Scattering of 42-MeV /6.7-pJ/ alpha particles from even isotopes of cadmium
Scattering of 42 MeV alpha particles from even cadmium isotopes
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Scattering of 42 MeV alpha particles from even cadmium isotopes
Differential elastic cross sections of 42 MeV alpha particles scattering from He 3, using optical model with spin-orbit potential
Biological effect of high energy protons and alpha particles on small animals - radiation effects
The ability to evaluate the cosmic ray environment at Mars is of interest for future manned exploration. To support exploration, tools must be developed to accurately access the radiation environment in both free space and on planetary surfaces. The primary tool NASA uses to quantify radiation exposure behind shielding materials is the space radiation transport code, HZETRN. In order to build confidence in HZETRN, code benchmarking against Monte Carlo radiation transport codes is often used. This work compares the dose calculations at Mars by HZETRN and the Geant4 application Planetocosmics. The dose at ground and the energy deposited in the atmosphere by galactic cosmic ray protons and alpha particles has been calculated for the Curiosity landing conditions. In addition, this work has considered Solar Energetic Particle events, allowing for the comparison of varying input radiation environments. The results for protons and alpha particles show very good agreement between HZETRN and Planetocosmics.
Satellite observation of alpha particles trapped geomagnetically in radiation belts, including Injun 5 results
Apollo 11 lunar rock samples alpha particle activity in polished thin sections, using audioradiography and electron microprobe
Superconducting effects on alpha particle differential energy loss in tin, vanadium, and lead superconductors
The importance of Cosmic Rays on the performance of integrated circuits (IC's) in a space environment is evident in the upset rate of the Tracking and Data Relay Satellite (TDRS) launched in Apr. 1983. This satellite experiences a single-event-upset (SEU) per day which must be corrected from the ground. Such experience caused a redesign of the Galileo spacecraft with SEU resistant IC's. The solution to the SEU problem continues to be important as the complexity of spacecraft grows, the feature size of IC's decreases, and as space systems are designed with circuits fabricated at non-radiation hardened foundries. This paper describes an approach for verifying the susceptibility of CMOS latches to heavy-ion induced state changes. The approach utilizes alpha particles to induce the upsets in test circuits. These test circuits are standard cells that have offset voltages which sensitize the circuits to upsets. These results are then used to calculate the upsetability at operating voltages. In this study results are presented for the alpha particle upset of a six-transistor static random access memory (SRAM) cell. Then a methodology is described for the analysis of a standard-cell inverter latch.
Energy spectrum of primary cosmic ray alpha particles measured by nuclear photographic emulsion, estimating geomagnetic cut-off energies
Proton and alpha particle effects on thermal properties of spacecraft and solar concentrator coating of anodic-coated aluminum, zinc oxide/ potassium silicate, etc
Proton and alpha particle effects on thermal properties of spacecraft and solar concentrator coatings of anodic-coated aluminum, zinc oxide/ potassium silicate, etc
Ag, In and Sb core excitations caused by inelastic scattering of alpha particles
Differential energy losses of alpha particles traversing materials in superconducting and normal states
Temporal intensity variations of geomagnetically trapped solar alpha particles from Injun 5 observations
An alpha particle experiment similar to the one performed successfully on the Surveyor lunar missions is described. It is designed to provide a chemical analysis of the Martian surface and atmosphere. Analyses of rocks of known and unknown compositions have been made under simulated Martian conditions. The accuracies attained are generally comparable to those of the Surveyor lunar analyses. Improvements have been achieved in determining carbon and oxygen, so that a few per cent of water or carbonates in rocks can be detected. Some aspects of the integration of such an experiment with the spacecraft, a possible mission profile, and some other problems associated with a soft-landing mission to Mars are discussed. The importance of such a chemical analysis experiment in answering current questions about the nature and history of Martian surface material and its suitability for life processes is presented.
An approximate model was developed to establish design curves for the saturation region and a more complete model developed to characterize the current-voltage curves for an alpha-particle pressure sensor.
Elastic and nonelastic scattering cross sections from 42-MeV alpha particles interacting with helium isotopes
Alpha particle and proton beams in radiation therapy of pituitary gland tumors and adenoma