VARIATION IN PROTON-INDUCED UPSETS RATES FROM LARGE SOLAR-FLARES USING AN IMPROVED SEU MODEL

被引：15

作者：

NORMAND, E ^{[1
]}

STAPOR, WJ ^{[1
]}

机构：

[1] USN,RES LAB,WASHINGTON,DC 20375

来源：

IEEE TRANSACTIONS ON NUCLEAR SCIENCE | 1990年 / 37卷 / 06期

关键词：

D O I：

10.1109/23.101213

中图分类号：

TM [电工技术]; TN [电子技术、通信技术];

学科分类号：

0808 ; 0809 ;

摘要：

Proton integral flux measurements during solar energetic particle (SEP) events, from the CPME instrument onboard the IMP-8 satellite, and the proton detector on the GOES-7 satellite, were utilized to calculate proton-induced SEU. An improved two-parameter SEU cross section model was used for three RAM devices. The log of the 239 actual RAM upsets on the TDRS-1 satellite during the Oct. 19, 1989 SEP event allowed a comparison between the recorded number of upset/chip per day, and those predicted based on the GOES-7 data, the 2-parameter model and the shielding distribution curve. © 1990 IEEE

引用

页码：1947 / 1952

页数：6

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