{"title":"表征SKA阶段1的RFI","authors":"A. Otto, R. Millenaar, P. S. van der Merwe","doi":"10.1109/RFINT.2016.7833536","DOIUrl":null,"url":null,"abstract":"The radio frequency environment in which the SKA Phase 1 telescopes should operate is characterised at locations within the proposed spiral arm layout. The total integrated power level of the radio frequency interference at the various locations is determined.","PeriodicalId":298772,"journal":{"name":"2016 Radio Frequency Interference (RFI)","volume":"1 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2016-10-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"5","resultStr":"{\"title\":\"Characterising RFI for SKA phase 1\",\"authors\":\"A. Otto, R. Millenaar, P. S. van der Merwe\",\"doi\":\"10.1109/RFINT.2016.7833536\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The radio frequency environment in which the SKA Phase 1 telescopes should operate is characterised at locations within the proposed spiral arm layout. The total integrated power level of the radio frequency interference at the various locations is determined.\",\"PeriodicalId\":298772,\"journal\":{\"name\":\"2016 Radio Frequency Interference (RFI)\",\"volume\":\"1 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2016-10-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"5\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"2016 Radio Frequency Interference (RFI)\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/RFINT.2016.7833536\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"2016 Radio Frequency Interference (RFI)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/RFINT.2016.7833536","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
The radio frequency environment in which the SKA Phase 1 telescopes should operate is characterised at locations within the proposed spiral arm layout. The total integrated power level of the radio frequency interference at the various locations is determined.