Volume 422, Number 1, July IV 2004
|Page(s)||23 - 27|
|Section||Cosmology (including clusters of galaxies)|
|Published online||06 July 2004|
Magnetic amplification in cylindrical cosmological structure
Astronomical Observatory, Jagellonian University, Faculty of Physics, Astronomy and Applied Computer Science, ul. Orla 171, 30–244 Kraków, Poland
Corresponding author: G. Siemieniec-Oziębło, email@example.com
Accepted: 1 April 2004
We derive the amplification of the cosmological magnetic field associated with forming gravitational structure. The self-similar solutions of magnetohydrodynamic equations are computed both in linear and nonlinear regimes. We find that the relatively fast magnetic field enhancement becomes substantial in the nonlinear phase.
Key words: cosmology: theory / cosmology: miscellaneous
© ESO, 2004
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