Upper limits of the cosmic gamma-ray flux from oso-1.
Upper limits on cosmic gamma ray flux obtained using OSO-I and sodium iodide scintillation counters
OSO-1↗
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Contributions of the University of Minnesota to the Ninth International Conference on Cosmic Rays
Cosmic ray conference - intensity and energy spectra of particles in primary cosmic radiation, solar modulation, and measurements using Cerenkov scintillation counter
CONFERENCE↗
Low-energy electrons in the dark magnetosphere.
Scintillation counter satellite data on low energy electron flux and particle trapping in dark magnetosphere
GEOMAGNETIC LATITUDE↗
Upper limits of the cosmic gamma-ray flux from OSO-1.
Upper limits on cosmic gamma ray flux obtained using OSO-I and sodium iodide scintillation counters
COSMIC RAY PROPAGATION↗
Experiment data analysis report. OGO-A experiment no. 1
OGO-A scintillation counter to detect 3 to 90 MeV protons in solar cosmic rays
Anderson, K. A.↗
Temporal variations of the 100 keV trapped protons observed on satellite Explorer 26 during first half of 1965
Temporal variations of 100 keV to 1700 keV trapped protons from data recorded by scintillation counter on Explorer 26 - Jan. 29, 1965 - June 29, 1965
Davis, L. R.↗
High-energy X-rays from Cygnus XR-1.
High energy X rays from Cygnus XR-1, Cassiopeia A and SN 1572 measured by balloon- borne scintillation counter
Overbeck, J. W.↗
Measurements of the low-energy cosmic radiation during the summer of 1966.
Isotopic composition of hydrogen and helium nuclei in low energy cosmic rays based on scintillation counter telescope data during balloon flights
Badhwar, G. D.↗
Recent development in organic scintillators
Discussion on recent developments of organic scintillators includes studies of organic compounds that form glass-like masses which scintillate and are stable at room temperature, correlations between molecular structure of organic scintillators and self-quenching, recently developed fast scintillators, and applications of liquid-scintillation counters.
Horrocks, D. L.↗
Improved sterilizable multiplier phototubes Final report
Development of sterilizable multiplier phototube for scintillation counter
Dumas, E. J.↗
Response of the ion-electron detector flown on Explorer 12, August to December 1961
Graphs depicting output of ion-electron scintillation counter flown on Explorer 12 satellite - August - December 1961
Davis, L. R.↗
The hard solar X-ray spectrum observed from the third orbiting solar observatory.
Solar X-ray events observed by scintillation counter telescope on OSO 3 satellite, discussing X ray spectra during burst initial and decay phases
Hudson, H. S.↗
A proton spectrometer for NASA's Apollo applications program
Particle spectrometer for Apollo measurements of trapped protons and electrons, using directional telescope composed of solid state and scintillation counters
Guenther, G. A.↗
Search for charge 1/3e and 2/3e quarks in cosmic radiation near sea level
Quark search in cosmic radiation near sea level, using scintillation counter telescope
Bowen, T.↗
A versatile pulse amplifier
Versatile pulse amplifier for use with scintillation counters, surface barrier detectors, proportional counters or channel electron multipliers
Lampton, M.↗
Techniques in balloon X-ray astronomy
Balloon X ray astronomy techniques and observations, noting collimated scintillation counter instrumentation and PCM telemetry
Matteson, J. L.↗
An experiment to study the nuclear component of primary cosmic rays
An apparatus has been designed and is being fabricated to study the charge composition, fluxes, and energy spectra of light nuclei in the energy region from 1 GeV to 100 GeV. The apparatus essentially consists of an array of a large number of particle detectors operated in coincidence and serving as a charged particle telescope. A mosaic silicon semiconductor detector, a plastic scintillation counter and a lucite Cerenkov detector are used to measure the charges of the incident nuclei. Two one-inch thick CsI detectors are used to study low energy particles. An ionization spectrometer is utilized to measure primary energies in the 1 to 100 GeV energy interval. A gas Cerenkov counter is being designed to distinguish between electrons and protons. It is planned to calibrate the apparatus at an accelerator using particles of known energy.
Paul, J. M.↗
Comparison of the energy response of an ionization spectrometer for pions and protons
An ionization spectrometer consisting of a sandwich of iron absorbers and plastic scintillation counters was used to measure the energy of pions and protons in the interval 10 to 1000 GeV. For the limited energy interval of 10 to 40 GeV, pions and protons were identified by an air cerenkov counter. Interactions in carbon were studied in a multiplate cloud chamber placed between the cerenkov counter and the spectrometer. Knowledge of these interactions were used in conjunction with a Monte Carlo simulation of the cascade process to study differences in the response of the spectrometer to pions and protons.
Jones, W. V.↗