元件级和系统级加速DRAM软错误率的比较

Ludger Borucki, G. Schindlbeck
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引用次数: 58

摘要

在现代DRAM设备中,来自地球宇宙射线(即高能中子)的单事件扰动比α粒子引起的软误差更重要。使用来自Los Alamos中子科学中心(LANSCE)的高强度广谱中子源,使用便携式存储器测试器表征了DRAM技术中从180 nm到70 nm的这些扰动的性质,这些扰动来自多个供应商的DIMM组件级。另一组加速中子束试验是用安装在主板上的DRAM内存进行的。利用这两种方法对软误差进行了表征,确定了中子角度、频率、数据模式和处理技术对软误差的影响。本研究的目的是分析这些差异对DRAM软错误的影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Comparison of accelerated DRAM soft error rates measured at component and system level
Single event upsets from terrestrial cosmic rays (i.e. high-energy neutrons) are more important than alpha particle induced soft errors in modern DRAM devices. A high intensity broad spectrum neutron source from the Los Alamos Neutron Science Center (LANSCE) was used to characterize the nature of these upsets in DRAM technologies ranging from 180 nm down to 70 nm from several vendors at the DIMM component level using a portable memory tester. Another set of accelerated neutron beam tests were made with DRAM DIMMs mounted on motherboards. Soft errors were characterized using these two methods to determine the influence of neutron angle, frequency, data patterns and process technology. The purpose of this study is to analyze the effects of these differences on DRAM soft errors.
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