How do recollimation-induced instabilities shape the propagation of hydrodynamic relativistic jets?

Open Access

Fig. 6.

Spatial component of the velocity, $β = \sqrt{β_{r}^{2} + β_{z}^{2}}$ $\beta= \sqrt{\beta_r^2+\beta_z^2}$ (top), and the radial component β_r (bottom) at the end of the SHC05 2D simulation, and start of the 3D one. There are superimposed the values of angular velocity at the discontinuity, normalized to the maximum: ${\tilde{Ω}}_{c}$ $\tilde{\Omega}_{\text{c}}$ .

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.