Kinev Nickolay V, Rudakov Kirill I, Filippenko Lyudmila V, Baryshev Andrey M, Koshelets Valery P
Kotelnikov Institute of Radio Engineering and Electronics of RAS, Mokhovaya 11-7, 125009 Moscow, Russia.
Kapteyn Astronomical Institute, University of Groningen, 9712 CP Groningen, The Netherlands.
Sensors (Basel). 2020 Dec 18;20(24):7267. doi: 10.3390/s20247267.
We report on the first implementation of a terahertz (THz) source based on a Josephson flux-flow oscillator (FFO) that radiates to open space. The excellent performance of this source and its maturity for practical applications has been demonstrated by the spectroscopy of gas absorption. To study the radiated power, we used a bolometric detection method and additionally calibrated the power by means of pumping the superconductor-insulator-superconductor (SIS) junction, integrated on a single chip with the FFO. For calibration, we developed a program using the SIS-detected power calculations in accordance with the Tien and Gordon model. The power emitted to open space is estimated to be from fractions of µW to several µW in the wide region from 0.25 THz up to 0.75 THz for different designs, with a maximum power of 3.3 µW at 0.34 THz. Next, we used a gas cell and a heterodyne superconducting integrated receiver to trace the absorption lines of water and ammonia with a spectral resolution better than 100 kHz. Our experiment for gas absorption is the first demonstration of the applicability of the FFO as an external active source for different tasks, such as THz spectroscopy, near-field THz imaging and microscopy.
我们报道了首个基于约瑟夫森磁通流振荡器(FFO)且能向开放空间辐射的太赫兹(THz)源的实现。该源的卓越性能及其在实际应用中的成熟度已通过气体吸收光谱得以证明。为研究辐射功率,我们采用了测辐射热检测方法,并通过对与FFO集成在同一芯片上的超导-绝缘体-超导(SIS)结进行抽运来额外校准功率。为进行校准,我们根据Tien和Gordon模型开发了一个使用SIS检测功率计算的程序。对于不同设计,在从0.25太赫兹到0.75太赫兹的宽区域内,向开放空间发射的功率估计为几微瓦的几分之一到几微瓦,在0.34太赫兹时最大功率为3.3微瓦。接下来,我们使用气室和外差超导集成接收器,以优于100千赫兹的光谱分辨率追踪水和氨的吸收线。我们的气体吸收实验首次证明了FFO作为用于不同任务(如太赫兹光谱学、近场太赫兹成像和显微镜)的外部有源源的适用性。