Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988afz....28..111b&link_type=abstract
Astrofizika, Vol.28:1, P. 111, 1988
Astronomy and Astrophysics
Astronomy
1
Scientific paper
It has been shown that the possibility of generation of the MHD turbulence by collisionless shocks in consequence of anisotropy of pressure behind the front of a reverse shock in the hot spot of powerful radio galaxies takes place. The energy density of MHD turbulence has been estimated. The analysis of theoretical and experimental data on collisionless shocks in solar wind shows the important role of reflection ion streams which generate plasma and MHD turbulence in the region before a shock front. Transfer of this idea on shocks in powerful radiogalaxies should be carefully made because of strong difference of parameters of these shocks from the parameters of shocks of the solar wind.
Baryshev Yuriy V.
Morozov V. N.
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