K. Abdalmalak, S. Romano, L. E. García Muñoz, Daniel Segovia Vargas
{"title":"双极化超宽带馈电系统在VLBI全球观测系统中的应用","authors":"K. Abdalmalak, S. Romano, L. E. García Muñoz, Daniel Segovia Vargas","doi":"10.1109/GSMM.2016.7500321","DOIUrl":null,"url":null,"abstract":"A new topology covering the new VGOS (VLBI Global Observation System) configuration is presented. The VGOS's requirement is a feed system covering from 2 GHz to 14 GHz. The new receiver topology is based on a log-spiral antenna printed on a conical surface. To achieve the dual circular polarization, an array of four elements is proposed. A proper balun for feeding the antenna and covering the whole band is also presented. The simulated results of radiation patterns show a pretty high symmetry in the radiation patterns at all frequencies with a maximum CP-XP level greater than 15 dB with a 10 dB gain.","PeriodicalId":156809,"journal":{"name":"2016 Global Symposium on Millimeter Waves (GSMM) & ESA Workshop on Millimetre-Wave Technology and Applications","volume":"27 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2016-06-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":"{\"title\":\"Dual polarized ultra wideband feed system for VLBI global observation system applications\",\"authors\":\"K. Abdalmalak, S. Romano, L. E. García Muñoz, Daniel Segovia Vargas\",\"doi\":\"10.1109/GSMM.2016.7500321\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"A new topology covering the new VGOS (VLBI Global Observation System) configuration is presented. The VGOS's requirement is a feed system covering from 2 GHz to 14 GHz. The new receiver topology is based on a log-spiral antenna printed on a conical surface. To achieve the dual circular polarization, an array of four elements is proposed. A proper balun for feeding the antenna and covering the whole band is also presented. The simulated results of radiation patterns show a pretty high symmetry in the radiation patterns at all frequencies with a maximum CP-XP level greater than 15 dB with a 10 dB gain.\",\"PeriodicalId\":156809,\"journal\":{\"name\":\"2016 Global Symposium on Millimeter Waves (GSMM) & ESA Workshop on Millimetre-Wave Technology and Applications\",\"volume\":\"27 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2016-06-06\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"2016 Global Symposium on Millimeter Waves (GSMM) & ESA Workshop on Millimetre-Wave Technology and Applications\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/GSMM.2016.7500321\",\"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 Global Symposium on Millimeter Waves (GSMM) & ESA Workshop on Millimetre-Wave Technology and Applications","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/GSMM.2016.7500321","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Dual polarized ultra wideband feed system for VLBI global observation system applications
A new topology covering the new VGOS (VLBI Global Observation System) configuration is presented. The VGOS's requirement is a feed system covering from 2 GHz to 14 GHz. The new receiver topology is based on a log-spiral antenna printed on a conical surface. To achieve the dual circular polarization, an array of four elements is proposed. A proper balun for feeding the antenna and covering the whole band is also presented. The simulated results of radiation patterns show a pretty high symmetry in the radiation patterns at all frequencies with a maximum CP-XP level greater than 15 dB with a 10 dB gain.