Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004jkas...37..547o&link_type=abstract
Journal of the Korean Astronomical Society, vol. 37, no. 5, pp. 547-551
Astronomy and Astrophysics
Astronomy
Clusters Of Galaxies, Magnetic Fields, Instabilities, Plasmas
Scientific paper
We showed that magnetic fields are generated in the plasma which have the temperature inhomogeneities. The mechanism is the same as the Weibel instability because the velocity distribution functions are at non-equilibrium and anisotropic under the temperature gradients. The growth timescale is much shorter than the dynamical time of structure formation. The coherence length of magnetic fields at the saturated time is much shorter than kpc scale and then, at nonlinear phase, become longer by inverse-cascade process. We report the application of our results to clusters of galaxies, not including hydrodynamic effects.
Hattori Makoto
Okabe Nobuhiro
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