Image Details

Choose export citation format:

Particle Acceleration by Magnetic Reconnection in Relativistic Jets: The Transition from Small to Large Scales

  • Authors: Tania E. Medina-Torrejón, Elisabete M. de Gouveia Dal Pino, Grzegorz Kowal

Tania E. Medina-Torrejón et al 2023 The Astrophysical Journal 952 .

  • Provider: AAS Journals

Caption: Figure 1.

A 3D view of the σ ∼ 1 jet evolved with the MHD-PIC mode at t = 20 (top), and 45 L/c (bottom). Left panels: the black lines represent the magnetic field, and the circles the 50,000 particle distribution. The color and size of the circles indicate the value of their kinetic energy normalized by the rest mass energy (γ p − 1). Right panels: the orange color represents isosurfaces of half of the maximum of the current density intensity ∣J∣, the black lines the magnetic field, and the green squares correspond to the positions of the fastest magnetic reconnection events, with reconnection rate ≥0.05. See the text for more details.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse