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CREME96 and Related Error Rate Prediction Methods

机译:CREME96及其相关的错误率预测方法

摘要

Predicting the rate of occurrence of single event effects (SEEs) in space requires knowledge of the radiation environment and the response of electronic devices to that environment. Several analytical models have been developed over the past 36 years to predict SEE rates. The first error rate calculations were performed by Binder, Smith and Holman. Bradford and Pickel and Blandford, in their CRIER (Cosmic-Ray-Induced-Error-Rate) analysis code introduced the basic Rectangular ParallelePiped (RPP) method for error rate calculations. For the radiation environment at the part, both made use of the Cosmic Ray LET (Linear Energy Transfer) spectra calculated by Heinrich for various absorber Depths. A more detailed model for the space radiation environment within spacecraft was developed by Adams and co-workers. This model, together with a reformulation of the RPP method published by Pickel and Blandford, was used to create the CR ME (Cosmic Ray Effects on Micro-Electronics) code. About the same time Shapiro wrote the CRUP (Cosmic Ray Upset Program) based on the RPP method published by Bradford. It was the first code to specifically take into account charge collection from outside the depletion region due to deformation of the electric field caused by the incident cosmic ray. Other early rate prediction methods and codes include the Single Event Figure of Merit, NOVICE, the Space Radiation code and the effective flux method of Binder which is the basis of the SEFA (Scott Effective Flux Approximation) model. By the early 1990s it was becoming clear that CREME and the other early models needed Revision. This revision, CREME96, was completed and released as a WWW-based tool, one of the first of its kind. The revisions in CREME96 included improved environmental models and improved models for calculating single event effects. The need for a revision of CREME also stimulated the development of the CHIME (CRRES/SPACERAD Heavy Ion Model of the Environment) and MACREE (Modeling and Analysis of Cosmic Ray Effects in Electronics). The Single Event Figure of Merit method was also revised to use the solar minimum galactic cosmic ray spectrum and extended to circular orbits down to 200 km at any inclination. More recently a series of commercial codes was developed by TRAD (Test & Radiations) which includes the OMERE code which calculates single event effects. There are other error rate prediction methods which use Monte Carlo techniques. In this chapter the analytic methods for estimating the environment within spacecraft will be discussed.
机译:预测空间中单事件效应(SEE)的发生率需要了解辐射环境以及电子设备对该环境的响应。在过去的36年中,已经开发了几种分析模型来预测SEE率。第一次错误率计算是由Binder,Smith和Holman执行的。 Bradford和Pickel和Blandford在他们的CRIER(宇宙射线诱发的误差率)分析代码中引入了基本的Recruular ParallelePiped(RPP)方法来进行误差率计算。对于部件的辐射环境,两者都利用了由海因里希(Heinrich)计算的各种吸收深度的Cosmic Ray LET(线性能量转移)光谱。亚当斯和同事们为航天器内的空间辐射环境开发了更详细的模型。该模型与Pickel和Blandford发布的RPP方法的重新制定一起,用于创建CR ME(微电子上的宇宙射线效应)代码。大约在同一时间,夏皮罗根据布拉德福德(Bradford)出版的RPP方法编写了CRUP(宇宙射线打乱程序)。这是第一个专门考虑由于入射宇宙射线引起的电场变形而从耗尽区外部收集电荷的代码。其他早期速率预测方法和代码包括单事件品质因数,NOVICE,空间辐射代码以及作为SEFA(斯科特有效通量逼近)模型基础的Binder有效通量方法。到1990年代初,已经很明显CREME和其他早期模型需要修订。此修订版本CREME96已完成并作为基于WWW的工具发布,这是同类工具中的第一个。 CREME96中的修订包括改进的环境模型和用于计算单事件影响的改进模型。修订CREME的需要也刺激了CHIME(CRRES / SPACERAD重离子环境模型)和MACREE(电子宇宙射线效应的建模和分析)的发展。还对单项功因数法进行了修改,以使用太阳最小银河宇宙射线光谱,并在任何倾角下延伸至低至200 km的圆形轨道。最近,TRAD(测试与辐射)开发了一系列商业代码,其中包括计算单个事件效果的OMERE代码。还有其他使用蒙特卡洛技术的错误率预测方法。在本章中,将讨论估算航天器内环境的分析方法。

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    Adams James H. Jr.;

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  • 年度 2012
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