Figure 2From: Origin of the filamentary structure in space plasmasMagnetic energy spectrum E ( k ⊥ , ω ) averaged over the spatial coordinates parallel to the large-scale magnetic field for two simulation boxes at an earlier evolution time (200 ion gyroperiods, t Ω p =200). The wave modes are marked by IB1 (ion Bernstein ω/Ω p = 1), IB2 (ion Bernstein ω/Ω p = 2), IC (ion cyclotron), and W (whistlers).Back to article page