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Parady, B.

Publications and source records attributed to Parady, B..

Observations of ULF electric field fluctuations in the dayside auroral oval

Electric field oscillations at frequencies centered below 10 Hz were measured by a payload equipped with double-probe electric field detectors which was launched into the dayside auroral oval during the Greenland rocket campaign on January 11, 1975. These oscillations exceeded an amplitude of 3 mV/m broadband and occurred over a period of about 90 s. These oscillations occurred during a proton injection event when the quasi-static electric field was less than 20 mV/m on the average. However, during a brief 2-s interval the electric field exceeded 50 mV/m. Analysis of the amplitude as a function of the spin frequency showed that the electric field was confined to a plane perpendicular to the magnetic field. The power spectrum was of the form f to the -6.5 + or - 1.5 power, where f is the frequency over the range from 8 to 18 Hz. The existence of a large electric field fluctuation in a spatially or temporally confined region of low-amplitude turbulence suggests that this may be an observation of the low-altitude projection of a turbulent region associated with electrostatic shocks which have recently been observed at higher altitudes.

Temerin, M.↗

ELF observations during the December 1971 storm.

Initial results from the University of Minnesota search coil magnetometers aboard the Explorer 45 Satellite show several types of ELF signals during the magnetic storms of Dec. 16-19, 1971. The orbit of the satellite at this time was nearly equatorial, with an apogee near 5 earth radii at 2100 local time, and a perigee below 300 km. The emissions vary during different phases of the storms and also with the position of the spacecraft in the magnetosphere. The location of the plasmapause appears to be a particularly important factor in determining the type and intensity of the signals.

Parady, B.↗