Characteristics of effect of different types of radiation on the higher nervous activity of small animals, III
Comparative effects of fast neutrons, protons, and gamma radiation on higher nervous activity of August rats
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Comparative effects of fast neutrons, protons, and gamma radiation on higher nervous activity of August rats
Average cross sections for nuclear reaction for gamma radiation spectrum of fission products
Gamma radiation exposure and weightlessness effects compared for biological material during Biosatelle 2 flight and in earth control capsule, noting radiation sources
A study of the gamma-radiation produced by the interaction of cosmic rays with the interstellar matter and photons is extended, based on recent COS-B satellite results and background estimates (1982) and evaluations of the 21-cm radiation in the Galaxy. Gamma-ray intensities predicted over the latitude range of -10 to 10 degrees for energy ranges 70-150, 150-300, and 300-5000 MeV agree well with the COS-B longitude distributions. The agreement suggests that the radial distribution of the emission, calculated from the model, is also approximately correct. The energy spectrum is calculated using COS-B and SAS-2 data. Finally, it is noted that contribution by the arms on the far side of the Galaxy for small galactic latitudes (between -0.4 and +0.4 degrees) makes it possible to identify very large far-side molecular clouds.
Very small, individual polymeric microspheres with very precise size and a wide variation in monomer type and properties are produced by deploying a precisely formed liquid monomer droplet, suitably an acrylic compound such as hydroxyethyl methacrylate into a containerless environment. The droplet which assumes a spheroid shape is subjected to polymerizing radiation such as ultraviolet or gamma radiation as it travels through the environment. Polymeric microspheres having precise diameters varying no more than plus or minus 5 percent from an average size are recovered. Many types of fillers including magnetic fillers may be dispersed in the liquid droplet.
Gamma radiation effects on polyethylene terephthalate
X-ray and gamma radiation astronomy - OSO MEASUREMENTS
Instability, high threshold voltage, and gamma radiation in MOS transistors
Buildup dose factors with inclined incident gamma radiations, for radiation shielding design
Spectral energy and angular distributions of gamma radiation through single and double layered shielding barriers
Gamma radiation tests on n-p-n silicon epitaxial transistors
The effects of 1.2 MeV gamma radiation and 20 MeV electrons on the operational characteristics of CCDs are studied. The effects of ionizing radiation on the charge transfer efficiency, dark current, and input/output circuitry are described. The improved radiation hardness of buried channel CCDs is compared to surface channel results. Both ion implanted and epitaxial layer buried channel device results are included. The advantages of using a single thickness SiO2 gate dielectric are described. The threshold voltage shifts and surface state density changes of dry, steam, and HCl doped oxides are discussed. Recent results on the recovery times and total dose effects of high dose rate pulses of 20 MeV electrons are reported.
Mechanisms of solar gamma radiation production - prediction of fluxes at earth
Instability, high threshold voltage and gamma radiation sensitivity of metal-oxide-silicon transistors
Causes of instability, high threshold voltage, and gamma radiation sensitivity of metal-oxide silicon transistors
Observations of cosmic and gamma radiation by SAS-2 satellite are summarized and analyzed to determine processes responsible for producing observed galactic radiation. In addition to the production of gamma rays in discrete galactic objects such as pulsars, there are three main mechanisms by which high-energy (greater than 100 MeV) radiation is produced by high-energy interactions involving cosmic rays in interstellar space. These processes, which produce what may be called diffuse galactic gamma-rays, are: (1) the decay of pi mesons produced by interactions of cosmic ray nucleons with interstellar gas nuclei; (2) the bremsstrahlung radiation produced by cosmic ray electrons interacting in the Coulomb fields of nuclei of interstellar gas atoms; and (3) Compton interactions between cosmic ray electrons and low-energy photons in interstellar space.
Thermal conductivity cell measurements of depolymerization rate of polytetrafluoroethylene exposed to gamma radiation in flowing helium atmosphere
Measurements of primary cosmic radiation gamma quanta from Proton I and II satellites