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- W1971460817 abstract "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." @default.
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- W1971460817 date "2000-02-01" @default.
- W1971460817 modified "2023-09-26" @default.
- W1971460817 title "The origin of primeval magnetic fields: Self-consistent simulation of magnetic field generation and amplification" @default.
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- W1971460817 doi "https://doi.org/10.1063/1.873855" @default.
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