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Particle reacceleration by compressible turbulence in galaxy clusters: effects of reduced mean free path
acceleration of particles - turbulence - radiation mechanisms non{thermal - galaxies clusters general radio continuum general - X{rays general
2010/11/11
Direct evidence for in situ particle acceleration mechanisms in the inter-galactic-medium (IGM) is provided by the di use Mpc{scale synchrotron emissions observed from galaxy clusters.
Reduced description of light impurities in hydrogen coronal plasmas
hydrogen coronal plasmas light impurities
2009/6/4
Reduced description of light impurities in hydrogen coronal plasmas。
On the reduced mhd for compressible fluids。