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Official Journal of the Asia Oceania Geosciences Society (AOGS)

Figure 2 | Geoscience Letters

Figure 2

From: Origin of the filamentary structure in space plasmas

Figure 2

Magnetic 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).

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