天鹅座电信号的分析

H. Truong, K. Hogge, M. Misch, J. Smith, M. Garcia, E. Ormond, M. Parrales
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引用次数: 0

摘要

1992年暂停地下核试验后不久,美国启动了亚临界试验(SCE)项目,以支持储备管理任务。许多SCE是在内华达州的内华达国家安全基地(NNSS)进行的。Cygnus是位于NNSS并运行的高能辐射产生装置(RGD),是SCE项目的主要诊断设备。这种分析方法将为单个Cygnus射击的故障排除结果提供标准,并且还可以监控Cygnus的长期性能。因此,这种类型的广泛分析将有助于优化sce上的Cygnus性能。天鹅座双光束射线照相设备由两个相同的射线照相源组成,天鹅座1号和天鹅座2号。从创建高功率V-I驱动器到能量传输和在棒捏二极管的x射线转换,Cygnus机器利用以下组件:充满油的马克思发生器,充满水的脉冲形成线(PFL),充满水的同轴传输线(CTL),三单元真空感应电压加法器(IVA)和棒捏二极管。二极管脉冲具有以下电气规格:2.25 MV, 60 kA, 60 ns。每个源具有以下x射线规格:直径1mm, 1m处4 rad, 50ns辐射脉冲。SCE是单事件和高价值的,因此高水平的可靠性和可重复性是Cygnus的关键问题。在执行这样的SCE之前,必须执行大量的射击(例如,两个Cygnus RGD的每一个充电和放电正确地进入杆捏二极管负载),以确定Cygnus RGD的可靠性和可重复性。对于天鹅座上的每一次射击,沿着机器的电压和电流都会被记录和分析。本文用分布图总结了不同位置的电压和电流波形的特性。这些分布图用于量化Cygnus的可靠性和再现性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Analysis of Cygnus Electrical Signals
The United States initiated the Subcritical Experiment (SCE) program to support a 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. This analysis methodology will provide a standard to trouble shoot results of individual Cygnus shots, and also to monitor long term Cygnus performance. Accordingly, this type of extensive analysis will contribute to optimized Cygnus performance on SCEs. 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.
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