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Conference Spotlight
Nuclear Energy Conference & Expo (NECX)
September 8–11, 2025
Atlanta, GA|Atlanta Marriott Marquis
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The Standards Committee is responsible for the development and maintenance of voluntary consensus standards that address the design, analysis, and operation of components, systems, and facilities related to the application of nuclear science and technology. Find out What’s New, check out the Standards Store, or Get Involved today!
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Deep Space: The new frontier of radiation controls
In commercial nuclear power, there has always been a deliberate tension between the regulator and the utility owner. The regulator fundamentally exists to protect the worker, and the utility, to make a profit. It is a win-win balance.
From the U.S. nuclear industry has emerged a brilliantly successful occupational nuclear safety record—largely the result of an ALARA (as low as reasonably achievable) process that has driven exposure rates down to what only a decade ago would have been considered unthinkable. In the U.S. nuclear industry, the system has accomplished an excellent, nearly seamless process that succeeds to the benefit of both employee and utility owner.
Dennis G. Perry, Margaret L. Simmons, James S. Gilmore
Nuclear Technology | Volume 33 | Number 1 | April 1977 | Pages 103-109
Technical Paper | Accelerator | doi.org/10.13182/NT77-A31767
Articles are hosted by Taylor and Francis Online.
The neutron flux generated at the main proton beam stop of the Los Alamos Clinton P. Anderson Meson Physics Facility (LAMPF) has unique properties of interest to materials radiation studies. Two of these properties—the total neutron flux and the neutron energy spectrum—were studied. The total neutron flux at the LAMPF radiation effects facility has been calculated by Monte Carlo techniques and measured by foil activation methods. The measurement compares well with the calculation and gives a total flux at the measurement position of 2 × 1011 n. mm−2 . s−1 at 1 mA of proton beam current. Later calculations at other locations show a flux of 1 × 1012 n . mm−2 . s−1.
