22–28 Jun 2019
DoubleTree at the Entrance to Universal Orlando
America/New_York timezone

3P81 - Analysis of Cygnus Electrical Signals

26 Jun 2019, 13:30
1h 30m
Universal Center (Double Tree at the Entrance to Universal Orlando)

Universal Center

Double Tree at the Entrance to Universal Orlando

Speaker

Mr Hoai-Tam (Tam) Truong (Mission Support and Test Services, LLC)

Description

MSTS product number: DOE/NV/03624-0386
The United States initiated the Subcritical Experiment (SCE) program to support stockpile stewardship mission shortly after the 1992 moratorium on underground nuclear testing was established. Many SCE’s are conducted at the Nevada National Security Site (NNSS) in Nevada. Cygnus is a high energy radiation generating device (RGD) located and operated at the NNSS and is a primary diagnostic for the SCE program.
The Cygnus Dual Beam Radiographic Facility consists of two identical radiographic sources, Cygnus 1 and Cygnus 2. From creation of the high power V-I drive to energy transport and X-ray conversion at the rod-pinch diode, the Cygnus machines utilize the following components: oil-filled Marx generator, water-filled pulse-forming line (PFL), water-filled coaxial transmission line (CTL), three-cell vacuum induction voltage adder (IVA), and rod-pinch diode. The diode pulse has the following electrical specifications: 2.25 MV, 60 kA, 60 ns. Each source has the following X-ray specifications: 1-mm diameter, 4 rad at 1 m, and 50 ns radiation pulse.
SCE’s are both single-event and high-value, therefore a high level of performance in reliability and reproducibility are key issues of Cygnus. Prior to executing such a SCE, there are a formidable number of shots (e.g. each of the two Cygnus RGD’s charging and discharging properly into the rod-pinch diode load) that must be executed to determine reliability and reproducibility of the Cygnus RGD’s. For every shot on Cygnus, voltages and currents along the machine are recorded and analyzed. In this paper we summarize attributes of the voltage and current waveforms at different locations using distribution plots. These distribution plots are used to quantify the reliability and reproducibility for Cygnus.
• This work was done by Mission Support and Test Services LLC, under Contract No. DE-NA0003624 with the U.S. Department of Energy.

Authors

Mr Hoai-Tam (Tam) Truong (Mission Support and Test Services, LLC) Mr Keith Hogge (Mission Support and Test Services, LLC) Mr Michael Misch (Mission Support and Test Services, LLC) Dr John Smith (Los Alamos National Laboratory) Mr Michael Garcia (Sandia National Laboratories) Mr Eugene Ormond (Sandia National Laboratories) Mr Martin Parrales (Sandia National Laboratories)

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