The origin of primeval magnetic fields: Self-consistent simulation of magnetic field generation and amplification
Autor: | H. Wiechen, G. T. Birk, Harald Lesch |
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Rok vydání: | 2000 |
Předmět: | |
Zdroj: | Physics of Plasmas. 7:701-705 |
ISSN: | 1089-7674 1070-664X |
DOI: | 10.1063/1.873855 |
Popis: | A self-consistent numerical model of self-generation and amplification of magnetic fields in weakly ionized protogalactic matter is presented. This model is based on three-dimensional two-fluid simulations of the dynamics expected for protogalactic plasma–neutral gas clouds characterized by shear flow. Due to the friction between the ionized and neutral gas components self-generated magnetic fields of seed field order, i.e., 10−17 G are created on time scales of 105 yr. Moreover, unstable Kelvin–Helmholtz modes are excited yielding a significant amplification of the field. |
Databáze: | OpenAIRE |
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