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Earth, Planets and Space
Fig. 1 | Earth, Planets and Space

Fig. 1

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

Fig. 1

Field of view of the Hokkaido, Tiger, and Unwin radars, the footprints of the THEMIS A, D, and E satellites at an altitude of 100 km, and geomagnetic stations at 09:12 UT on August 19, 2010. Shaded regions of the field of view indicate locations of echoes with Pi2 frequencies. Satellite footprints were calculated by using the T96 geomagnetic field model

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