地球同步微波降水辐射计的设计

W. Wilson, C. Ruf, C. Satter, Y. Rahmat-Samii
{"title":"地球同步微波降水辐射计的设计","authors":"W. Wilson, C. Ruf, C. Satter, Y. Rahmat-Samii","doi":"10.1109/MWSYM.1991.147222","DOIUrl":null,"url":null,"abstract":"The Geostationary Microwave Precipitation Radiometer is a passive microwave radiometer system to be flown on the NASA Geostationary Earth Observatory. This instrument will provide microwave images for meteorology. It will measure radiation from the Earth and its atmosphere in seven frequency bands from 37 to 220 GHz. The instrument will have a 4.4*4.0 m offset parabolic antenna which will be mechanically scanned to provide images of the Earth in about two hours. The radiometer system uses a low-loss quasi-optical frequency multiplexer. This multiplexer divides the input signal into four separate focal planes for the different radiometers. Conventional low-noise heterodyne mixer systems were used for most of the radiometers. However, because of the narrow bandwidths required in the 54 and 118 GHz radiometers, low-noise millimeter-wave amplifiers were used in the first stage.<<ETX>>","PeriodicalId":263441,"journal":{"name":"1991 IEEE MTT-S International Microwave Symposium Digest","volume":"11 9-10","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1991-07-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Design of a geostationary microwave precipitation radiometer\",\"authors\":\"W. Wilson, C. Ruf, C. Satter, Y. Rahmat-Samii\",\"doi\":\"10.1109/MWSYM.1991.147222\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The Geostationary Microwave Precipitation Radiometer is a passive microwave radiometer system to be flown on the NASA Geostationary Earth Observatory. This instrument will provide microwave images for meteorology. It will measure radiation from the Earth and its atmosphere in seven frequency bands from 37 to 220 GHz. The instrument will have a 4.4*4.0 m offset parabolic antenna which will be mechanically scanned to provide images of the Earth in about two hours. The radiometer system uses a low-loss quasi-optical frequency multiplexer. This multiplexer divides the input signal into four separate focal planes for the different radiometers. Conventional low-noise heterodyne mixer systems were used for most of the radiometers. However, because of the narrow bandwidths required in the 54 and 118 GHz radiometers, low-noise millimeter-wave amplifiers were used in the first stage.<<ETX>>\",\"PeriodicalId\":263441,\"journal\":{\"name\":\"1991 IEEE MTT-S International Microwave Symposium Digest\",\"volume\":\"11 9-10\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1991-07-10\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"1991 IEEE MTT-S International Microwave Symposium Digest\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/MWSYM.1991.147222\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"1991 IEEE MTT-S International Microwave Symposium Digest","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/MWSYM.1991.147222","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0

摘要

地球同步微波降水辐射计是一种被动微波辐射计系统,将在美国宇航局地球同步观测卫星上运行。这台仪器将为气象学提供微波图像。它将在37至220千兆赫的7个频段测量来自地球及其大气的辐射。该仪器将有一个4.4*4.0米偏移抛物面天线,将在大约两小时内对其进行机械扫描,以提供地球的图像。辐射计系统采用低损耗准光多频器。这个多路复用器将输入信号分成四个独立的焦平面,用于不同的辐射计。大多数辐射计采用传统的低噪声外差混频器系统。然而,由于54 GHz和118 GHz辐射计所需的带宽较窄,因此在第一阶段使用了低噪声毫米波放大器。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Design of a geostationary microwave precipitation radiometer
The Geostationary Microwave Precipitation Radiometer is a passive microwave radiometer system to be flown on the NASA Geostationary Earth Observatory. This instrument will provide microwave images for meteorology. It will measure radiation from the Earth and its atmosphere in seven frequency bands from 37 to 220 GHz. The instrument will have a 4.4*4.0 m offset parabolic antenna which will be mechanically scanned to provide images of the Earth in about two hours. The radiometer system uses a low-loss quasi-optical frequency multiplexer. This multiplexer divides the input signal into four separate focal planes for the different radiometers. Conventional low-noise heterodyne mixer systems were used for most of the radiometers. However, because of the narrow bandwidths required in the 54 and 118 GHz radiometers, low-noise millimeter-wave amplifiers were used in the first stage.<>
求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
自引率
0.00%
发文量
0
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信