<i>In situ</i>generation of coronal Alfvén waves by jets
<i>In situ</i>generation of coronal Alfvén waves by jets
Within the framework of 3D resistive magnetohydrodynamic, we simulate the formation of a plasma jet with the morphology, upward velocity up to 130 km s−1, and time-scale formation between 60 and 90 s after beginning of simulation, similar to those expected for type II spicules. Initial results of this simulation …