Solar surface nuclear reactions
Nuclear reactions on solar surface - radiochemical studies of material recovered from discoverer xvii launched during solar flare
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Nuclear reactions on solar surface - radiochemical studies of material recovered from discoverer xvii launched during solar flare
Nuclear reaction products effect on population inversion in gas lasers, considering neutron irradiation enhancement of carbon dioxide laser output
Asymptotic boundary conditions as constraints in shell model for scattering, reactions and nuclear structure calculations
Nonresonant nuclear reaction calculation method for stellar temperature
Energy spread in outgoing particles from nuclear reaction due to finite target thickness - optimum target orientation in nuclear reactor experiments
Nuclear reaction rates between nuclei vibrating about adjacent lattice sites in highly dense stars from solving Schroedinger equation
Nuclear reactions and elementary particle reactions in Friedman universe with positive lepton abundance and degenerate electrons, discussing prestellar helium synthesis
Information on solar He-3 from nuclear reactions in flares was considered. Consideration was also given to the development of models for these reactions as well as the abundance of He-3 in the photosphere. Data show that abundances may be explained by nuclear reactions of flare acceleration protons and alpha particles with the ambient atmosphere, provided that various assumptions are made on the directionality of the interacting beams and acceleration of the particles after production.
Measurement of secondary spectra from high-energy nuclear reactions
Calculational methods for estimation of dose from external proton exposure of arbitrary convex bodies are briefly reviewed. All the necessary information for the estimation of dose in soft tissue is presented. Special emphasis is placed on retaining the effects of nuclear reaction, especially in relation to the dose equivalent. Computer subroutines to evaluate all of the relevant functions are discussed. Nuclear reaction contributions for standard space radiations are in most cases found to be significant. Many of the existing computer programs for estimating dose in which nuclear reaction effects are neglected can be readily converted to include nuclear reaction effects by use of the subroutines described herein.
Three-body problem application to nuclear reactions involving neutron, proton and heavy nucleus, parametrizing two-body interactions in terms of s-wave separable potentials
Rate of nuclear reactions in stars calculated using solid state method
Nuclear reaction cross section data for spacecraft shield design, and for determining radiation dose effect on astronauts
Procedure for calculating rates of non-resonant nuclear reactions at stellar temperatures
Several aspects of nonelastic nuclear reactions which proceed through the formation of a compound nucleus are dealt with. The full statistical model and the partial statistical model are described and computer programs based on these models are presented along with operating instructions and input and output for sample problems. A theoretical development of the expression for the reaction cross section for the hybrid case which involves a combination of the continuum aspects of the full statistical model with the discrete level aspects of the partial statistical model is presented. Cross sections for level excitation and gamma production by neutron inelastic scattering from the nuclei Al-27, Fe-56, Si-28, and Pb-208 are calculated and compared with avaliable experimental data.
The use of the various nuclear reactions is described by which I-123,a low radiation dose radiopharmaceutical, can be cyclotron-produced. Methods of directly producing I-123 and those which indirectly produce the radionuclide through the beta (+) decay of its nautral precursor, Xe-123. It is impossible to separate from the radioiodine contaminants, notably I-124, which occur in the direct method. Thus, it is preferable to produce pure I-123 from Xe-123 which is easily separated from the radioiodines. Among the characteristics of I-123 is the capability of reducing the patient dose in a thyroid uptake measurement to a very small percentage of that delivered by the more commonly used I-131.
Annular lithium drifted germanium detector for studying nuclear reaction gamma rays
Energetic nuclear bombardment effects on stellar surface element abundance calculated with statistical theory in A magnetic variable star abundance anomaly