Figure 3 from KINETIC SIMULATIONS OF THE LOWEST-ORDER UNSTABLE MODE OF RELATIVISTIC MAGNETOSTATIC EQUILIBRIA

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF

KINETIC SIMULATIONS OF THE LOWEST-ORDER UNSTABLE MODE OF RELATIVISTIC MAGNETOSTATIC EQUILIBRIA

Authors: Krzysztof Nalewajko, Jonathan Zrake, Yajie Yuan, William E. East, and Roger D. Blandford

2016 The Astrophysical Journal 826 115.

Provider: AAS Journals

Caption: Figure 3.

Linear instability growth rate, defined as e-folding timescale of the total electric energy normalized to L/c, as a function of the mean value of the hot magnetization. The point size indicates the simulation domain size L. The blue arrow indicates the asymptotic value measured in FF simulations (East et al. 2015).

Other Images in This Article

Copyright and Terms & Conditions