and Plasma Jetting over Penumbrae.- Selforganization in the Corona and Flare Precursors.- Quiescent Prominences.- Laboratory Experiments Scaled to Solar and Space Plasmas.- What to Observe in Low Atmosphere.- What to Observe in the Upper Atmosphere.- Solutions.

Über Autor(innen)

Margarita Ryutova (Kemoklidze) received her MSc and PhD from the famous Landau Theoretical Department, Kapitsa Institute for Physical Problems, Moscow and worked there until she married and moved to Budker Institute  of Nuclear Physics. Since 1994 she lives in the United States where she has been affiliated with Stanford Lockheed Institute for Space Research in Palo Alto and Lawrence Livermore National laboratory.She has 30 years of experience in teaching undergraduate and graduate courses in Physics and Mathematics. This includes supervising graduate and PhD students. She has published over 100 research papers and reviews in various fields of theoretical and experimental physics such as Statistical Physics, Solar Physics, Laboratory and Plasma Astrophysics, Nonlinear Fluid Dynamics, Solitons, Shocks and Selforganization, Superfluidity and Superconductivity.Along with research in physics, she works in and has published books and essays on the history of physics and mathematics.