Overview

Recent progress in instrumentation and observational techniques has brought a wealth of new information to astronomists about the sun. This introductory text presents a complete overview of solar physics, including present knowledge of the subject and problems yet to be investigated. The increasing number of observations of solar phenomena in neighbouring stars will make this text of interest not only to students specializing in solar physics but also to researchers interested in stellar structure and the solar-stellar connection.

Full Product Details

Author:   Michael Stix
Publisher:   Springer-Verlag Berlin and Heidelberg GmbH & Co. KG
Imprint:   Springer-Verlag Berlin and Heidelberg GmbH & Co. K
Edition:   Softcover reprint of the original 1st ed. 1989
Dimensions:   Width: 15.50cm , Height: 2.10cm , Length: 23.50cm
Weight:   0.620kg
ISBN:  

9783540537960

ISBN 10:   3540537961
Pages:   390
Publication Date:   28 May 1991
Audience:   College/higher education ,  Professional and scholarly ,  Undergraduate ,  Postgraduate, Research & Scholarly
Replaced By:   9783642624773
Format:   Paperback
Publisher's Status:   Active
Availability:   Out of stock  
The supplier is temporarily out of stock of this item. It will be ordered for you on backorder and shipped when it becomes available.

Table of Contents

1. Introduction: The Sun’s Distance, Mass, Radius, Luminosity ....- 1.1 Distance.- 1.2 Mass.- 1.3 Radius.- 1.4 Luminosity.- 1.5 Spectral Energy Distribution.- 1.6 Bibliographical Notes.- 2. Internal Structure.- 2.1 Construction of a Model.- 2.2 Age and Pre-Main-Sequence Evolution.- 2.3 Model Ingredients.- 2.4 Results for a Standard Solar Model.- 2.5 Non-Standard Models.- 2.6 Bibliographical Notes.- 3. Tools for Solar Observation.- 3.1 Limitations.- 3.2 High-Resolution Telescopes.- 3.3 Spectrographs and Spectrometers.- 3.4 Filters and Monochromators.- 3.5 Magnetic Fields and Polarimetry.- 3.6 Special-Purpose Instruments.- 3.7 Bibliographical Notes.- 4. The Atmosphere.- 4.1 Radiative Transfer — Local Thermodynamic Equilibrium.- 4.2 Radiative Transfer — Statistical Equilibrium.- 4.3 Atmospheric Models.- 4.4 The Chemical Composition of the Sun.- 4.5 Bibliographical Notes.- 5. Oscillations.- 5.1 Observations.- 5.2 Linear Adiabatic Oscillations of a Non-rotating Sun.- 5.3 Helioseismology.- 5.4 Excitation and Damping.- 5.5 Bibliographical Notes.- 6. Convection.- 6.1 Stability.- 6.2 Mixing-Length Theory.- 6.3 Granulation.- 6.4 Mesogranulation.- 6.5 Supergranulation.- 6.6 Giant Cells.- 6.7 Bibliographical Notes.- 7. Rotation.- 7.1 Axis of Rotation.- 7.2 Oblateness.- 7.3 Rotational History.- 7.4 Surface Observations.- 7.5 Models of a Rotating Convection Zone.- 7.6 Bibliographical Notes.- 8. Magnetism.- 8.1 Fields and Conducting Matter.- 8.2 Flux Tubes.- 8.3 Sunspots.- 8.4 The Solar Cycle.- 8.5 Bibliographical Notes.- 9. Chromosphere, Corona, and Solar Wind.- 9.1 Empirical Facts.- 9.2 Consequences of High Temperature.- 9.3 The Magnetic Field in the Outer Atmosphere.- 9.4 The Energy Balance.- 9.5 Explosive Events.- 9.6 Bibliographical Notes.- List of Symbols.- References.

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