18–22 Jun 2017
Hilton Brighton Metropole Hotel
Europe/London timezone

Cygnus Performance on Five Subcritical Experiments

20 Jun 2017, 16:30
15m
Oxford Hall (Hilton Brighton Metropole Hotel)

Oxford Hall

Hilton Brighton Metropole Hotel

Speaker

Dr John Smith (Los Alamos National Laboratory)

Description

The Cygnus Dual Beam Radiographic Facility includes two identical radiographic sources - Cygnus 1 and Cygnus 2. Cygnus is the radiography source used in Subcritical Experiments (SCEs) at the Nevada National Security Site (NNSS). The machine specifications are: Electric - 2.25 MV, 60 kA, 60 ns; Radiation - 4 Rad, 1 mm, 50 ns; Operation - single shot, 2-shots/day. Cygnus has operated at the NNSS since February 2004. In this period, it has participated on five SCE experiments - Armando, Bacchus, Barolo A, Barolo B, and Pollux. SCE projects typically require over a hundred preparatory shots culminating in a single full-fidelity or SCE shot, and typically take over a year for completion. Therefore, SCE shots are high risk and high value making reproducibility and reliability utmost priority. In this regard, major effort is focused on operational performance. A quantitative performance measurement is valuable for tracking and maintaining Cygnus preparedness. In this work, we present a new model for analysis of Cygnus performance. This model uses dose distribution as the basis for calculation of reproducibility and reliability. It will be applied both to long-term (historical) and short-term (readiness) periods for each of the five SCEs.

*Work supported by the U.S. Department of Energy.

Author

Dr John Smith (Los Alamos National Laboratory)

Co-authors

Mr Keith Hogge (National Security Technologies) Mr Eugene Ormond (Sandia National Laboratories)

Presentation materials

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