Complementary Measurement of Thermal Architecture of NbSi TES with Alpha Particle and Complex Impedance
Abstract As shown by the Planck mission (Planck Collaboration. Astronomy and astrophysics. arXiv1303.5071P, 2013), background limited bolometers in a space environment are very sensitive to high energy particles. In order to not degrade their sensitivity, it is necessary to reduce this unwanted sign...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Martino, J. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2014 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science+Business Media New York 2014 |
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| Übergeordnetes Werk: |
Enthalten in: Journal of low temperature physics - Springer US, 1969, 176(2014), 3-4 vom: 14. Jan., Seite 350-355 |
|---|---|
| Übergeordnetes Werk: |
volume:176 ; year:2014 ; number:3-4 ; day:14 ; month:01 ; pages:350-355 |
| Links: |
|---|
| DOI / URN: |
10.1007/s10909-013-1053-9 |
|---|
| Katalog-ID: |
OLC2036822444 |
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| 245 | 1 | 0 | |a Complementary Measurement of Thermal Architecture of NbSi TES with Alpha Particle and Complex Impedance |
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| 520 | |a Abstract As shown by the Planck mission (Planck Collaboration. Astronomy and astrophysics. arXiv1303.5071P, 2013), background limited bolometers in a space environment are very sensitive to high energy particles. In order to not degrade their sensitivity, it is necessary to reduce this unwanted signal. To achieve this goal, a good understanding of the detector’s thermal architecture is mandatory. To investigate this question, we used an $$\alpha $$ particle source in front of our niobium silicon (NbSi) alloy Transition edge sensors (TES). The number of time constants required to fit the data and the way these time constants behave as we change the bias power gave us a good insight on the TES thermal architecture. Indeed we expect a decrease of the detector time constant due to the electro-thermal feedback properties. We will first present some standard characterizations of NbSi TES using a simple thermal model and how they indicate the presence of multiple thermal decouplings. Then we will show the results of the $$\alpha $$ particles measurements and how we used them to build our thermal model for Complex Impedance fitting. All this work has been done for the QUBIC experiment, a B-modes instrument. | ||
| 650 | 4 | |a Transition edge sensors | |
| 650 | 4 | |a Cosmic microwave background | |
| 650 | 4 | |a Alpha particles | |
| 650 | 4 | |a Complex impedance | |
| 650 | 4 | |a Thermal architecture | |
| 700 | 1 | |a Miniussi, A. |4 aut | |
| 700 | 1 | |a Piat, M. |4 aut | |
| 700 | 1 | |a Prêle, D. |4 aut | |
| 700 | 1 | |a Pajot, F. |4 aut | |
| 700 | 1 | |a Decourcelle, T. |4 aut | |
| 700 | 1 | |a Voisin, F. |4 aut | |
| 700 | 1 | |a Bélier, B. |4 aut | |
| 700 | 1 | |a Coron, N. |4 aut | |
| 700 | 1 | |a Ghribi, A. |4 aut | |
| 700 | 1 | |a Marnieros, S. |4 aut | |
| 700 | 1 | |a Perbost, C. |4 aut | |
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10.1007/s10909-013-1053-9 doi (DE-627)OLC2036822444 (DE-He213)s10909-013-1053-9-p DE-627 ger DE-627 rakwb eng 530 VZ Martino, J. verfasserin aut Complementary Measurement of Thermal Architecture of NbSi TES with Alpha Particle and Complex Impedance 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media New York 2014 Abstract As shown by the Planck mission (Planck Collaboration. Astronomy and astrophysics. arXiv1303.5071P, 2013), background limited bolometers in a space environment are very sensitive to high energy particles. In order to not degrade their sensitivity, it is necessary to reduce this unwanted signal. To achieve this goal, a good understanding of the detector’s thermal architecture is mandatory. To investigate this question, we used an $$\alpha $$ particle source in front of our niobium silicon (NbSi) alloy Transition edge sensors (TES). The number of time constants required to fit the data and the way these time constants behave as we change the bias power gave us a good insight on the TES thermal architecture. Indeed we expect a decrease of the detector time constant due to the electro-thermal feedback properties. We will first present some standard characterizations of NbSi TES using a simple thermal model and how they indicate the presence of multiple thermal decouplings. Then we will show the results of the $$\alpha $$ particles measurements and how we used them to build our thermal model for Complex Impedance fitting. All this work has been done for the QUBIC experiment, a B-modes instrument. Transition edge sensors Cosmic microwave background Alpha particles Complex impedance Thermal architecture Miniussi, A. aut Piat, M. aut Prêle, D. aut Pajot, F. aut Decourcelle, T. aut Voisin, F. aut Bélier, B. aut Coron, N. aut Ghribi, A. aut Marnieros, S. aut Perbost, C. aut Enthalten in Journal of low temperature physics Springer US, 1969 176(2014), 3-4 vom: 14. Jan., Seite 350-355 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:176 year:2014 number:3-4 day:14 month:01 pages:350-355 https://doi.org/10.1007/s10909-013-1053-9 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_22 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2185 GBV_ILN_4126 GBV_ILN_4323 AR 176 2014 3-4 14 01 350-355 |
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10.1007/s10909-013-1053-9 doi (DE-627)OLC2036822444 (DE-He213)s10909-013-1053-9-p DE-627 ger DE-627 rakwb eng 530 VZ Martino, J. verfasserin aut Complementary Measurement of Thermal Architecture of NbSi TES with Alpha Particle and Complex Impedance 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media New York 2014 Abstract As shown by the Planck mission (Planck Collaboration. Astronomy and astrophysics. arXiv1303.5071P, 2013), background limited bolometers in a space environment are very sensitive to high energy particles. In order to not degrade their sensitivity, it is necessary to reduce this unwanted signal. To achieve this goal, a good understanding of the detector’s thermal architecture is mandatory. To investigate this question, we used an $$\alpha $$ particle source in front of our niobium silicon (NbSi) alloy Transition edge sensors (TES). The number of time constants required to fit the data and the way these time constants behave as we change the bias power gave us a good insight on the TES thermal architecture. Indeed we expect a decrease of the detector time constant due to the electro-thermal feedback properties. We will first present some standard characterizations of NbSi TES using a simple thermal model and how they indicate the presence of multiple thermal decouplings. Then we will show the results of the $$\alpha $$ particles measurements and how we used them to build our thermal model for Complex Impedance fitting. All this work has been done for the QUBIC experiment, a B-modes instrument. Transition edge sensors Cosmic microwave background Alpha particles Complex impedance Thermal architecture Miniussi, A. aut Piat, M. aut Prêle, D. aut Pajot, F. aut Decourcelle, T. aut Voisin, F. aut Bélier, B. aut Coron, N. aut Ghribi, A. aut Marnieros, S. aut Perbost, C. aut Enthalten in Journal of low temperature physics Springer US, 1969 176(2014), 3-4 vom: 14. Jan., Seite 350-355 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:176 year:2014 number:3-4 day:14 month:01 pages:350-355 https://doi.org/10.1007/s10909-013-1053-9 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_22 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2185 GBV_ILN_4126 GBV_ILN_4323 AR 176 2014 3-4 14 01 350-355 |
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10.1007/s10909-013-1053-9 doi (DE-627)OLC2036822444 (DE-He213)s10909-013-1053-9-p DE-627 ger DE-627 rakwb eng 530 VZ Martino, J. verfasserin aut Complementary Measurement of Thermal Architecture of NbSi TES with Alpha Particle and Complex Impedance 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media New York 2014 Abstract As shown by the Planck mission (Planck Collaboration. Astronomy and astrophysics. arXiv1303.5071P, 2013), background limited bolometers in a space environment are very sensitive to high energy particles. In order to not degrade their sensitivity, it is necessary to reduce this unwanted signal. To achieve this goal, a good understanding of the detector’s thermal architecture is mandatory. To investigate this question, we used an $$\alpha $$ particle source in front of our niobium silicon (NbSi) alloy Transition edge sensors (TES). The number of time constants required to fit the data and the way these time constants behave as we change the bias power gave us a good insight on the TES thermal architecture. Indeed we expect a decrease of the detector time constant due to the electro-thermal feedback properties. We will first present some standard characterizations of NbSi TES using a simple thermal model and how they indicate the presence of multiple thermal decouplings. Then we will show the results of the $$\alpha $$ particles measurements and how we used them to build our thermal model for Complex Impedance fitting. All this work has been done for the QUBIC experiment, a B-modes instrument. Transition edge sensors Cosmic microwave background Alpha particles Complex impedance Thermal architecture Miniussi, A. aut Piat, M. aut Prêle, D. aut Pajot, F. aut Decourcelle, T. aut Voisin, F. aut Bélier, B. aut Coron, N. aut Ghribi, A. aut Marnieros, S. aut Perbost, C. aut Enthalten in Journal of low temperature physics Springer US, 1969 176(2014), 3-4 vom: 14. Jan., Seite 350-355 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:176 year:2014 number:3-4 day:14 month:01 pages:350-355 https://doi.org/10.1007/s10909-013-1053-9 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_22 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2185 GBV_ILN_4126 GBV_ILN_4323 AR 176 2014 3-4 14 01 350-355 |
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10.1007/s10909-013-1053-9 doi (DE-627)OLC2036822444 (DE-He213)s10909-013-1053-9-p DE-627 ger DE-627 rakwb eng 530 VZ Martino, J. verfasserin aut Complementary Measurement of Thermal Architecture of NbSi TES with Alpha Particle and Complex Impedance 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media New York 2014 Abstract As shown by the Planck mission (Planck Collaboration. Astronomy and astrophysics. arXiv1303.5071P, 2013), background limited bolometers in a space environment are very sensitive to high energy particles. In order to not degrade their sensitivity, it is necessary to reduce this unwanted signal. To achieve this goal, a good understanding of the detector’s thermal architecture is mandatory. To investigate this question, we used an $$\alpha $$ particle source in front of our niobium silicon (NbSi) alloy Transition edge sensors (TES). The number of time constants required to fit the data and the way these time constants behave as we change the bias power gave us a good insight on the TES thermal architecture. Indeed we expect a decrease of the detector time constant due to the electro-thermal feedback properties. We will first present some standard characterizations of NbSi TES using a simple thermal model and how they indicate the presence of multiple thermal decouplings. Then we will show the results of the $$\alpha $$ particles measurements and how we used them to build our thermal model for Complex Impedance fitting. All this work has been done for the QUBIC experiment, a B-modes instrument. Transition edge sensors Cosmic microwave background Alpha particles Complex impedance Thermal architecture Miniussi, A. aut Piat, M. aut Prêle, D. aut Pajot, F. aut Decourcelle, T. aut Voisin, F. aut Bélier, B. aut Coron, N. aut Ghribi, A. aut Marnieros, S. aut Perbost, C. aut Enthalten in Journal of low temperature physics Springer US, 1969 176(2014), 3-4 vom: 14. Jan., Seite 350-355 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:176 year:2014 number:3-4 day:14 month:01 pages:350-355 https://doi.org/10.1007/s10909-013-1053-9 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_22 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2185 GBV_ILN_4126 GBV_ILN_4323 AR 176 2014 3-4 14 01 350-355 |
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Martino, J. ddc 530 misc Transition edge sensors misc Cosmic microwave background misc Alpha particles misc Complex impedance misc Thermal architecture Complementary Measurement of Thermal Architecture of NbSi TES with Alpha Particle and Complex Impedance |
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530 VZ Complementary Measurement of Thermal Architecture of NbSi TES with Alpha Particle and Complex Impedance Transition edge sensors Cosmic microwave background Alpha particles Complex impedance Thermal architecture |
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ddc 530 misc Transition edge sensors misc Cosmic microwave background misc Alpha particles misc Complex impedance misc Thermal architecture |
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ddc 530 misc Transition edge sensors misc Cosmic microwave background misc Alpha particles misc Complex impedance misc Thermal architecture |
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Complementary Measurement of Thermal Architecture of NbSi TES with Alpha Particle and Complex Impedance |
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Complementary Measurement of Thermal Architecture of NbSi TES with Alpha Particle and Complex Impedance |
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Martino, J. Miniussi, A. Piat, M. Prêle, D. Pajot, F. Decourcelle, T. Voisin, F. Bélier, B. Coron, N. Ghribi, A. Marnieros, S. Perbost, C. |
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complementary measurement of thermal architecture of nbsi tes with alpha particle and complex impedance |
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Complementary Measurement of Thermal Architecture of NbSi TES with Alpha Particle and Complex Impedance |
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Abstract As shown by the Planck mission (Planck Collaboration. Astronomy and astrophysics. arXiv1303.5071P, 2013), background limited bolometers in a space environment are very sensitive to high energy particles. In order to not degrade their sensitivity, it is necessary to reduce this unwanted signal. To achieve this goal, a good understanding of the detector’s thermal architecture is mandatory. To investigate this question, we used an $$\alpha $$ particle source in front of our niobium silicon (NbSi) alloy Transition edge sensors (TES). The number of time constants required to fit the data and the way these time constants behave as we change the bias power gave us a good insight on the TES thermal architecture. Indeed we expect a decrease of the detector time constant due to the electro-thermal feedback properties. We will first present some standard characterizations of NbSi TES using a simple thermal model and how they indicate the presence of multiple thermal decouplings. Then we will show the results of the $$\alpha $$ particles measurements and how we used them to build our thermal model for Complex Impedance fitting. All this work has been done for the QUBIC experiment, a B-modes instrument. © Springer Science+Business Media New York 2014 |
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Abstract As shown by the Planck mission (Planck Collaboration. Astronomy and astrophysics. arXiv1303.5071P, 2013), background limited bolometers in a space environment are very sensitive to high energy particles. In order to not degrade their sensitivity, it is necessary to reduce this unwanted signal. To achieve this goal, a good understanding of the detector’s thermal architecture is mandatory. To investigate this question, we used an $$\alpha $$ particle source in front of our niobium silicon (NbSi) alloy Transition edge sensors (TES). The number of time constants required to fit the data and the way these time constants behave as we change the bias power gave us a good insight on the TES thermal architecture. Indeed we expect a decrease of the detector time constant due to the electro-thermal feedback properties. We will first present some standard characterizations of NbSi TES using a simple thermal model and how they indicate the presence of multiple thermal decouplings. Then we will show the results of the $$\alpha $$ particles measurements and how we used them to build our thermal model for Complex Impedance fitting. All this work has been done for the QUBIC experiment, a B-modes instrument. © Springer Science+Business Media New York 2014 |
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Abstract As shown by the Planck mission (Planck Collaboration. Astronomy and astrophysics. arXiv1303.5071P, 2013), background limited bolometers in a space environment are very sensitive to high energy particles. In order to not degrade their sensitivity, it is necessary to reduce this unwanted signal. To achieve this goal, a good understanding of the detector’s thermal architecture is mandatory. To investigate this question, we used an $$\alpha $$ particle source in front of our niobium silicon (NbSi) alloy Transition edge sensors (TES). The number of time constants required to fit the data and the way these time constants behave as we change the bias power gave us a good insight on the TES thermal architecture. Indeed we expect a decrease of the detector time constant due to the electro-thermal feedback properties. We will first present some standard characterizations of NbSi TES using a simple thermal model and how they indicate the presence of multiple thermal decouplings. Then we will show the results of the $$\alpha $$ particles measurements and how we used them to build our thermal model for Complex Impedance fitting. All this work has been done for the QUBIC experiment, a B-modes instrument. © Springer Science+Business Media New York 2014 |
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Complementary Measurement of Thermal Architecture of NbSi TES with Alpha Particle and Complex Impedance |
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Miniussi, A. Piat, M. Prêle, D. Pajot, F. Decourcelle, T. Voisin, F. Bélier, B. Coron, N. Ghribi, A. Marnieros, S. Perbost, C. |
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