This paper demonstrates a method to calculate the magnetic field distribution in and around a 3D object when it is magnetized by a strong homogeneous magnetic field. The numerical technique is based on the explicit finite difference method. The calculation method is validated against analytical solu
β¦ LIBER β¦
3D numerical models of magnetic field evolution in galaxies interacting with the ICM
β Scribed by Katarzyna Otmianowska-Mazur; Bernd Vollmer
- Book ID
- 110389183
- Publisher
- Springer Netherlands
- Year
- 2002
- Tongue
- English
- Weight
- 131 KB
- Volume
- 281
- Category
- Article
- ISSN
- 0004-640X
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