
An Introduction to Waves and Oscillations in the Sun
Description
Alles über E-Books | Antworten auf Fragen rund um E-Books, Kopierschutz und Dateiformate finden Sie in unserem Info- & Hilfebereich.
Reviews / Votes
From the reviews:
"The book . give an introductory development of the theory of wave motion and oscillations in the sun and describe the experimental and observational work that has been done. . Much of the material in this book is presented at an introductory level that would be accessible to students in an advanced undergraduate or graduate course on the subject. . The book can . be a valuable resource for scientists at any level working in this area." (Stephen Wollman, Zentralblatt MATH, Vol. 1262, 2013)More details
Other editions
Additional editions


Person
Content
Chapter 1: Introduction.- 1.1: Historical Perspectives.- 1.2: The Core of the Sun.- 1.3: Radiative Zone.- 1.4: Convection Zone.- 1.5: Photosphere.- 1.6: Chromosphere.- 1.7: Corona.- 1.8: Solar Wind.- Chapter 2: Electro-Magneto Statics.- 2.1: Charge and Current Distributions.- 2.2: Coulomb's Law.- 2.3: Gauss's Law.- 2.4: Ampere's Law.- 2.5: Faraday's Law.- 2.6: Vector Magnetic Potential.- 2.7: Maxwell's Equations.- Chapter 3: MHD Equations and Concepts.- 3.1: Assumptions.- 3.2: Dimensionless Parameters.- 3.3: Mass Continuity.- 3.4: Equations of Motion.- 3.5: Energy Equation.- 3.6: MHD Equilibrium.- 3.7: Magnetic Flux Tubes.- 3.8: Current-free (Potential) fields.- 3.9: Force-Free Fields.- 3.10: Parker's Solution for Solar Wind.- Chapter 4: Waves in Uniform Media.- 4.1: Basic Equations.- 4.2: SoundWaves.- 4.3: Alfv'enWaves.- 4.4: Shear Alfv'enWaves.- 4.5: Compressional Alfv'enWaves.- 4.6: Magneto acoustic Waves.- 4.7: Internal and Magneto acoustic Gravity Waves.- 4.8: Phase-Mixing and Resonant Absorption of Waves.- Chapter 5: Waves in Non-Uniform Media- 5.1: Waves at Magnetic Interface.- 5.2: Surface and InterfacialWaves.- 5.3: Waves in a Magnetic Slab.- 5.4: Waves in Cylindrical Geometries.- 5.5: Waves in Untwisted and Twisted Tubes.- Chapter 6: Instabilities.- 6.1: Introduction.- 6.2: Rayleigh-Taylor (RT) Instability.- 6.3: Kelvin-Helmholtz (KH) Instability.- 6.4: Parametric Instability.- 6.5: Parker Instability.- Chapter 7: Waves in the Sun.- 7.1: Five minute oscillations.- 7.2: Oscillations in Sunspots.- 7.3: Chromospheric Oscillations.- 7.4: CoronalWaves.- 7.5: Coronal Seismology.- 7.6: Coronal Heating due to Waves.- 7.7: EIT and MoretonWaves.- Chapter 8: Heliosesimology.- 8.1: Equations of Motion.- 8.2: Equilibrium Structure.- 8.3: Perturbation Analysis.- 8.4: Acoustic Waves.- 8.5: Internal Gravity Waves.- 8.6: Equations of Linear Stellar Oscillations.- 8.7: Properties of Solar Oscillations (Internal).- 8.8: p and g modes.- References.- Index.
System requirements
File format: PDF
Copy protection: Watermark-DRM (Digital Rights Management)
System requirements:
- Computer (Windows; MacOS X; Linux): Use the free software Adobe Reader, Adobe Digital Editions, or any other PDF viewer of your choice (see eBook Help).
- Tablet/Smartphone (Android; iOS): Install the free app Adobe Digital Editions or another reading app for eBooks, e.g., PocketBook (see eBook Help).
- E-reader: Bookeen, Kobo, Pocketbook, Sony, Tolino and many more (only limited: Kindle).
The file format PDF always displays a book page identically on any hardware. This makes PDF suitable for complex layouts such as those used in textbooks and reference books (images, tables, columns, footnotes). Unfortunately, on the small screens of e-readers or smartphones, PDFs are rather annoying, requiring too much scrolling.
This eBook uses Watermark-DRM, a „soft” copy protection. This means that there are no technical restrictions to prevent illegal distribution. However, there is a personalised watermark embedded in the eBook that can be used to identify the purchaser of the eBook in the event of misuse and to provide evidence for legal purposes.
For more information, see our eBook Help page.