... For the first time we obtain strong explosion for the core collapsed supernova. ... rotation leads to the formation of MHD shockwave, which produces supernova explosion ...
... Numerical simulations of the bounce shock and neutrino driven supernova mechanisms either do not lead to the explosion or the explosion energy is too small. ...
... CR acceleration (generation) at the shocks, produced by supernova explosions, and the properties of nonthermal emission generated by CRs accelerated in supernova remnants are detaily discussed. ...
... repentinos en la intensidad de radiaci n, asociados con explosiones en el Sol, la mayor a con fulguraciones visibles ... fen menos de aceleraci n solar son acompa ados a menudo por explosiones de rayos X, que alcanzan a veces su intensidad pico en ...
... explosion power movie 1: Model A: inner region , R<1000 km radius; colour image - log(), g/cm3 movie 2: Model A: inner region, R<1000 km radius; lines and colour poloidal magnetic field lines Model A, t=0.2s unit length=2km log10 density (g/cm3); vp/c ...
... first time the magnetorotational supernova explosion was simulated numerically in 2D ... Explosion energy is (0.5-0.6 10^{51}erg) what is enough for the explanation of the ...