T. W. Armstrong, B. L. Colborn, K. Dietz, S. O’Dell, M. Weisskopf
{"title":"宇宙射线质子产生的AXAF探测器背景","authors":"T. W. Armstrong, B. L. Colborn, K. Dietz, S. O’Dell, M. Weisskopf","doi":"10.1109/CHERBS.1997.660219","DOIUrl":null,"url":null,"abstract":"X-ray detector backgrounds expected for the planned AXAF mission due to the galactic cosmic ray (GCR) proton environment have been determined by detailed Monte Carlo simulations. The predicted GCR-induced prompt and activation backgrounds are about 0.03 and 0.02 counts/cm/sup 2/-s, respectively which are small compared to signal strengths expected for planned AXAF observation scenarios.","PeriodicalId":197895,"journal":{"name":"Conference on the High Energy Radiation Background in Space. Workshop Record","volume":"38 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1997-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"AXAF detector backgrounds produced by cosmic ray protons\",\"authors\":\"T. W. Armstrong, B. L. Colborn, K. Dietz, S. O’Dell, M. Weisskopf\",\"doi\":\"10.1109/CHERBS.1997.660219\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"X-ray detector backgrounds expected for the planned AXAF mission due to the galactic cosmic ray (GCR) proton environment have been determined by detailed Monte Carlo simulations. The predicted GCR-induced prompt and activation backgrounds are about 0.03 and 0.02 counts/cm/sup 2/-s, respectively which are small compared to signal strengths expected for planned AXAF observation scenarios.\",\"PeriodicalId\":197895,\"journal\":{\"name\":\"Conference on the High Energy Radiation Background in Space. Workshop Record\",\"volume\":\"38 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1997-07-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Conference on the High Energy Radiation Background in Space. Workshop Record\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/CHERBS.1997.660219\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Conference on the High Energy Radiation Background in Space. Workshop Record","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/CHERBS.1997.660219","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
AXAF detector backgrounds produced by cosmic ray protons
X-ray detector backgrounds expected for the planned AXAF mission due to the galactic cosmic ray (GCR) proton environment have been determined by detailed Monte Carlo simulations. The predicted GCR-induced prompt and activation backgrounds are about 0.03 and 0.02 counts/cm/sup 2/-s, respectively which are small compared to signal strengths expected for planned AXAF observation scenarios.
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