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Fig. 7 | Earth, Planets and Space

Fig. 7

From: Latitudinal dependence on the frequency of Pi2 pulsations near the plasmapause using THEMIS satellites and Asian-Oceanian SuperDARN radars

Fig. 7

Time series of Doppler velocities from a beam 14 at ranges 3–5 and 14–22 for UNW, b beam 4 at the range 13–27 for TIG, and c beam 4 at ranges 21–29 and 52–57 for HOK in the upper panels, and the magnetic field data in the dH component at a and b MCQ and c PTK in the bottom panels. The arrows indicated the locations of the plasmasphere

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