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ID 70101
フルテキストURL
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著者
Hirose, Haruaki Department of Physics, Graduate School of Engineering Science, Yokohama National University
Hasegawa, Masaya Institute of Particle and Nuclear Studies (IPNS), High Energy Accelerator Research Organization (KEK)
Kaneko, Daisuke International Center for Quantum-field Measurement Systems for Studies of the Universe and Particles (WPI-QUP), High Energy Accelerator Research Organization (KEK)
Nagasaki, Taketo Accelerator Laboratory (ACCL), High Energy Accelerator Research Organization (KEK)
Takaku, Ryota Graduate School of Environmental, Life, Natural Science and Technology, Okayama University
de Haan, Tijmen Institute of Particle and Nuclear Studies (IPNS), High Energy Accelerator Research Organization (KEK)
Takakura, Satoru Department of Physics, Faculty of Science, The University of Tokyo
Fujino, Takuro International Center for Quantum-field Measurement Systems for Studies of the Universe and Particles (WPI-QUP), High Energy Accelerator Research Organization (KEK)
抄録
We demonstrate a novel beam pattern measurement method for the side lobe characterization of cosmic microwave background telescopes. The method employs a power-variable artificial microwave source under feedback control from the detector under test on the telescope. It enables us to extend the dynamic range of the beam pattern measurement without introducing nonlinearity effects from the detector. We conducted a laboratory-based proof-of-concept experiment, measuring the H-plane beam pattern of a horn antenna coupled to a diode detector at 81 GHz. We gained an additional dynamic range of 60.3 dB attributed to the feedback control. In addition, we verified the measurement by comparing it with other reference measurements obtained using conventional methods. The method is also applicable to general optical measurements requiring a high dynamic range to detect subtle nonidealities in the characteristics of optical devices.
発行日
2026-01-20
出版物タイトル
Progress of Theoretical and Experimental Physics
2026巻
2号
出版者
Oxford University Press (OUP)
開始ページ
023F01
ISSN
2050-3911
資料タイプ
学術雑誌論文
言語
英語
OAI-PMH Set
岡山大学
著作権者
© The Author(s) 2026.
論文のバージョン
publisher
DOI
関連URL
isVersionOf https://doi.org/10.1093/ptep/ptag013
ライセンス
https://creativecommons.org/licenses/by/4.0/
Citation
Haruaki Hirose, Masaya Hasegawa, Daisuke Kaneko, Taketo Nagasaki, Ryota Takaku, Tijmen de Haan, Satoru Takakura, Takuro Fujino, Feedback-Controlled Beam Pattern Measurement Method Using a Power-Variable Calibration Source for Cosmic Microwave Background Telescopes, Progress of Theoretical and Experimental Physics, Volume 2026, Issue 2, February 2026, 023F01, https://doi.org/10.1093/ptep/ptag013
助成情報
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20H01921: 世界最大のミリ波超伝導検出器アレイで迫るニュートリノ質量絶対スケール ( 独立行政法人日本学術振興会 / Japan Society for the Promotion of Science )
22H04945: 謎の宇宙加速膨張 - 先進的な宇宙マイクロ波背景放射望遠鏡で解明に挑む - ( 独立行政法人日本学術振興会 / Japan Society for the Promotion of Science )
25H00403: 世界最大の超伝導センサー焦点面で解明する熱いビッグバン以前の宇宙 ( 独立行政法人日本学術振興会 / Japan Society for the Promotion of Science )
JPJSCCA20200003: ( 独立行政法人日本学術振興会 / Japan Society for the Promotion of Science )
( 文部科学省 / Ministry of Education )