{"title":"低频射电天文接收相控阵噪声参数测量及其应用","authors":"A. Sutinjo, D. Ung","doi":"10.1109/CAMA47423.2019.8959782","DOIUrl":null,"url":null,"abstract":"The noise temperature of a phased array is a function the noise parameters of the low-noise amplifiers connected to the antenna elements. However, noise parameters at low-frequency radio astronomy bands (below few hundred MHz) are not usually readily available. We discuss the significance of noise parameters in phased arrays and demonstrate a low-cost option for noise parameter extraction.","PeriodicalId":170627,"journal":{"name":"2019 IEEE Conference on Antenna Measurements & Applications (CAMA)","volume":"1 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2019-10-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Noise Parameter Measurement and Its Application in Receiving Phased Arrays for Low-Frequency Radio Astronomy\",\"authors\":\"A. Sutinjo, D. Ung\",\"doi\":\"10.1109/CAMA47423.2019.8959782\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The noise temperature of a phased array is a function the noise parameters of the low-noise amplifiers connected to the antenna elements. However, noise parameters at low-frequency radio astronomy bands (below few hundred MHz) are not usually readily available. We discuss the significance of noise parameters in phased arrays and demonstrate a low-cost option for noise parameter extraction.\",\"PeriodicalId\":170627,\"journal\":{\"name\":\"2019 IEEE Conference on Antenna Measurements & Applications (CAMA)\",\"volume\":\"1 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2019-10-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"2019 IEEE Conference on Antenna Measurements & Applications (CAMA)\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/CAMA47423.2019.8959782\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"2019 IEEE Conference on Antenna Measurements & Applications (CAMA)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/CAMA47423.2019.8959782","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Noise Parameter Measurement and Its Application in Receiving Phased Arrays for Low-Frequency Radio Astronomy
The noise temperature of a phased array is a function the noise parameters of the low-noise amplifiers connected to the antenna elements. However, noise parameters at low-frequency radio astronomy bands (below few hundred MHz) are not usually readily available. We discuss the significance of noise parameters in phased arrays and demonstrate a low-cost option for noise parameter extraction.