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A Comprehensive Comparison of Relativistic Particle Integrators

  • Authors: B. Ripperda, F. Bacchini, J. Teunissen, C. Xia, O. Porth, L. Sironi, G. Lapenta, and R. Keppens

2018 The Astrophysical Journal Supplement Series 235 21.

  • Provider: AAS Journals

Caption: Figure 16.

Distance between the predicted position at t = 30 with the Boris method and the GCA for the magnetic null case. The distance is shown as a function of the particles’ initial ϕ angle on the circle ﹩{x}^{2}+{y}^{2}=1﹩. Particles close to the diagonals (at ﹩\phi \approx \pi /4,3\pi /4,5\pi /4,7\pi /4﹩) move toward the magnetic null, where the GCA breaks down.

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