skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Accelerator skyshine: Tyger, tyger, burning bright

Conference ·
OSTI ID:10133907
 [1];  [2];  [3]
  1. Southeastern Universities Research Association, Inc., Newport News, VA (United States). Continuous Electron Beam Accelerator Facility
  2. Northern Arizona Univ., Flagstaff, AZ (United States)
  3. Lawrence Livermore National Lab., CA (United States)

Neutron skyshine is, in most cases, the dominant source of radiation exposure to the general public from operation of well-shielded, high-energy accelerators. To estimate this exposure, tabulated solutions of the transport of neutrons through the air are frequently used. In previous works on skyshine, these tabular data have been parameterized into simple empirical equations that are easy and fast to use but are limited to distances greater than a few hundred meters from the accelerator. Our current report has refined this earlier work by including more realistic assumptions of neutron differential energy spectrum and angular distribution. These improved calculations essentially endorse the earlier parameterizations but make possible reasonably accurate dose estimates much closer to the skyshine source than before.

Research Organization:
Lawrence Livermore National Lab., CA (United States); Northern Arizona Univ., Flagstaff, AZ (United States)
Sponsoring Organization:
USDOE, Washington, DC (United States)
DOE Contract Number:
W-7405-ENG-48; AC05-84ER40150; AC03-76SF00098
OSTI ID:
10133907
Report Number(s):
UCRL-JC-108796; CONF-920617-14; ON: DE93007113
Resource Relation:
Conference: Annual meeting of the Health Physics Society,Columbus, OH (United States),21-25 Jun 1992; Other Information: PBD: Jun 1992
Country of Publication:
United States
Language:
English