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A Photonic Local Oscillator Source for Far-IR and Sub-mm Heterodyne Receivers
https://jaxa.repo.nii.ac.jp/records/36693
https://jaxa.repo.nii.ac.jp/records/3669339246949-6aaf-4294-bd94-de7276c1eff1
名前 / ファイル | ライセンス | アクション |
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SA4618319.pdf (207.3 kB)
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Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||
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公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | A Photonic Local Oscillator Source for Far-IR and Sub-mm Heterodyne Receivers | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | departmental bulletin paper | |||||
著者 |
Shuji, MATSUURA
× Shuji, MATSUURA× Geofrey, A. BLAKE× Pin, CHEN× Rolf, A. WYSS× John, C. PEARSON× Herbert, M. PIKETT× Andrew, W. JACKSON× Christoph, KADOW× Arthur, C. GOSSARD |
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著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science | ||||||
著者所属(英) | ||||||
en | ||||||
Division of Geological and Planetary Sciences, California Institute of Technology | ||||||
著者所属(英) | ||||||
en | ||||||
Time and Frequency Division, National Institute of Standars and Technology | ||||||
著者所属(英) | ||||||
en | ||||||
Jet Propulsion Laboratory, California Institute of Technology | ||||||
著者所属(英) | ||||||
en | ||||||
Jet Propulsion Laboratory, California Institute of Technology | ||||||
著者所属(英) | ||||||
en | ||||||
Jet Propulsion Laboratory, California Institute of Technology | ||||||
著者所属(英) | ||||||
en | ||||||
Materials Depatment, University of California | ||||||
著者所属(英) | ||||||
en | ||||||
Materials Depatment, University of California | ||||||
著者所属(英) | ||||||
en | ||||||
Materials Depatment, University of California | ||||||
出版者 | ||||||
出版者 | 宇宙科学研究所 | |||||
出版者(英) | ||||||
出版者 | Institute of Space and Astronautical Science | |||||
書誌情報 |
en : The Institute of Space and Astronautical Science report. S.P. : Mid- and Far-Infrared Astronomy and Future Space Mission 巻 14, p. 337-344, 発行日 2000-12 |
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抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | We presented a recently developed compact solid-state far-infrared and sub-mm(terahertz) source. The radiation is generated by the optical heterodyne conversion (photomixing)in a low-temperature-grown GaAs (LTG-GaAs) photoconductor with a sub-picosecond responsetime. In photomixing, two frequency-offset laser beams are used to illuminate the photoconductor,resulting in the photocurrent oscillation at the difference frequency that drives a planar antenna onthe device. Such a photonic source has the great advantage of compactness, wide tuning range andhigh efficiency over existing electronic devices, and would be suitable for use as local oscillators inheterodyne receivers for IR/sub-mm astronomy. | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 0288-433X | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA10455137 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: SA4618319000 |