The present set of lectures is devoted to magnetohydrodynamic turbulence in astrophysics, with strong emphasis on numerical simulations. The book strives for a balance between state-of-the-art reports and a tutorial approach. It is thus particularly suited as an introduction to the field for nonspec
[Lecture Notes in Physics] Turbulence and Magnetic Fields in Astrophysics Volume 614 || Recent Developments in Magnetic Dynamo Theory
β Scribed by Falgarone, Edith; Passot, Thierry
- Book ID
- 120030422
- Publisher
- Springer Berlin Heidelberg
- Year
- 2003
- Tongue
- German
- Weight
- 404 KB
- Edition
- 2003
- Category
- Article
- ISBN
- 354000274X
No coin nor oath required. For personal study only.
β¦ Synopsis
The present set of lectures is devoted to magnetohydrodynamic turbulence in astrophysics, with strong emphasis on numerical simulations. The book strives for a balance between state-of-the-art reports and a tutorial approach. It is thus particularly suited as an introduction to the field for nonspecialist researchers and postgraduate students. In addition, experienced scientists in the field will find the book to be a comprehensive source of reference for their research.
π SIMILAR VOLUMES
The present set of lectures is devoted to magnetohydrodynamic turbulence in astrophysics, with strong emphasis on numerical simulations. The book strives for a balance between state-of-the-art reports and a tutorial approach. It is thus particularly suited as an introduction to the field for nonspec
The present set of lectures is devoted to magnetohydrodynamic turbulence in astrophysics, with strong emphasis on numerical simulations. The book strives for a balance between state-of-the-art reports and a tutorial approach. It is thus particularly suited as an introduction to the field for nonspec
The physics of strongly interacting matter in an external magnetic field is presently emerging as a topic of great cross-disciplinary interest for particle, nuclear, astro- and condensed matter physicists. It is known that strong magnetic fields are created in heavy ion collisions, an insight that h