Observations of the solar proton event of August 28, 1966.
August 28, 1966 Solar Proton Event observed with CsI scintillator telescope aboard IMP 3 compared to other large proton events
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August 28, 1966 Solar Proton Event observed with CsI scintillator telescope aboard IMP 3 compared to other large proton events
Gravitational fields effects on light intensity related to detectability of gravitational waves by starlight scintillation measurement
Primary cosmic ray energy spectra and charge composition during 1965 solar modulation minimum, using scintillator photomultiplier detector on OGO 1
Primary cosmic ray proton and He energy spectra and solar modulation effects during sunspot minimum from balloon-borne scintillation counter telescope data
Counter telescope consisting of plastic scintillators and NaI crystal to determine charge, mass and energy of low energy cosmic rays
Pulsar CP 1919 observed simultaneously at Arecibo and Stanford, discussing interstellar scintillation as possible explanation for amplitude variations
Pulsed neutron source operates in conjunction with a photomultiplier tube coupled to a gamma ray scintillation crystal. This allows measurements of gamma radiation from both inelastic scattering and thermal neutron capture in a single experiment.
Multipurpose digital delay timer simultaneously controls both a buffer pump and a fraction-collector. Timing and control may be in 30-second increments for up to 15 hours. Use of glassware and scintillation vials make it economical.
Spaced receiver method for measuring height variations in scintillating radio signals from artificial satellites
Variable energy gamma ray production, neutron sources, and scintillation dosimeters
Development of sterilizable multiplier phototube for scintillation counter
Graphs depicting output of ion-electron scintillation counter flown on Explorer 12 satellite - August - December 1961
Satellite observations of aberrations of radio signals traversing auroral ionosphere indicating decreasing trend in scintillation activity
Differential energy spectrum of protons and helium nuclei using lithium drifted silicon detectors and scintillator-Cerenkov counter
Log amplitude variance calculation methods compared in statistics of optical scintillation by application to measurements with laser
Optical communications experiments for quantitative data at 6328 A on system fading due to scintillation and atmospheric turbulence effects on coherent propagation at 10.6 micron
Low level beta, X and gamma radiation detector incorporating Geiger, proportional and scintillation counting features in various modes suiting radionuclide decay scheme
Solar X-ray events observed by scintillation counter telescope on OSO 3 satellite, discussing X ray spectra during burst initial and decay phases