With an emphasis on numerical modelling, Physics of the Sun: A First Course presents a quantitative examination of the physical structure of the Sun and the conditions of its extended atmosphere.
With an emphasis on numerical modelling, Physics of the Sun: A First Course presents a quantitative examination of the physical structure of the Sun and the conditions of its extended atmosphere.Hinweis: Dieser Artikel kann nur an eine deutsche Lieferadresse ausgeliefert werden.
Dermott J. Mullan is an Emeritus Professor in the Department of Physics and Astronomy at the University of Delaware.
Inhaltsangabe
1. The Global Parameters of the Sun. 2. Radiation Flow through the Solar Atmosphere. 3. Toward a Model of the Sun: Opacity. 4. Toward a Model of the Sun: Ionization. 5. Computing a Model of the Sun: The Photosphere. 6. Convection in the Sun: Empirical Properties. 7. Computing a Model of the Sun: The Convection Zone. 8. Radiative Transfer in the Deep Interior of the Sun. 9. Computing a Mechanical Model of the Sun: The Radiative Interior. 10. Polytropes. 11. Energy Generation in the Sun. 12. Neutrinos from the Sun. 13. Oscillations in the Sun: The Observations. 14. Oscillations in the Sun: Theory. 15. The Chromosphere. 16. Magnetic Fields in the Sun. 17. The Corona. 18. The Solar Wind.
1. The Global Parameters of the Sun. 2. Radiation Flow through the Solar Atmosphere. 3. Toward a Model of the Sun: Opacity. 4. Toward a Model of the Sun: Ionization. 5. Computing a Model of the Sun: The Photosphere. 6. Convection in the Sun: Empirical Properties. 7. Computing a Model of the Sun: The Convection Zone. 8. Radiative Transfer in the Deep Interior of the Sun. 9. Computing a Mechanical Model of the Sun: The Radiative Interior. 10. Polytropes. 11. Energy Generation in the Sun. 12. Neutrinos from the Sun. 13. Oscillations in the Sun: The Observations. 14. Oscillations in the Sun: Theory. 15. The Chromosphere. 16. Magnetic Fields in the Sun. 17. The Corona. 18. The Solar Wind.
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