The time structure of solar X-ray bursts above 7.7 kev.
Time structure of solar X ray bursts from OSO 3 satellite observations showing impulsive and gradual components
Engineering topics
Publications and source records attributed to Peterson, L. E..
Time structure of solar X ray bursts from OSO 3 satellite observations showing impulsive and gradual components
Description and operations of Environmental Research Satellite-18
Balloon results on Crab nebula spectrum and time stability and X ray objects in Cygnus region
Hard solar and cosmic X rays observed by OSO 3, noting Lupus XR-1 and galaxy M 87 sources
Crab Nebula and Cygnus XR-1 X ray spectra shown to have differential number power law spectra and same intensity
Instrumental and observational aspects of balloon X-ray astronomy involving position, angular size, intensity and spectral measurements of X-ray sources
Cosmic and solar X ray data obtained by Orbiting Solar Observatory /OSO-3/
Ionizing radiation effects on dark current and noise pulse spectrum of photomultiplier tubes used in balloon and satellite X-ray observations
Balloon observation of upper limits of solar gamma rays for spectral ranges 20-200 kev and 1-10 mev
Instrumental and observational aspects of balloon X-ray astronomy involving position, angular size, intensity and spectral measurements of X-ray sources
Upper limits resulting from search for solar photons in 100-kev to 2-mev range from balloon observations
Exponential spectrum of Scorpius XR-1 to 50 kev observed by balloon
Balloon flight data on upper limit solar gamma ray spectrum from quiet sun
Balloon telescopic measurements of strongest X-ray source in Scorpius
Crab Nebula X-ray spectrum from 16-120 kev by balloon
Upper limits on cosmic gamma ray flux obtained using OSO-I and sodium iodide scintillation counters
Upper limits on cosmic gamma ray flux obtained using OSO-I and sodium iodide scintillation counters
Radioactivity induced in sodium iodide by trapped protons during OSO-1 passage through lower edge of inner Van Allen zone, presenting gamma-ray counting rates