W. Boynton, L. Evans, R. Starr, J. Bruckner, S. Bailey, J. Trombka
{"title":"火星观察者伽玛射线光谱仪的感应背景","authors":"W. Boynton, L. Evans, R. Starr, J. Bruckner, S. Bailey, J. Trombka","doi":"10.1109/CHERBS.1997.660242","DOIUrl":null,"url":null,"abstract":"The Mars Observer Gamma-Ray Spectrometer has provided data on background lines due to natural and cosmic-ray induced radioactivity during the mission's 11-month cruise. These data will help in determining, for future missions, the sensitivity for detection of gamma-ray lines of interest that are at or near the energy of measured background lines.","PeriodicalId":197895,"journal":{"name":"Conference on the High Energy Radiation Background in Space. Workshop Record","volume":"136 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1997-07-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"3","resultStr":"{\"title\":\"Induced background in the Mars Observer Gamma-Ray Spectrometer\",\"authors\":\"W. Boynton, L. Evans, R. Starr, J. Bruckner, S. Bailey, J. Trombka\",\"doi\":\"10.1109/CHERBS.1997.660242\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The Mars Observer Gamma-Ray Spectrometer has provided data on background lines due to natural and cosmic-ray induced radioactivity during the mission's 11-month cruise. These data will help in determining, for future missions, the sensitivity for detection of gamma-ray lines of interest that are at or near the energy of measured background lines.\",\"PeriodicalId\":197895,\"journal\":{\"name\":\"Conference on the High Energy Radiation Background in Space. Workshop Record\",\"volume\":\"136 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1997-07-22\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"3\",\"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.1997.660242\",\"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.1997.660242","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Induced background in the Mars Observer Gamma-Ray Spectrometer
The Mars Observer Gamma-Ray Spectrometer has provided data on background lines due to natural and cosmic-ray induced radioactivity during the mission's 11-month cruise. These data will help in determining, for future missions, the sensitivity for detection of gamma-ray lines of interest that are at or near the energy of measured background lines.