2012
DOI: 10.1007/s10909-012-0497-7
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Effect of Magnetic Fields on TiAu TES Bolometers for the SAFARI Instrument on the SPICA FIR Telescope

Abstract: At the Netherlands Institute for Space Research (SRON) we are developing Transition Edge Sensors (TES) bolometers for the SAFARI Imaging Spectrometer on the SPICA telescope. With the current design of the SPICA telescope a background magnetic field of about a Gauss with fluctuations of a couple percent is expected. The effect of this external magnetic field on the bolometer needs to be well understood in order to design effective shielding. We present the results of an investigation of magnetic field on the pe… Show more

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Cited by 8 publications
(6 citation statements)
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References 8 publications
(9 reference statements)
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“…Under ac bias (colored-dotted lines) with the TES in transition we observed a Fraunhofer-like oscillating pattern, typical of a superconducting weak-link structure. Under dc bias (dark line) the current oscillations are generally much smaller and more difficult to see as it was previously reported 12 . Another interesting difference between the ac and dc bias measurement is that at large applied magnetic field the ac current does not decrease as one would expect from the Meissner effect.…”
Section: Resultsmentioning
confidence: 54%
See 1 more Smart Citation
“…Under ac bias (colored-dotted lines) with the TES in transition we observed a Fraunhofer-like oscillating pattern, typical of a superconducting weak-link structure. Under dc bias (dark line) the current oscillations are generally much smaller and more difficult to see as it was previously reported 12 . Another interesting difference between the ac and dc bias measurement is that at large applied magnetic field the ac current does not decrease as one would expect from the Meissner effect.…”
Section: Resultsmentioning
confidence: 54%
“…The electrical contact to the bolometer is realized by 90nm thick Nb leads deposited on the top of the SiN legs. The sensor was previously characterised under dc bias 11,12 and showed a power plateau of 9.4fW and a dark NEP of 4.8 × 10 −19 W/ √ Hz at 30mK. Below we report the results for the TES ac biased at a frequency of 2.4MHz.…”
Section: Experimental Set-upmentioning
confidence: 96%
“…[78] . 2012年, 荷兰研究人员研制了Ti/Au超导TES探测器, 在85 mK温度下测量NEP达到了5.0×10 −19 W Hz −1/2 左 右, 拟应用在SPICA望远镜的SAFARI成像光谱仪 上 [79] . 目前国内在超导TES研究方面还处于起步阶段, 中国科学院紫金山天文台、清华大学、中国科学技术 大学等单位开展了相关的研究工作.…”
Section: −2009年又进一步将阵元规模扩充到64×256像unclassified
“…The electrical contact to the bolometer is realized by 90 nm thick Nb wiring on the top of SiN legs. The sensor was previously characterised under dc bias in the set-up described in 5,6 and showed a power plateau of 9.4fW and a dark NEP of 4.8 · 10 −19 W/ √ Hz at 30 mK. The pixel is fabricated on a test chip with 4 other pixels.…”
Section: Singel Pixel Characterization With the Fdm Set-upmentioning
confidence: 99%
“…Here below we present the results of the single pixel characterisation under ac bias of a low-G bolometer developed for Safari. 5,6…”
Section: Introductionmentioning
confidence: 99%