完整後設資料紀錄
DC 欄位 | 值 | 語言 |
---|---|---|
dc.contributor.author | Chen, Ying | en_US |
dc.contributor.author | Wu, Kun-Long | en_US |
dc.contributor.author | Huang, Ching-Ying | en_US |
dc.contributor.author | Chang, Che-Kun | en_US |
dc.contributor.author | Sun, Xin | en_US |
dc.contributor.author | Li, Bin | en_US |
dc.contributor.author | Hu, Robert | en_US |
dc.date.accessioned | 2018-08-21T05:57:04Z | - |
dc.date.available | 2018-08-21T05:57:04Z | - |
dc.date.issued | 2017-01-01 | en_US |
dc.identifier.uri | http://hdl.handle.net/11536/147004 | - |
dc.description.abstract | This paper describes our progress in the design of cryogenic LNAs using OMMIC 70nm mHEMT for the Square Kilometer-Array (SKA) project and the Shanghai 65-Meter radio astronomical telescope. Different LNAs covering the aggregate 1 similar to 40GHz frequency range are designed and measured on-wafer at room temperature, and T-n for the 1 similar to 10, 5 similar to 15, and 10 similar to 40GHz LNAs are 80K, 90K, and 120K, respectively, with the gain all larger than 20dB. One 1 similar to 10GHz LNA chip is then packaged and tested cryogenically, and the noise temperature improvement factor is 6 similar to 8, which is smaller than what can be obtained from the WIN pHEMT. Performance repeatability among different chips has been carried out. | en_US |
dc.language.iso | en_US | en_US |
dc.subject | LNA | en_US |
dc.subject | wideband | en_US |
dc.subject | cryogenic | en_US |
dc.subject | mHEMT | en_US |
dc.title | OMMIC 70nm-mHEMT LNA Design | en_US |
dc.type | Proceedings Paper | en_US |
dc.identifier.journal | 2017 IEEE ASIA PACIFIC MICROWAVE CONFERENCE (APMC) | en_US |
dc.citation.spage | 1192 | en_US |
dc.citation.epage | 1195 | en_US |
dc.contributor.department | 電機學院 | zh_TW |
dc.contributor.department | College of Electrical and Computer Engineering | en_US |
dc.identifier.wosnumber | WOS:000426648000311 | en_US |
顯示於類別: | 會議論文 |