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A Flux Rope Network and Particle Acceleration in Three-dimensional Relativistic Magnetic Reconnection

  • Authors: Daniel Kagan, Miloš Milosavljević, and Anatoly Spitkovsky

Kagan, Milosavljević, & Spitkovsky 2013 The Astrophysical Journal 774 41.

  • Provider: AAS Journals

Caption: Figure 1.

The total current density J ≡ | J| (left two columns) and total particle density n (right two columns) in a slice y = 5 λ p. In each pair of columns, the first column shows times t = (37.5, 47, 56, 65.5, 75) τ c0 and the second column shows t = (84.5, 94, 103, 112.5, 122) τ c0 . The particle density n, which is not used directly in the PIC code, is calculated from particle positions using a uniform kernel of half-width two grid lengths. The same kernel is used to smooth the current density J.

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