The collision between pairs of quasi-parallel shocks is examined using hybrid numerical simulations. In the interaction, the two shocks are transmitted through each other leaving behind a hot plasma with a population of particles with energies in excess of 40 E0, where E0 is the kinetic energy of particles in the shock frame prior to the collision. The energization is more efficient for quasi-parallel shocks than parallel shocks. Collisions between shocks of equal strengths are more efficient than those that are unequal. The results are of importance for phenomena during the impulsive phase of solar flares, in the distant solar wind and at planetary bow shocks.
Collisions between quasi-parallel shocks
Advances in Space Research ; 11 , 9 19
1991-01-01
Sonstige
Keine Angabe
Englisch
Collisions between quasi-parallel shocks
Elsevier | 1991
|NTRS | 1986
|Elsevier | 1986
|The formation of quasi-parallel shocks
Elsevier | 1991
|The formation of quasi-parallel shocks
NTRS | 1991
|