Data Library and Four-Parameter Empirical Formula for the Response Functions for Gamma-Ray Skyshine Dose

Author:

Hirayama Hideo1,Harima Yoshiko2,Sakamoto Yukio3,Kurosawa Naohiro4,Nemoto Makoto4

Affiliation:

1. High Energy Accelerator Research Organization 1-1, Oho, Tsukuba, Ibaraki 305-080, Japan

2. Techno-Solutions Corporation 3-2-5, Kasumigaseki Chiyoda-ku, Tokyo 100-6080, Japan

3. Japan Atomic Energy Agency Tokai, Ibaraki 319-1195, Japan

4. Visible Information Center, Inc., Tokai, Naka, Ibaraki 319-1112, Japan

Publisher

Informa UK Limited

Subject

Condensed Matter Physics,Nuclear Energy and Engineering,Nuclear and High Energy Physics

Reference6 articles.

1. The Integral Line-Beam Method for Gamma Skyshine Analysis

2. W. R. NELSON, Y. HIRAYAMA, and D. W. O. ROGERS, “EGS4 Code System,” SLAC-265, Stanford Linear Accelerator Center (1985).

3. “Photon Interaction Cross Section Library,” Radiation Shielding Information Center Data Package DLC-136/PHOTX, National Institute of Standards Technology.

4. J. K. SHULTIS and R. E. FAW, “Extensions to the Integral Line-Beam Method for Gamma-Ray Skyshine Analyses,” SAND94-2019, Sandia National Laboratories (1995).

5. C. D. ZERBY, “Radiation Flux Transformation as a Function of Density of an Infinite Medium with Anisotropic Point Sources,” ORNL-2100, Oak Ridge National Laboratory (1956).

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