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首页> 外文期刊>Superconductor Science & Technology >Fabarication process and noise properties of antenna- coupled microbolometers based on superconducting YBCO films
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Fabarication process and noise properties of antenna- coupled microbolometers based on superconducting YBCO films

机译:基于超导YBCO薄膜的天线耦合测微仪的制造过程和噪声特性

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摘要

An analysis of how the detectivity and lifetimedepend on the fabrication process of Superconducting antenna-coupled microbolometers has been carried out. The temperaturedependences of responsivity and noise equivalent power (NEP)have been estimated in terms of the thermal model. To reveal themain degradation mechanism, 1/f-noise characterization has beenused. Monte-Carlo simulation of the annealing procedure ofYBa_2Cu_3O_7 (YBCO) films for the operating ranges offrequency and temperature has shown that prevailing sources offlicker noise in superconducting microstrips are associated withtransitions of oxygen atoms situated close to low-angleboundaries of the film blocks. The magnetron sputteringtechnique has been optimized to reduce the Hooge parameter forflicker noise to a record-breaking low value for YBCO films ofabout 10~(-4) at 93 K. Comparative analysis of chemical, ionand laser etching techniques by low-temperature scanningelectron microscopy and magneto-optics allowed the fabricationof microstrips with uniform current distribution characterized bycritical current density higher than 10~6 A cm~(-2) at 77 K andlong-time stability. The process of low-energy ion milling ofYBCO films with an Ar~+ beam generated in a duopigatron ionsource was used to reach a width resolution at the topology edgebetter than 0.2 #mu#m. The antenna-coupled bolometersfabricated from the superconducting microstrips were used toregister microwave radiation at a frequency of 70.3 GHz andtemperature of 93 K. It is demonstrated that the developedtechnology makes possible the fabrication of long-lived YBCO-based antenna microbolometers with electrical NEP_e = 1.5 X10~(-12) W Hz~(-1/2). The calculated response time of theantenna is about 3-l50 ns. Further development is associated withfabrication of coupling microbolometers with immersed lens,with predicted optical detectivityD*= (4 X 10~9-4 X 10~(10)) cm Hz~(1/2) W~(-1) in thewavelength range 100-1000 #mu#m.
机译:已经进行了关于探测性和寿命如何取决于超导天线耦合微辐射热计的制造过程的分析。已经根据热模型估算了响应度和噪声等效功率(NEP)的温度依赖性。为了揭示主要的降解机理,已使用1 / f噪声表征。对YBa_2Cu_3O_7(YBCO)薄膜在频率和温度范围内的退火过程的蒙特卡洛模拟表明,超导微带中主要的闪烁噪声源与位于薄膜块低角边界附近的氧原子跃迁有关。对磁控溅射技术进行了优化,以将在93 K下约10〜(-4)的YBCO膜的Hooge参数闪烁噪声降低到创纪录的低值。通过低温扫描电子显微镜和化学方法对化学,离子和激光蚀刻技术进行比较分析磁光技术可以制造出具有均匀电流分布的微带,其特征在于:在77 K时的临界电流密度高于10〜6 A cm〜(-2),并且具有长期稳定性。利用双光电子产生的Ar〜+束对YBCO薄膜进行低能离子铣削,以使其在拓扑边缘处的宽度分辨率优于0.2#μm。由超导微带制成的天线耦合测辐射热计用于记录频率为70.3 GHz,温度为93 K的微波辐射。事实证明,这项开发的技术使NEP_e = 1.5 X10的长寿命基于YBCO的天线测微辐射计的制造成为可能。 〜(-12)W Hz〜(-1/2)。天线的计算响应时间约为3到50 ns。进一步的发展与具有浸没透镜的耦合测微计的制造有关,预测的光学探测性D * =(4 X 10〜9-4 X 10〜(10))cm Hz〜(1/2)W〜(-1) 100-1000#mu#m。

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