{"title":"比例计数器在近地任务中作为太阳x射线监测器的有效性","authors":"P. Clark, S. Floyd, J. Trombka","doi":"10.1109/CHERBS.1997.660255","DOIUrl":null,"url":null,"abstract":"A proportional counter with a special mask/filter (SMPC) designed to measure solar output from 1 to 10 keV and to enhance sensitivity at higher energies where the solar flux is lower, as well as an experimental Si PIN detector (SMPN) are being used to measure solar flux on the Near Earth Asteroid Rendezvous (NEAR) mission. The complimentary nature of their performances is considered.","PeriodicalId":197895,"journal":{"name":"Conference on the High Energy Radiation Background in Space. Workshop Record","volume":"1 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1997-07-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"3","resultStr":"{\"title\":\"The effectiveness of the proportional counter as a solar X-ray monitor on the NEAR mission\",\"authors\":\"P. Clark, S. Floyd, J. Trombka\",\"doi\":\"10.1109/CHERBS.1997.660255\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"A proportional counter with a special mask/filter (SMPC) designed to measure solar output from 1 to 10 keV and to enhance sensitivity at higher energies where the solar flux is lower, as well as an experimental Si PIN detector (SMPN) are being used to measure solar flux on the Near Earth Asteroid Rendezvous (NEAR) mission. The complimentary nature of their performances is considered.\",\"PeriodicalId\":197895,\"journal\":{\"name\":\"Conference on the High Energy Radiation Background in Space. Workshop Record\",\"volume\":\"1 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.1997.660255\",\"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.1997.660255","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
The effectiveness of the proportional counter as a solar X-ray monitor on the NEAR mission
A proportional counter with a special mask/filter (SMPC) designed to measure solar output from 1 to 10 keV and to enhance sensitivity at higher energies where the solar flux is lower, as well as an experimental Si PIN detector (SMPN) are being used to measure solar flux on the Near Earth Asteroid Rendezvous (NEAR) mission. The complimentary nature of their performances is considered.
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