Overview

A wealth of new experimental and theoretical results has been obtained in solar physics since the first edition of this textbook appeared in 1989. Thus all nine chapters have been thoroughly revised, and about 100 pages and many new illustrations have been added to the text. The additions include element diffusion in the solar interior, the recent neutrino experiments, methods of image restoration, observational devices used for spectroscopy and polarimetry, and new developments in helioseismology and numerical simulation. The book takes particular advantage of the results of several recent space missions, which lead to substantial progress in our understanding of the Sun, from the deep interior to the corona and solar wind.

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:   2nd ed. 2002. Corr. 2nd printing 2004
Dimensions:   Width: 15.50cm , Height: 2.50cm , Length: 23.50cm
Weight:   1.022kg
ISBN:  

9783540207412

ISBN 10:   3540207414
Pages:   492
Publication Date:   23 January 2004
Audience:   College/higher education ,  Tertiary & Higher Education
Format:   Hardback
Publisher's Status:   Active
Availability:   Out of stock  
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Table of Contents

1. Characteristics of the Sun.- 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 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 The Angular Velocity of the Sun.- 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.

Reviews

From the reviews: <p> This is the definitive book on the physics of the sun, and if thata (TM)s your interest, then I can thoroughly recommend it. (C.R. Kitchin, Astronomy Now, June 2003) <p> This is an excellent introduction to the whole of Solar physics at a consistent level of mathematics and assumed physics background. It would be suitable as a reference for some advance undergraduate courses and should be compulsory reading for postgraduate students studying the Sun. It could also be read with interest by anyone with a physics background wishing to learn more detail about the Sun than is available online or through general astrophysics books. (International Journal of Astrobiology, 2/1, 2003) <p> The book from the Springer Astronomy and Astrophysics Library Series gives an introduction to the physics of the Sun. [...] From an amateur solar observera (TM)s perspective, there are many parts of the book which are of interest. [...] This book has been well produced with plenty of diagrams and photographs (with a view in colour) throughout. (The Astronomer, 39/465, 2003) <p> This must-have book is of great value to every Sun specialist as well to students or graduates. Nearly each sub-chapter contains a small number of problems linked to the previous paragraphs, and this invitation to become a more active reader must be encouraged. (Physicalia 2005, 57, page 211-212) <p>From the reviews of the second edition: <p> This book provides a solid and extremely readable introduction to the physics and the phenomenology of the solar interior and lower atmosphere a ] . its status as a classic is well deserved. It is a delight to read, and I can recommend it strongly a ] . the book iswell presented and easy to use. It is amply and appropriately illustrated a ] . The author conveniently includes bibliographic notes a ] . will continue to be a basic reference text a ] . (Dr. L. Fletcher, Contemporary Physics, Vol. 46 (4), 2005) <p> This is a serious introduction to solar physics. a ] The maths is effectively aimed at the serious senior undergraduate or post graduate student. a ] This second edition updates the original 1989 publication a ] . It is essentially an advanced text book with problems set throughout. a ] There is a much needed list of symbols a ] list of references and a comprehensive index. (Roger Feasey, Journal of the Auckland Astronomical Society, December, 2004) <p> The first edition, published in 1989, was excellent. It was clear, thorough, well illustrated and well referenced. a ] The second edition is just as good and has been brought right up to date. a ] The Sun is a member of Springera (TM)s highly commendable Astronomy and Astrophysics Library and is a first-class example of what a good textbook should be. (David W. Hughes, The Observatory, Vol. 124 (1183), 2004) <p> This book is an introduction to the physics of the Sun a ] . This must-have book is of great value to every Sun specialist as well as to students or graduates. Nearly each sub-chapter contains a small number of problems linked to the previous paragraphs, and this invitation to become a more active reader must be encouraged. (Gaston Marrette, Physicalia, Vol. 57 (3), 2005) <p>

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