High-energy interactions in Kinetic Inductance Detectors arrays

被引：4

作者：

D'Addabbo, A. ^{[1
,2
,3
]}

Calvo, M. ^{[1
,2
]}

Goupy, J. ^{[1
,2
]}

Benoit, A. ^{[3
]}

Bourrion, O. ^{[4
,5
]}

Catalano, A. ^{[4
,5
]}

Macias-Perez, J. F. ^{[4
,5
]}

Monfardini, A. ^{[1
,2
]}

机构：

[1] Univ Grenoble 1, CNRS, Inst Neel, BP 166, F-38042 Grenoble, France

[2] Univ Grenoble 1, CNRS, F-38042 Grenoble, France

[3] Univ Roma La Sapienza, I-00185 Rome, Italy

[4] CNRS, LPSC, F-75700 Paris, France

[5] Univ Grenoble, Grenoble, France

来源：

MILLIMETER, SUBMILLIMETER, AND FAR-INFRARED DETECTORS AND INSTRUMENTATION FOR ASTRONOMY VII | 2014年 / 9153卷

关键词：

KID; Cosmic Rays; phonon propagation; space missions; PARTICLE;

D O I：

10.1117/12.2056441

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The impacts of Cosmic Rays on the detectors are a key problem for space-based missions. We are studying the effects of such interactions on arrays of Kinetic Inductance Detectors (KID), in order to adapt this technology for use on board of satellites. Before proposing a new technology such as the Kinetic Inductance Detectors for a space-based mission, the problem of the Cosmic Rays that hit the detectors during in-flight operation has to be studied in detail. We present here several tests carried out with KID exposed to radioactive sources, which we use to reproduce the physical interactions induced by primary Cosmic Rays, and we report the results obtained adopting different solutions in terms of substrate materials and array geometries. We conclude by outlining the main guidelines to follow for fabricating KID for space-based applications.

引用

页数：13

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