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Magnetic Field-line Curvature and Its Role in Particle Acceleration by Magnetically Dominated Turbulence

  • Authors: Samuel T. Sebastian, Luca Comisso

Samuel T. Sebastian and Luca Comisso 2025 The Astrophysical Journal Letters 994 .

  • Provider: AAS Journals

Caption: Figure 8.

Example trajectory of a proton from the reference simulation (δB0/B0 = 1). The top panel shows the trajectory color-coded by the particle Lorentz factor γ. The bottom panel shows the same trajectory color-coded by the magnetic field-line contraction (vE · κ)lc/c at the particle location. The trajectory is plotted over a duration of 4 lc/c.

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