Solar Hydrodynamics
1st Edition
Will be published approx. on 15. January 2027
Book
Hardback
X, 500 pages
978-3-11-026666-5 (ISBN)
Description
The highly complex processes that take place inside a star like our Sun are the subject of extensive study and several observatories are dedicated solely to this field of research. The Sun's activity directly affects our daily lives, for example, our communications systems; thus, researchers require a reference work that presents the state of research on this subject matter in a coherent manner.
More details
Series
Language
English
Place of publication
Berlin/Boston
Germany
Target group
Professional and scholarly
US School Grade: College Graduate Student
Illustrations
200 Abbildungen
200 b/w ill.
Dimensions
Height: 24 cm
Width: 17 cm
Weight
500 gr
ISBN-13
978-3-11-026666-5 (9783110266665)
Schweitzer Classification
Person
Content
CHAPTER 1. Introduction.
CHAPTER 2. Observations of solar convection.
CHAPTER 3. Toward understanding the physics of solar
CHAPTER 4. Thermal convection in fluid layers: Basic concepts.
CHAPTER 5. Vertical structure of solar convection.
CHAPTER 6. Thermal convection in plane fluid layers and on the
CHAPTER 7. Principles and achievements of helioseismology.
CHAPTER 8. Sunspots and local solar magnetic fields.
CHAPTER 9. Solar differential rotation and meridional circulation.
CHAPTER 10. Global magnetic field of the Sun and the 11-year
CHAPTER 11. Mean-field electrodynamics and models of turbulent
CHAPTER 12. Gasdynamic phenomena in the solar chromosphere
CHAPTER 13. Conclusion.
CHAPTER 2. Observations of solar convection.
CHAPTER 3. Toward understanding the physics of solar
CHAPTER 4. Thermal convection in fluid layers: Basic concepts.
CHAPTER 5. Vertical structure of solar convection.
CHAPTER 6. Thermal convection in plane fluid layers and on the
CHAPTER 7. Principles and achievements of helioseismology.
CHAPTER 8. Sunspots and local solar magnetic fields.
CHAPTER 9. Solar differential rotation and meridional circulation.
CHAPTER 10. Global magnetic field of the Sun and the 11-year
CHAPTER 11. Mean-field electrodynamics and models of turbulent
CHAPTER 12. Gasdynamic phenomena in the solar chromosphere
CHAPTER 13. Conclusion.