GREAT - a Monte Carlo Procedure for Calculating Gamma-radiation Environments Above Terrain PDF Download

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GREAT - a Monte Carlo Procedure for Calculating Gamma-radiation Environments Above Terrain

GREAT - a Monte Carlo Procedure for Calculating Gamma-radiation Environments Above Terrain PDF Author: J. H. Price
Publisher:
ISBN:
Category : Gamma rays
Languages : en
Pages : 46

Book Description
The GREAT Monte Carlo Procedure was written for the IBM 1130 Computer to calculate the energy and angle distribution of the scattered gamma-ray flux at a point detector in an air-ground geometry resulting from a plane-isotropic monoenergetic gamma-ray source parallel to the air-ground interface. The source, which is finite and annular in shape, may be positioned below the smooth ground surface to simulate the effects of a source located on rough ground. The point detector is located on the vertical axis of the annular source. Initial photon parameters, path lengths, interactions and scattering angles are obtained by random sampling of appropriate probability distributions. Each photon is traced as it scatters within the defined geometry and estimates are made of the flux contribution at the detector from each collision.

GREAT - a Monte Carlo Procedure for Calculating Gamma-radiation Environments Above Terrain

GREAT - a Monte Carlo Procedure for Calculating Gamma-radiation Environments Above Terrain PDF Author: J. H. Price
Publisher:
ISBN:
Category : Gamma rays
Languages : en
Pages : 46

Book Description
The GREAT Monte Carlo Procedure was written for the IBM 1130 Computer to calculate the energy and angle distribution of the scattered gamma-ray flux at a point detector in an air-ground geometry resulting from a plane-isotropic monoenergetic gamma-ray source parallel to the air-ground interface. The source, which is finite and annular in shape, may be positioned below the smooth ground surface to simulate the effects of a source located on rough ground. The point detector is located on the vertical axis of the annular source. Initial photon parameters, path lengths, interactions and scattering angles are obtained by random sampling of appropriate probability distributions. Each photon is traced as it scatters within the defined geometry and estimates are made of the flux contribution at the detector from each collision.

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