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AbstractAbstract
[en] New calculations of the skyshine dose distribution of neutrons and secondary photons have been performed at Jefferson Lab using the Monte Carlo method. The dose dependence on neutron energy, distance to the neutron source, polar angle of a source neutron, and azimuthal angle between the observation point and the momentum direction of a source neutron have been studied. The azimuthally asymmetric term in the skyshine dose distribution is shown to be important in the dose calculations around high-energy accelerator facilities. A parameterization formula and corresponding computer code have been developed which can be used for detailed calculations of the skyshine dose maps
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1997; 7 p; SARE-3: simulation of accelerator radiation environments; Tsukuba, Ibaraki (Japan); 7-9 May 1997; JLAB-ACC--97-05; CONF-9705113--; CONTRACT AC05-84ER40150; Also available from OSTI as DE98001407; NTIS; US Govt. Printing Office Dep
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