S. Duzellier, S. Bourdarie, R. Velazco, B. Nicolescu, R. Ecoffet
{"title":"在高地球轨道上查看两个静态32KB存储器的飞行数据","authors":"S. Duzellier, S. Bourdarie, R. Velazco, B. Nicolescu, R. Ecoffet","doi":"10.1109/REDW.2002.1045524","DOIUrl":null,"url":null,"abstract":"SEE (single event effect) in-flight measurements are presented for two 32 kB SRAMs in the MPTB orbit. The major contribution to the event rates comes from the proton radiation belts. During solar events, stuck bits occurred and the SEU rate is correlated to the high energy proton flux but the amplitude is not conserved.","PeriodicalId":135340,"journal":{"name":"IEEE Radiation Effects Data Workshop","volume":"27 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2002-12-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"9","resultStr":"{\"title\":\"SEE in-flight data for two static 32KB memories on high earth orbit\",\"authors\":\"S. Duzellier, S. Bourdarie, R. Velazco, B. Nicolescu, R. Ecoffet\",\"doi\":\"10.1109/REDW.2002.1045524\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"SEE (single event effect) in-flight measurements are presented for two 32 kB SRAMs in the MPTB orbit. The major contribution to the event rates comes from the proton radiation belts. During solar events, stuck bits occurred and the SEU rate is correlated to the high energy proton flux but the amplitude is not conserved.\",\"PeriodicalId\":135340,\"journal\":{\"name\":\"IEEE Radiation Effects Data Workshop\",\"volume\":\"27 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2002-12-10\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"9\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"IEEE Radiation Effects Data Workshop\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/REDW.2002.1045524\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"IEEE Radiation Effects Data Workshop","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/REDW.2002.1045524","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
SEE in-flight data for two static 32KB memories on high earth orbit
SEE (single event effect) in-flight measurements are presented for two 32 kB SRAMs in the MPTB orbit. The major contribution to the event rates comes from the proton radiation belts. During solar events, stuck bits occurred and the SEU rate is correlated to the high energy proton flux but the amplitude is not conserved.