The Ogo 1 triaxial search coil magnetometer was designed to study natural magnetic fluctuations from 0.01 to 1000 cps in the vicinity of the earth. This frequency range was chosen in order to explore the magnetic spectrum between the ranges previously explored in space by dc magnetometers and extremely low frequency electromagnetic equipment. The highly eccentric Ogo 1 orbit makes possible an investigation of time-varying magnetic fields in the magnetosphere, the magnetosheath (transition region), and the interplanetary medium. The preliminary analysis of the data reported here concerns: (1) the character and location of the magnetopause and hydromagnetic bow shock over portions of the subsolar hemisphere, and (2) the characteristics of broad band magnetic noise detected in the magnetosheath behind the bow shock.
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