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. 2017 Apr 24;44(8):3456–3464. doi: 10.1002/2017GL073048

Figure 3.

Figure 3

(first to third rows) MMS wave magnetic field in field‐aligned (μ), poloidal (ν), and toroidal (φ) directions. The three horizontal bars indicate the time intervals selected for estimating the azimuthal wavenumbers. (fourth row) The observed time lags in b ν versus longitudinal separations between MMS satellites.