SIS junction as a detector at submillimeter wavelength

被引：0

作者：

Karpov, A ^{[1
]}

Blondel, J ^{[1
]}

Voss, M ^{[1
]}

Gundlach, KH ^{[1
]}

机构：

[1] Inst Radio Astron Millimetr, F-38406 St Martin Dheres, France

来源：

APPLIED SUPERCONDUCTIVITY 1997, VOLS 1 AND 2: VOL 1: SMALL SCALE AND ELECTRONIC APPLICATIONS; VOL 2: LARGE SCALE AND POWER APPLICATIONS | 1997年 / 158期

关键词：

D O I：

暂无

中图分类号：

O59 [应用物理学];

学科分类号：

摘要：

We present a possibility to create a new type of practical detector for the use in radio astronomy at submillimeter wavelength. The sensitivity of the developed submillimeter SIS direct detector receiver is competitive the best semiconductor bolometer receiver for the same wavelength. The SIS direct detector works at 4.5 K instead of 0.1-0.3 K required for a bolometer.

引用

页码：373 / 376

页数：4

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