Cosmic Ray Astrophysics: Astronomy and Astrophysics Library
Autor Reinhard Schlickeiseren Limba Engleză Hardback – 9 oct 2001
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Specificații
ISBN-13: 9783540664659
ISBN-10: 3540664653
Pagini: 536
Ilustrații: XV, 519 p. 30 illus., 2 illus. in color.
Dimensiuni: 155 x 235 x 40 mm
Greutate: 0.85 kg
Ediția:2002
Editura: Springer Berlin, Heidelberg
Colecția Springer
Seria Astronomy and Astrophysics Library
Locul publicării:Berlin, Heidelberg, Germany
ISBN-10: 3540664653
Pagini: 536
Ilustrații: XV, 519 p. 30 illus., 2 illus. in color.
Dimensiuni: 155 x 235 x 40 mm
Greutate: 0.85 kg
Ediția:2002
Editura: Springer Berlin, Heidelberg
Colecția Springer
Seria Astronomy and Astrophysics Library
Locul publicării:Berlin, Heidelberg, Germany
Public țintă
GraduateCuprins
1. Introduction.- 2. Cosmic Rays as Part of the Universe.- 3. Direct Observations of Cosmic Rays.- 4. Interactions of Cosmic Ray Electrons.- 5. Interactions of Cosmic Ray Nuclei.- 6. Indirect Observations of Cosmic Rays.- 7. Immediate Consequences of Galactic Cosmic Ray Observations.- 8. Statistical Mechanics of Charged Particles.- 9. Test Wave Approach 1. Waves in Cold Magnetized Plasmas.- 10. Test Wave Approach 2. Waves in Hot Magnetized Isotropic Plasmas.- 11. Test Wave Approach 3. Generation of Plasma Waves.- 12. Test Particle Approach 1. Hierarchy of Transport Equations.- 13. Test Particle Approach 2. Calculation of Transport Parameters.- 14. Acceleration and Transport Processes of Cosmic Rays.- 15. Interplanetary Transport of Cosmic Ray Particles.- 16. Acceleration of Cosmic Ray Particles at Shock Waves.- 17. Galactic Cosmic Rays.- 18. Formation of Cosmic Ray Momentum Spectra.- 19. Summary and Outlook.- Append.- A. Radiation Transport.- B. Conductivity Tensor in a Hot Magnetized Plasma.- B.1 The General Case.- B.2 Isotropic Distribution Functions.- C. Calculation of the Integral (10.3.10).- References.- Illustration Credits.
Recenzii
From the reviews of the first edition:
"This excellent book is the most complete development of cosmic ray astrophysics theory published. It is aimed at current researchers and commencing postgraduate students. … One of the great benefits of this book is the explicit description of all the assumptions that are made and the limitations they imply on interpretations from the theory. This makes the book particularly valuable for postgraduate students and established researchers starting in the field." (M.L. Duldig, The Physicist, Vol.39 (3), 2002)
"This excellent book is the most complete development of cosmic ray astrophysics theory published. It is aimed at current researchers and commencing postgraduate students. … One of the great benefits of this book is the explicit description of all the assumptions that are made and the limitations they imply on interpretations from the theory. This makes the book particularly valuable for postgraduate students and established researchers starting in the field." (M.L. Duldig, The Physicist, Vol.39 (3), 2002)
Textul de pe ultima copertă
This book provides an exhaustive account of the origin and dynamics of cosmic rays. Divided into three parts, it first gives an up-to-date summary of the observational data, then -- in the following theory section -- deals with the kinetic description of cosmic ray plasma. The underlying diffusion-convection transport equation, which governs the coupling between cosmic rays and the background plasma, is derived and analyzed in detail. In the third part, several applications of the solutions of the transport equation are presented and how key observations in cosmic ray physics can be accounted for is demonstrated. The applications include cosmic ray modulation, acceleration near shock waves and the galactic propagation of cosmic rays. While the book is primarily of interest to scientists working at the forefront of research, the very careful derivations and explanations make it suitable also as an introduction to the field of cosmic rays for graduate students.
Caracteristici
This is the only modern book on the market All competitive titles date back to 1990 and do not take the latest developments into account Includes supplementary material: sn.pub/extras