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Kenji OHYA Hiroyuki EGUCHI Masashi HAYAKAWA Yoshihito TANAKA
An analogue equipment is developed and described, which can automatically identify and track the magnetospheric whistler signal so that we can measure the amplitude ratio and phase difference between two horizontal magnetic field components of each whistler over a wide frequency range (6 to 3 kHz) and then we can study the ionospheric transmission characteristics of whistlers.