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. 2021 Jun 21;126(6):e2021JA029117. doi: 10.1029/2021JA029117

Figure 4.

Figure 4

(a–e) In situ plasma density (at ∼845 km altitude), cross‐track velocity (positive values indicating westward flows), the magnetic field perturbations (an increase in the azimuthal direction toward higher latitudes indicating downward field‐aligned currents), and the energy spectrum of the precipitating electrons and ions measured by DMSP F17. (f–j) Similar to (a–e) but showing measurements of F16.