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. Author manuscript; available in PMC: 2019 Feb 20.
Published in final edited form as: Phys Plasmas. 2018 Feb 20;25(2):022303. doi: 10.1063/1.5009158

Figure 2.

Figure 2.

(a) The direction and (b) magnitude of wave vectors (k) determined by the J×B method as a function of frequency in the spacecraft frame in GSE coordinates. Data were averaged over all four MMS observatories. Here, kkk॥.k varies as ωsc and ωsc0.47±0.10 for fsc below and above 4 Hz, respectively.