Figure 9 from

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 9.

Probability density functions of ΔW_c and ΔW_⊥, normalized to the particle energy γ₀m_ic², accumulated over Δt = 0.5 l_c/c starting at t₀ = 2 l_c/c (γ₀ is the particle Lorentz factor at t₀) in the reference simulation. Different colors correspond to three distinct ranges of γ₀.

Copyright and Terms & Conditions

Additional terms of reuse

Other Images in This Article

Copyright and Terms & Conditions