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2021 46th International Conference on Infrared, Millimeter and Terahertz Waves (IRMMW-THz)最新文献

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How 50 Years of Technology Development Has Transformed Millimeter-THz Astronomical Spectroscopy 50年的技术发展如何改变了毫米-太赫兹天文光谱学
Pub Date : 2021-08-29 DOI: 10.1109/IRMMW-THz50926.2021.9567033
P. Goldsmith
Millimeter wavelength astronomical spectroscopy started about 50 years ago, with the detection of carbon monoxide in interstellar space. The detection of massive clouds of molecular material in the Milky Way answered a long-standing question of from what stars form, but understanding the formation, structure, and evolution of these clouds demanded ever more sensitive receivers operating throughout the millimeter/submillimeter//THz range. Fractional frequency resolution R>3x105 is required to measure the motions in star-forming regions, with the result that heterodyne systems have become the dominant technology for detailed kinematic studies. To unravel the complexity of chemistry in molecular clouds, higher sensitivity was required. To achieve this, the Schottky diodes initially used as nonlinear elements were first cooled to reduce noise, but then replaced by superconductor insulator superconductor (SIS) and hot electron bolometer (HEB) mixers. Noise temperatures dropped from many thousands of K to < 100 K. Local oscillators (LOs) evolved from vacuum tubes to solid state devices. Large efforts were devoted to the development of frequency multipliers which allow mixers up to several THz to operate, starting with spectrally pure, tunable sources below 100 GHz. These allowed unbiased "spectral scans" and better use of observing time. The quantum cascade laser LO has allowed exploiting frequencies to 5 THz and beyond. Single antennas grew by more than an order of magnitude in collecting area. Interferometric arrays providing unprecedented angular resolution have allowed detailed observations of sources ranging from planet-forming disks to star-forming regions in distant galaxies. The interplay between technology and astronomical spectroscopy has been hugely productive, and continues, with new types of mixers for individual pixels and sophisticated focal plane arrays being developed for ground and space-based applications.
大约50年前,毫米波天文光谱学开始探测星际空间中的一氧化碳。对银河系中大量分子物质云的探测回答了一个长期存在的问题,即恒星是由什么形成的,但要了解这些云的形成、结构和演化,需要在毫米/亚毫米/太赫兹范围内工作的更灵敏的接收器。测量恒星形成区域的运动需要分数频率分辨率R>3x105,结果外差系统已成为详细运动学研究的主导技术。为了揭示分子云中化学的复杂性,需要更高的灵敏度。为了实现这一目标,最初用作非线性元件的肖特基二极管首先被冷却以降低噪声,但随后被超导体绝缘体(SIS)和热电子测热计(HEB)混频器所取代。噪声温度从几千K降至100 K以下。本振从真空管发展到固态器件。大量的努力致力于开发频率乘法器,允许高达几个太赫兹的混频器工作,从频谱纯净,100 GHz以下的可调谐源开始。这使得无偏“光谱扫描”和更好地利用观测时间成为可能。量子级联激光LO允许开发频率达到5太赫兹甚至更高。单天线的收集面积增加了一个数量级以上。干涉测量阵列提供了前所未有的角度分辨率,可以详细观察从行星形成盘到遥远星系中恒星形成区域的各种来源。技术和天文光谱学之间的相互作用已经产生了巨大的成果,并且还在继续,为地面和空间应用开发了用于单个像素的新型混合器和复杂的焦平面阵列。
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引用次数: 3
Study on a W-Band U-shaped Microstrip Meander-line Slow-wave Structure w波段u形微带弯曲线慢波结构的研究
Pub Date : 2021-08-29 DOI: 10.1109/IRMMW-THz50926.2021.9566867
Chi-Kan Liu, Lingna Yue, Jia Lu, Ziqing Bai, Wenxiang Wang, Yanyu Wei, Jin Xu, H. Yin, G. Zhao
A W-band U-shaped microstrip meander-line (MML) slow-wave structure (SWS) for traveling-wave tube (TWT) was designed and simulated in this work. The selection of materials used for the dielectric substrate in the SWS was discussed. Meanwhile, to improve the interaction impedance of the SWS, a new structure named conformal dielectric substrate was proposed. According to particle-in-cell (PIC) simulation results, the proposed structure was able to reach an output power of 28.86 W at 96 GHz, with the corresponding maximum gain of 23.8 dB. The 3 dB bandwidth was 7 GHz from 92 GHz to 99 GHz.
设计了一种用于行波管(TWT)的w波段u型微带弯曲线(MML)慢波结构(SWS)。讨论了SWS中介质衬底材料的选择。同时,为了提高SWS的相互作用阻抗,提出了一种新的共形介质衬底结构。根据粒子池(PIC)仿真结果,该结构在96 GHz时的输出功率为28.86 W,相应的最大增益为23.8 dB。3db带宽从92 GHz到99 GHz为7 GHz。
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引用次数: 0
Improved Germanium photoswitch for cavity dumping of a free-electron laser 用于自由电子激光器空腔倾倒的改进锗光开关
Pub Date : 2021-08-29 DOI: 10.1109/IRMMW-THz50926.2021.9567541
R. Rana, J. Klopf, C. Ciano, Abhishek Singh, S. Winnerl, H. Schneider, M. Helm, A. Pashkin
We demonstrate an optical switch based on gold implanted germanium (Ge:Au) suitable for cavity dumping of a free-electron laser (FEL). We achieve a switching contrast of more than 50 % in a broad range of FEL wavelengths from 6 to 90 µm. A linear relationship between the switching fluence and the frequency of the FEL optical field supported by our simulation highlights the role of a photoinduced finite sub-µm thickness of the reflecting plasma layer. The plasma switch exhibits negligible absorption of the FEL radiation in the ʻoffʼ state and requires only a moderate thermoelectric cooling at incident FEL power of several Watts.
研究了一种适合于自由电子激光器空腔倾倒的基于金植入锗(Ge:Au)的光开关。我们在6至90 μ m的FEL波长范围内实现了超过50%的开关对比度。我们的模拟支持了开关通量与FEL光场频率之间的线性关系,强调了反射等离子体层的光诱导有限亚μ m厚度的作用。等离子体开关在“off”状态下对FEL辐射的吸收可以忽略不计,在入射FEL功率为几瓦时只需要适度的热电冷却。
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引用次数: 0
Finding the accurate permittivity model for liquid water and heavy water at different temperatures in the Terahertz range 建立了太赫兹范围内不同温度下液态水和重水的精确介电常数模型
Pub Date : 2021-08-29 DOI: 10.1109/IRMMW-THz50926.2021.9567238
M. Lavancier, J. Lampin, R. Peretti
We present a study of liquid water and heavy water in the terahertz range at temperatures between 283K and 348K. We will fit our data with the fit@TDS software that provides a criterion to discriminate good models from others. We will present a comparison between the models proposed in the literature for liquid water and use this criterion to find the most accurate one.
我们提出了一项在283K和348K之间温度的太赫兹范围内液态水和重水的研究。我们将使用fit@TDS软件来拟合我们的数据,该软件提供了一个区分好模型的标准。我们将在文献中提出的液态水模型之间进行比较,并使用该准则找到最准确的模型。
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引用次数: 0
Damage Effect of Devices Induced by High Power Terahertz-wave 高功率太赫兹波对器件的损伤效应
Pub Date : 2021-08-29 DOI: 10.1109/IRMMW-THz50926.2021.9567580
X. Qi, Jingcheng Wang, P. Liang, Zheng Yan, T. Song, Wei Wang, Diwei Liu
A two-dimensional electro-thermal model of bipolar transistor irradiated by high power terahertz wave is established. The transient behaviors of the bipolar transistor are simulated and analyzed when high power terahertz wave is injected. The damage effect of the electric field, current density and temperature are observed theoretically. The voltage amplitude and the frequency on the device are investigated in detail. Empirical formulas of power damage threshold and energy damage threshold with pulse-width are summarized.
建立了高功率太赫兹波辐照双极晶体管的二维电热模型。模拟和分析了高功率太赫兹波注入双极晶体管的瞬态行为。从理论上观察了电场、电流密度和温度的损伤效应。详细研究了器件上的电压幅值和频率。总结了功率损伤阈值和能量损伤阈值随脉宽变化的经验公式。
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引用次数: 0
Stability of optical beats in laser chaos for THz wave generation and detection 激光混沌中太赫兹波产生与探测的光拍稳定性
Pub Date : 2021-08-29 DOI: 10.1109/IRMMW-THz50926.2021.9567524
F. Kuwashima, M. Jarrahi, S. Cakmakyapan, O. Morikawa, T. Shirao, K. Iwao, K. Kurihara, H. Kitahara, T. Furuya, K. Wada, M. Nakajima, M. Tani
Stability of optical beats between longitudinal laser modes in a chaotically oscillated laser diodes for THz wave generation and detection is demonstrated compared to a free-running continuous-wave laser conventional laser. The high stability of chaotically oscillating lasers makes these lasers promising candidates for optical pump sources in terahertz time-domain spectroscopy systems.
与自由运行的连续波激光器和传统激光器相比,研究了混沌振荡激光二极管中纵向激光模式之间光拍的稳定性。混沌振荡激光器的高稳定性使得这些激光器有希望成为太赫兹时域光谱系统中光泵浦源的候选者。
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引用次数: 0
Fast image deconvolution for enhancement of the resolution in the video rate terahertz imaging 用于提高视频速率太赫兹成像分辨率的快速图像反卷积
Pub Date : 2021-08-29 DOI: 10.1109/IRMMW-THz50926.2021.9567526
A. Rashidi, A. Minasyan, A. Cailly, M. Hamdi, O. Redon, L. Dussopt, H. Yahia
A fast image deconvolution algorithm is used to demonstrate the resolution enhancement of video rate camera acquired Terahertz images. Our algorithm is based on variable splitting technique with the use of a family of sparsity inducing regularizers for the first time in an image deconvolution application, it is also suitable for practical applications in industry with computationally constrained conditions. The results of the proposed process provide substantial enhancement on the quality and resolution of THz images.
采用一种快速图像反卷积算法来演示视频速率摄像机采集的太赫兹图像的分辨率增强。该算法基于变量分割技术,首次在图像反卷积应用中使用了一系列稀疏性诱导正则化器,也适用于具有计算约束条件的工业实际应用。该方法的结果大大提高了太赫兹图像的质量和分辨率。
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引用次数: 0
Molecular alignment stimulated by the coupled pulses of the ultrashort laser pulse and the terahertz pulse 超短激光脉冲和太赫兹脉冲耦合脉冲刺激的分子排列
Pub Date : 2021-08-29 DOI: 10.1109/IRMMW-THz50926.2021.9567022
H. Du, Jiang Long, Rui-Bo Jin, Tao Wu, Yanjun Fu
Field-free molecular alignment can be induced by the strong ultrashort laser pulses. Here, the improvement of the alignment is completed by the coupled pulses of the ultrashort laser pulse and the strong broadband terahertz pulse. The gaseous CO molecules are aligned by such coupled pulses, and the evolution of its states are studied based on the rigid rotor approximation theory with the simulation method. The influences of the pulses parameters on the alignment are also discussed.
强超短激光脉冲可以诱导无场分子取向。在这里,通过超短激光脉冲和强宽带太赫兹脉冲的耦合脉冲来完成对对准的改善。基于刚体转子近似理论和仿真方法,研究了气体CO分子在这种耦合脉冲作用下的排列过程。讨论了脉冲参数对准直的影响。
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引用次数: 0
Observation of Atomic Oxygen in the Mesosphere and Thermosphere of Earth with the THz Heterodyne Spectrometer GREAT GREAT太赫兹外差光谱仪对地球中间层和热层原子氧的观测
Pub Date : 2021-08-29 DOI: 10.1109/IRMMW-THz50926.2021.9566924
H. Richter, C. Buchbender, R. Güsten, R. Higgins, B. Klein, J. Stutzki, H. Wiesemeyer, H. Hübers
Atomic oxygen governs photochemistry and energy balance of the mesosphere and lower thermosphere of the Earth. Its concentration is extremely difficult to measure with remote sensing techniques since it has only few optically active transitions. Current indirect measurements involve photochemical models and the results are not always in agreement, particularly when obtained with different instruments. In addition, altitudes above 100 km are not covered by these methods. We report on direct measurements of the 4.7-THz fine-structure transition of atomic oxygen at 4.7448 THz using the German Receiver for Astronomy at Terahertz Frequencies on board the Stratospheric Observatory for Infrared Astronomy. Our measurements agree well with atmospheric models and satellite observations below 100 km.
原子氧控制着地球中间层和低层热层的光化学和能量平衡。它的浓度极难用遥感技术测量,因为它只有很少的光学活性跃迁。目前的间接测量涉及光化学模型,结果并不总是一致的,特别是当用不同的仪器获得时。此外,这些方法不包括100公里以上的高度。我们报告了在4.7448太赫兹处原子氧的4.7太赫兹精细结构跃迁的直接测量,使用了平流层红外天文观测台上的德国太赫兹天文接收机。我们的测量结果与大气模式和100公里以下的卫星观测结果吻合得很好。
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引用次数: 1
Electrically tunable detector for millimeter frequency band 电可调谐探测器毫米波段
Pub Date : 2021-08-29 DOI: 10.1109/IRMMW-THz50926.2021.9567261
A. Chernyadiev, D. But, C. Kołaciński, K. Ikamas, A. Lisauskas
An electrically tunable detector for sub-THz-frequency radiation based on Si CMOS technology is proposed. The tunability range of the implemented detector covers frequencies from 150 GHz up to 270 GHz with optical responsivity close to 1 kV/W and noise equivalent power below 20 ${text{pW}}/sqrt {{text{Hz}}} $. Potential applications include microwave bio and medical sensing, spectroscopy, amateur radio use and nondestructive imaging.
提出了一种基于硅CMOS技术的亚太赫兹频率辐射电可调谐探测器。所实现的探测器的可调谐范围从150 GHz到270 GHz,光响应度接近1 kV/W,噪声等效功率低于20 ${text{pW}}/sqrt {{text{Hz}}} $。潜在的应用包括微波生物和医学传感、光谱学、业余无线电使用和无损成像。
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引用次数: 0
期刊
2021 46th International Conference on Infrared, Millimeter and Terahertz Waves (IRMMW-THz)
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