OGO-3 observations of ELF noise in the magnetosphere - Part 1 - Spatial extent and frequency of occurrence
OGO-3 spectrum analyzer measurements of magnetic noise in magnetosphere
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OGO-3 spectrum analyzer measurements of magnetic noise in magnetosphere
Low energy electrons in magnetosphere from OGO-1 and OGO-3 observations, discussing plasma sheet, magnetic bay activity, electron pressure, temperature and density gradient
OGO-1 and OGO-3 VLF emission records of magnetospheric electromagnetic noise
Samples of electron spectroscopy and ionization chamber data plots from OGO-1 and OGO-3
Low energy electrons in magnetosphere as observed by OGO satellites
Data plots obtained from ion chamber and electron spectrometer experiments aboard OGO A and OGO C satellites
Direct measurement of thermal ion distributions in magnetosphere to determine position and structure of plasmapause
Plasma proton and plasma electron prototype and flight models were designed, fabricated, and tested. Ground support equipment for the models was also prepared. The flight models were launched aboard the first and third Orbiting Geophysical Observatories on 4 Sept. 1964 and 6 June 1966. These experiments have generally functioned in accordance with the design specifications and useful data are still being received.
An oscillation in the OGO-3 roll control channel, resulting from the EP-5 and EP-6 boom motion coupling into the control channel and causing loss of attitude control, is investigated. The study includes (1) an analysis of the OGO-3 and OGO-2 flight data to determine the nature and extent of the roll oscillation phenomena, (2) design analysis of the complete attitude control subsystem (ACS) to evolve changes which would prevent recurrences of the coupled ACS boom oscillation observed on OGO-3, and (3) analog simulations to verify the performance of the design changes selected. Portions of OGO-3 and OGO-2 flight data are illustrated and the major flexible body oscillation are identified. A model of the major flexible appendage dynamics is developed and is shown analytically and through analog simulations to reproduce the OGO-3 oscillation phenomena. The design changes which were found necessary are: a reversal delay logic for the roll reaction wheels, widening of the solar array dead zone from 0.5 to 1.0 deg, and modification of the OPEP control loop to include a filter and stabilizing feedback loops.
Differential energy spectra of low energy protons and positive ions in earth inner radiation zone, using electrostatic analyzers aboard OGO-3 satellite
OGO-3 and ATS-1 data used in experimental verification of drift shell splitting in distorted magnetosphere
OGO-3 and ATS-1 measurements of intensity correlations and substorm electron drift effects in outer radiation belt
Atlas of energetic solar flare X rays and tentative atlas of proton events observed by OGO-1 and OGO-3 ionization chambers
Data collected by OGO-3 in detecting solar bursts
Electron energy density between inner edge of plasma sheet and plasmasphere measured by OGO-3 electrostatic analyzer
Dynamic spectra of type 3 solar bursts from OGO-3 antenna/radiometer observations
Electron densities between inner edge plasma sheet and plasmasphere as function of geocentric radial distance from OGO-3 electrostatic measurements
Quiet time fluxes and differential energy spectra of protons and alpha particles at 2-20 MeV measured by cosmic ray detectors on OGO-3