{"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}
引用次数: 5
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.