The cosmic gamma-ray spectrum near 1 MeV observed by the ERS-18 satellite
Omnidirectional cosmic gamma ray flux near one MeV observed by ERS-18 satellite, plotting spectral energy distribution
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Omnidirectional cosmic gamma ray flux near one MeV observed by ERS-18 satellite, plotting spectral energy distribution
Differential elastic cross sections of 42 MeV alpha particles scattering from He 3, using optical model with spin-orbit potential
Optical absorption in transparent materials during 1.5 MeV electron irradiation
Scattering of 42-MeV alpha particles from Sc-45
Neutron spectra calculations from proton-nucleus inelastic collisions for 15 to 18 MeV protons
Origin and isotropy of cosmic gamma ray flux between 1 and 6 MeV and its implications of future gamma ray investigations
Microwave cavity systems engineering for MeV electron beam ionization measurements
Galactic and extragalactic origin of cosmic gamma ray flux between 1 and 6 MeV
Angular distributions for /alpha,t/ reactions on Zr-90, Mo-92 and 96 at 41.5 MeV
Tilt angle dependence of 10 MeV proton cutoff lattitudes in image dipole model magnetosphere
Comparison of 1.5 MeV electron irradiation induced optical absorption of fused commercial silicas and optical transmission of Al2O3, MgF2, BaF2, LiF, and BeO
Interplanetary space He 3 differential energy spectrum in 10-30 MeV range from IMP 4 satellite observations, noting solar contributions
Production and annealing of defects in lithium diffused bulk silicon after irradiation with 30 MeV electrons and fission neutrons at 300 K
Solar flare electrons at 10-200 MeV region, discussing energy spectra and time history
Pulsating gamma ray flux from pulsar NP 0532 in energy range from 250 keV to 2.3 MeV
The extended particle-core coupling model was used to predict the properties of low-lying levels of Cu-65. A 42-MeV alpha particle cyclotron beam was used for the experiment. The experiment included magnetic analysis of the incident beam and particle detection by lithium-drifted silicon semiconductors. Angular distributions were measured for 10 to 50 degrees in the center of mass system. Data was reduced by fitting the peaks with a skewed Gaussian function using a least squares computer program with a linear background search. The energy calibration of each system was done by pulsar, and the excitation energies are accurate to + or - 25 keV. The simple weak coupling model cannot account for the experimentally observed quantities of the low-lying levels of Cu-65. The extended particle-core calculation showed that the coupling is not weak and that considerable configuration mixing of the low-lying states results.
The effects of 22-MeV protons on various types of silicon single junction and silicon controlled rectifiers were investigated. The results show that low-leakage devices and silicon controlled rectifiers are the most susceptable to radiation damage. There are also differences noted between single junction rectifiers of the same type made by different manufacturers, which emphasizes the need for better selection of devices used in spacecraft.
An experimental determination of the optical transmission of Corning 7940 UV and Suprasil 1 and 2 fused silica has been made during 1.5-MeV electron bombardment. The fused silica reached temperatures ranging from 150 to 1000 C. The Lewis Research Center dynamitron provided electron current densities which corresponded to a dose rate of 2.6 to 20 Mrad/sec. The irradiation induced absorption was measured at 215.0, 270.0, and 450.0 nm (2150, 2700, 4500 A). The length of each irradiation was sufficient so that an equilibrium between radiation induced coloration and high temperature annealing was reached. The experimental results indicate a significant optical absorption, with values of the induced absorption coefficient at 215.0 nm (2150 A) of 14.5 to 2.2/cm, at 270.0 nm (2700 A) of 9.7 to 3.0/cm and at 450.0 nm (4500 A) of 3.7 to 0.5/cm. This would make the use of fused silica as the separating wall material in the nuclear light bulb propulsion concept questionable.