Multi-beam local oscillator for a 100-pixel heterodyne array receiver at THz

Y. Gan, B. Mirzaei, Jose R. G. Silva, A. Khalatpour, Q. Hu, C. Groppi, J. Siles, F. V. D. Tak, Jiansong Gao
{"title":"Multi-beam local oscillator for a 100-pixel heterodyne array receiver at THz","authors":"Y. Gan, B. Mirzaei, Jose R. G. Silva, A. Khalatpour, Q. Hu, C. Groppi, J. Siles, F. V. D. Tak, Jiansong Gao","doi":"10.1117/12.2560939","DOIUrl":null,"url":null,"abstract":"Generating multiple local oscillator beams is one challenge to develop large heterodyne receiver arrays (~100 pixels), which allow astronomical instrumentations mapping more area within limited space mission lifetime. Here, We combine a reflective Fourier grating with an unidirectional antenna coupled 3rd-order distributed feedback (DFB) quantum cascade laser (QCL) to generate 81 beams at 3.86 THz. We have measured the beam pattern of the diffracted 81 beams, which agrees well with a simulated result from COMSOL Multiphysics with respect to the angular distribution and power distribution among the 81 beams. The diffraction efficiency of the Fourier grating is derived to be 94±3%, which is very close to the simulated result of 97%. For an array of equal superconducting hot electron bolometer mixers, 64 out of 81 beams can pump the HEB mixers with similar power, resulting in receiver sensitivities within 10%. Such a combination of a Fourier grating and a QCL can create an LO with 100 beams or more, enabling a new generation of large heterodyne arrays for astronomical instrumentation. This paper is essentially a copy of our paper in Optics Express.","PeriodicalId":393026,"journal":{"name":"Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X","volume":"1 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2020-12-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1117/12.2560939","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0

Abstract

Generating multiple local oscillator beams is one challenge to develop large heterodyne receiver arrays (~100 pixels), which allow astronomical instrumentations mapping more area within limited space mission lifetime. Here, We combine a reflective Fourier grating with an unidirectional antenna coupled 3rd-order distributed feedback (DFB) quantum cascade laser (QCL) to generate 81 beams at 3.86 THz. We have measured the beam pattern of the diffracted 81 beams, which agrees well with a simulated result from COMSOL Multiphysics with respect to the angular distribution and power distribution among the 81 beams. The diffraction efficiency of the Fourier grating is derived to be 94±3%, which is very close to the simulated result of 97%. For an array of equal superconducting hot electron bolometer mixers, 64 out of 81 beams can pump the HEB mixers with similar power, resulting in receiver sensitivities within 10%. Such a combination of a Fourier grating and a QCL can create an LO with 100 beams or more, enabling a new generation of large heterodyne arrays for astronomical instrumentation. This paper is essentially a copy of our paper in Optics Express.
查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
太赫兹波段100像素外差阵列接收机的多波束本振
产生多个本振波束是开发大型外差接收器阵列(~100像素)的一个挑战,该阵列允许天文仪器在有限的空间任务寿命内绘制更多区域。在这里,我们将反射傅立叶光栅与单向天线耦合三阶分布反馈(DFB)量子级联激光器(QCL)结合在一起,产生了81束3.86太赫兹的光束。我们测量了81束衍射后的光束模式,在81束的角分布和功率分布方面与COMSOL Multiphysics模拟结果吻合得很好。傅里叶光栅的衍射效率为94±3%,与模拟结果97%非常接近。对于一组等量超导热电子测热计混合器,81束中有64束可以以相似的功率泵送HEB混合器,从而使接收器灵敏度在10%以内。这种傅立叶光栅和QCL的组合可以创建一个具有100束或更多光束的LO,为天文仪器提供新一代大型外差阵列。这篇论文基本上是我们在《光学快报》上的论文的副本。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 去求助
来源期刊
自引率
0.00%
发文量
0
期刊最新文献
Optical design study for the 860 GHz first-light camera module of CCAT-p (Erratum) Front Matter: Volume 11453 Demonstration of five-layer phase-flat achromatic half-wave plate with anti-reflective structures and superconducting magnetic bearing for CMB polarization experiments Design and demonstration of the frequency independent fast axis of the Pancharatnam base multi-layer half-wave plate for CMB polarization experiment Concept design of low frequency telescope for CMB B-mode polarization satellite LiteBIRD
×
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
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:604180095
Book学术
文献互助 智能选刊 最新文献 互助须知 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 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1