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MgB2 Thin-Film Bolometer for Applications in Far-Infrared Instruments on Future Planetary Missions

机译:MgB2薄膜测厚仪,用于未来行星飞行任务的远红外仪器

摘要

A SiN membrane based MgB2 thin-film bolometer, with a non-optimized absorber, has been fabricated that shows an electrical noise equivalent power of 256 fW/square root Hz operating at 30 Hz in the 8.5 - 12.35 micron spectral bandpass. This value corresponds to an electrical specific detectivity of 7.6 x 10(exp 10) cm square root Hz/W. The bolometer shows a measured blackbody (optical) specific detectivity of 8.8 x 10(exp 9) cm square root Hz/W, with a responsivity of 701.5 kV/W and a first-order time constant of 5.2 ms. It is predicted that with the inclusion of a gold black absorber that a blackbody specific detectivity of 6.4 x 10(exp 10) cm/square root Hz/W at an operational frequency of 10 Hz, can be realized for integration into future planetary exploration instrumentation where high sensitivity is required in the 17 - 250 micron spectral wavelength range.
机译:制作了具有非优化吸收体的基于SiN膜的MgB2薄膜辐射热计,其在8.5-12.35微米光谱带通中在30 Hz下工作时显示出256 fW /平方根Hz的电噪声等效功率。该值对应于7.6 x 10(exp 10)cm平方根Hz / W的电气比探测率。辐射热计显示测得的黑体(光学)比探测率为8.8 x 10(exp 9)cm平方根Hz / W,响应率为701.5 kV / W,一阶时间常数为5.2 ms。预计通过包含金黑吸收剂,可以实现在10 Hz的工作频率下黑体比探测率为6.4 x 10(exp 10)cm /平方根Hz / W,可以集成到未来的行星探测仪器中在17-250微米光谱波长范围内要求高灵敏度的场合。

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