The time evolution of plasma parameters (density, magnetic field, etc.) in a two-dimensional MHD model of solar flare reconnection is computed numerically.
The time evolution of plasma parameters (density, magnetic field, etc.) in a two-dimensional MHD model of solar flare reconnection is computed numerically. (en)
Byla prezentována radiová vzplanutí, která mohou být generována v magnetické rekonexi ve slunečních erupcích. (cs)