Novel Frequency-Domain Multiplexing MKID Readout for the LiteBIRD Satellite
Abstract The satellite LiteBIRD (Light satellite for the studies of B-mode polarization and Inflation from cosmic background Radiation Detection) is being designed to detect the B-mode polarization of the cosmic microwave background radiation. LiteBIRD will carry about 2,000 detectors for measuremen...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Hattori, K. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2012 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science+Business Media, LLC 2012 |
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| Übergeordnetes Werk: |
Enthalten in: Journal of low temperature physics - Springer US, 1969, 167(2012), 5-6 vom: 20. Jan., Seite 671-677 |
|---|---|
| Übergeordnetes Werk: |
volume:167 ; year:2012 ; number:5-6 ; day:20 ; month:01 ; pages:671-677 |
| Links: |
|---|
| DOI / URN: |
10.1007/s10909-012-0506-x |
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| Katalog-ID: |
OLC2036817270 |
|---|
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| 100 | 1 | |a Hattori, K. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Novel Frequency-Domain Multiplexing MKID Readout for the LiteBIRD Satellite |
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| 520 | |a Abstract The satellite LiteBIRD (Light satellite for the studies of B-mode polarization and Inflation from cosmic background Radiation Detection) is being designed to detect the B-mode polarization of the cosmic microwave background radiation. LiteBIRD will carry about 2,000 detectors for measurements in five bands (60, 80, 100, 150, and 220 GHz). Microwave kinetic inductance detectors (MKIDs) that can be multiplexed in a single readout line are suitable for the large focal plane detector array. We develop an MKID readout system for LiteBIRD to monitor the amplitude, phase, and resonant frequency of each MKID resonator simultaneously and follow movements of the resonant frequency caused by changes in the input radiation intensity. This mechanism enables us to have a larger dynamic range for the MKIDs, compared with a system that monitors the amplitude and phase on the resonant frequency. We also propose an MKID having a half-wavelength resonator. This MKID transmits the resonant microwave signal from one feedline to another. It can offer clear microwaves passing through the resonators, even if the coupling and internal quality factors are mismatched. With this MKID, our readout system can track resonance frequency changes much more easily. We present the status of the readout system development and demonstrate the performance with the half-wavelength MKID. | ||
| 650 | 4 | |a Frequency-domain multiplexing | |
| 650 | 4 | |a Microwave kinetic inductance detectors | |
| 650 | 4 | |a Cosmic microwave background radiation | |
| 700 | 1 | |a Ariyoshi, S. |4 aut | |
| 700 | 1 | |a Hazumi, M. |4 aut | |
| 700 | 1 | |a Ishino, H. |4 aut | |
| 700 | 1 | |a Kibayashi, A. |4 aut | |
| 700 | 1 | |a Mima, S. |4 aut | |
| 700 | 1 | |a Otani, C. |4 aut | |
| 700 | 1 | |a Satoh, N. |4 aut | |
| 700 | 1 | |a Tomaru, T. |4 aut | |
| 700 | 1 | |a Yoshida, M. |4 aut | |
| 700 | 1 | |a Watanabe, H. |4 aut | |
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10.1007/s10909-012-0506-x doi (DE-627)OLC2036817270 (DE-He213)s10909-012-0506-x-p DE-627 ger DE-627 rakwb eng 530 VZ Hattori, K. verfasserin aut Novel Frequency-Domain Multiplexing MKID Readout for the LiteBIRD Satellite 2012 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, LLC 2012 Abstract The satellite LiteBIRD (Light satellite for the studies of B-mode polarization and Inflation from cosmic background Radiation Detection) is being designed to detect the B-mode polarization of the cosmic microwave background radiation. LiteBIRD will carry about 2,000 detectors for measurements in five bands (60, 80, 100, 150, and 220 GHz). Microwave kinetic inductance detectors (MKIDs) that can be multiplexed in a single readout line are suitable for the large focal plane detector array. We develop an MKID readout system for LiteBIRD to monitor the amplitude, phase, and resonant frequency of each MKID resonator simultaneously and follow movements of the resonant frequency caused by changes in the input radiation intensity. This mechanism enables us to have a larger dynamic range for the MKIDs, compared with a system that monitors the amplitude and phase on the resonant frequency. We also propose an MKID having a half-wavelength resonator. This MKID transmits the resonant microwave signal from one feedline to another. It can offer clear microwaves passing through the resonators, even if the coupling and internal quality factors are mismatched. With this MKID, our readout system can track resonance frequency changes much more easily. We present the status of the readout system development and demonstrate the performance with the half-wavelength MKID. Frequency-domain multiplexing Microwave kinetic inductance detectors Cosmic microwave background radiation Ariyoshi, S. aut Hazumi, M. aut Ishino, H. aut Kibayashi, A. aut Mima, S. aut Otani, C. aut Satoh, N. aut Tomaru, T. aut Yoshida, M. aut Watanabe, H. aut Enthalten in Journal of low temperature physics Springer US, 1969 167(2012), 5-6 vom: 20. Jan., Seite 671-677 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:167 year:2012 number:5-6 day:20 month:01 pages:671-677 https://doi.org/10.1007/s10909-012-0506-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_22 GBV_ILN_40 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2005 GBV_ILN_2185 GBV_ILN_4036 GBV_ILN_4126 GBV_ILN_4323 AR 167 2012 5-6 20 01 671-677 |
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10.1007/s10909-012-0506-x doi (DE-627)OLC2036817270 (DE-He213)s10909-012-0506-x-p DE-627 ger DE-627 rakwb eng 530 VZ Hattori, K. verfasserin aut Novel Frequency-Domain Multiplexing MKID Readout for the LiteBIRD Satellite 2012 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, LLC 2012 Abstract The satellite LiteBIRD (Light satellite for the studies of B-mode polarization and Inflation from cosmic background Radiation Detection) is being designed to detect the B-mode polarization of the cosmic microwave background radiation. LiteBIRD will carry about 2,000 detectors for measurements in five bands (60, 80, 100, 150, and 220 GHz). Microwave kinetic inductance detectors (MKIDs) that can be multiplexed in a single readout line are suitable for the large focal plane detector array. We develop an MKID readout system for LiteBIRD to monitor the amplitude, phase, and resonant frequency of each MKID resonator simultaneously and follow movements of the resonant frequency caused by changes in the input radiation intensity. This mechanism enables us to have a larger dynamic range for the MKIDs, compared with a system that monitors the amplitude and phase on the resonant frequency. We also propose an MKID having a half-wavelength resonator. This MKID transmits the resonant microwave signal from one feedline to another. It can offer clear microwaves passing through the resonators, even if the coupling and internal quality factors are mismatched. With this MKID, our readout system can track resonance frequency changes much more easily. We present the status of the readout system development and demonstrate the performance with the half-wavelength MKID. Frequency-domain multiplexing Microwave kinetic inductance detectors Cosmic microwave background radiation Ariyoshi, S. aut Hazumi, M. aut Ishino, H. aut Kibayashi, A. aut Mima, S. aut Otani, C. aut Satoh, N. aut Tomaru, T. aut Yoshida, M. aut Watanabe, H. aut Enthalten in Journal of low temperature physics Springer US, 1969 167(2012), 5-6 vom: 20. Jan., Seite 671-677 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:167 year:2012 number:5-6 day:20 month:01 pages:671-677 https://doi.org/10.1007/s10909-012-0506-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_22 GBV_ILN_40 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2005 GBV_ILN_2185 GBV_ILN_4036 GBV_ILN_4126 GBV_ILN_4323 AR 167 2012 5-6 20 01 671-677 |
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10.1007/s10909-012-0506-x doi (DE-627)OLC2036817270 (DE-He213)s10909-012-0506-x-p DE-627 ger DE-627 rakwb eng 530 VZ Hattori, K. verfasserin aut Novel Frequency-Domain Multiplexing MKID Readout for the LiteBIRD Satellite 2012 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, LLC 2012 Abstract The satellite LiteBIRD (Light satellite for the studies of B-mode polarization and Inflation from cosmic background Radiation Detection) is being designed to detect the B-mode polarization of the cosmic microwave background radiation. LiteBIRD will carry about 2,000 detectors for measurements in five bands (60, 80, 100, 150, and 220 GHz). Microwave kinetic inductance detectors (MKIDs) that can be multiplexed in a single readout line are suitable for the large focal plane detector array. We develop an MKID readout system for LiteBIRD to monitor the amplitude, phase, and resonant frequency of each MKID resonator simultaneously and follow movements of the resonant frequency caused by changes in the input radiation intensity. This mechanism enables us to have a larger dynamic range for the MKIDs, compared with a system that monitors the amplitude and phase on the resonant frequency. We also propose an MKID having a half-wavelength resonator. This MKID transmits the resonant microwave signal from one feedline to another. It can offer clear microwaves passing through the resonators, even if the coupling and internal quality factors are mismatched. With this MKID, our readout system can track resonance frequency changes much more easily. We present the status of the readout system development and demonstrate the performance with the half-wavelength MKID. Frequency-domain multiplexing Microwave kinetic inductance detectors Cosmic microwave background radiation Ariyoshi, S. aut Hazumi, M. aut Ishino, H. aut Kibayashi, A. aut Mima, S. aut Otani, C. aut Satoh, N. aut Tomaru, T. aut Yoshida, M. aut Watanabe, H. aut Enthalten in Journal of low temperature physics Springer US, 1969 167(2012), 5-6 vom: 20. Jan., Seite 671-677 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:167 year:2012 number:5-6 day:20 month:01 pages:671-677 https://doi.org/10.1007/s10909-012-0506-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_22 GBV_ILN_40 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2005 GBV_ILN_2185 GBV_ILN_4036 GBV_ILN_4126 GBV_ILN_4323 AR 167 2012 5-6 20 01 671-677 |
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10.1007/s10909-012-0506-x doi (DE-627)OLC2036817270 (DE-He213)s10909-012-0506-x-p DE-627 ger DE-627 rakwb eng 530 VZ Hattori, K. verfasserin aut Novel Frequency-Domain Multiplexing MKID Readout for the LiteBIRD Satellite 2012 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, LLC 2012 Abstract The satellite LiteBIRD (Light satellite for the studies of B-mode polarization and Inflation from cosmic background Radiation Detection) is being designed to detect the B-mode polarization of the cosmic microwave background radiation. LiteBIRD will carry about 2,000 detectors for measurements in five bands (60, 80, 100, 150, and 220 GHz). Microwave kinetic inductance detectors (MKIDs) that can be multiplexed in a single readout line are suitable for the large focal plane detector array. We develop an MKID readout system for LiteBIRD to monitor the amplitude, phase, and resonant frequency of each MKID resonator simultaneously and follow movements of the resonant frequency caused by changes in the input radiation intensity. This mechanism enables us to have a larger dynamic range for the MKIDs, compared with a system that monitors the amplitude and phase on the resonant frequency. We also propose an MKID having a half-wavelength resonator. This MKID transmits the resonant microwave signal from one feedline to another. It can offer clear microwaves passing through the resonators, even if the coupling and internal quality factors are mismatched. With this MKID, our readout system can track resonance frequency changes much more easily. We present the status of the readout system development and demonstrate the performance with the half-wavelength MKID. Frequency-domain multiplexing Microwave kinetic inductance detectors Cosmic microwave background radiation Ariyoshi, S. aut Hazumi, M. aut Ishino, H. aut Kibayashi, A. aut Mima, S. aut Otani, C. aut Satoh, N. aut Tomaru, T. aut Yoshida, M. aut Watanabe, H. aut Enthalten in Journal of low temperature physics Springer US, 1969 167(2012), 5-6 vom: 20. Jan., Seite 671-677 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:167 year:2012 number:5-6 day:20 month:01 pages:671-677 https://doi.org/10.1007/s10909-012-0506-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_22 GBV_ILN_40 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2005 GBV_ILN_2185 GBV_ILN_4036 GBV_ILN_4126 GBV_ILN_4323 AR 167 2012 5-6 20 01 671-677 |
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10.1007/s10909-012-0506-x doi (DE-627)OLC2036817270 (DE-He213)s10909-012-0506-x-p DE-627 ger DE-627 rakwb eng 530 VZ Hattori, K. verfasserin aut Novel Frequency-Domain Multiplexing MKID Readout for the LiteBIRD Satellite 2012 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, LLC 2012 Abstract The satellite LiteBIRD (Light satellite for the studies of B-mode polarization and Inflation from cosmic background Radiation Detection) is being designed to detect the B-mode polarization of the cosmic microwave background radiation. LiteBIRD will carry about 2,000 detectors for measurements in five bands (60, 80, 100, 150, and 220 GHz). Microwave kinetic inductance detectors (MKIDs) that can be multiplexed in a single readout line are suitable for the large focal plane detector array. We develop an MKID readout system for LiteBIRD to monitor the amplitude, phase, and resonant frequency of each MKID resonator simultaneously and follow movements of the resonant frequency caused by changes in the input radiation intensity. This mechanism enables us to have a larger dynamic range for the MKIDs, compared with a system that monitors the amplitude and phase on the resonant frequency. We also propose an MKID having a half-wavelength resonator. This MKID transmits the resonant microwave signal from one feedline to another. It can offer clear microwaves passing through the resonators, even if the coupling and internal quality factors are mismatched. With this MKID, our readout system can track resonance frequency changes much more easily. We present the status of the readout system development and demonstrate the performance with the half-wavelength MKID. Frequency-domain multiplexing Microwave kinetic inductance detectors Cosmic microwave background radiation Ariyoshi, S. aut Hazumi, M. aut Ishino, H. aut Kibayashi, A. aut Mima, S. aut Otani, C. aut Satoh, N. aut Tomaru, T. aut Yoshida, M. aut Watanabe, H. aut Enthalten in Journal of low temperature physics Springer US, 1969 167(2012), 5-6 vom: 20. Jan., Seite 671-677 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:167 year:2012 number:5-6 day:20 month:01 pages:671-677 https://doi.org/10.1007/s10909-012-0506-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_22 GBV_ILN_40 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2005 GBV_ILN_2185 GBV_ILN_4036 GBV_ILN_4126 GBV_ILN_4323 AR 167 2012 5-6 20 01 671-677 |
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Hattori, K. @@aut@@ Ariyoshi, S. @@aut@@ Hazumi, M. @@aut@@ Ishino, H. @@aut@@ Kibayashi, A. @@aut@@ Mima, S. @@aut@@ Otani, C. @@aut@@ Satoh, N. @@aut@@ Tomaru, T. @@aut@@ Yoshida, M. @@aut@@ Watanabe, H. @@aut@@ |
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Hattori, K. Ariyoshi, S. Hazumi, M. Ishino, H. Kibayashi, A. Mima, S. Otani, C. Satoh, N. Tomaru, T. Yoshida, M. Watanabe, H. |
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novel frequency-domain multiplexing mkid readout for the litebird satellite |
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Novel Frequency-Domain Multiplexing MKID Readout for the LiteBIRD Satellite |
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Abstract The satellite LiteBIRD (Light satellite for the studies of B-mode polarization and Inflation from cosmic background Radiation Detection) is being designed to detect the B-mode polarization of the cosmic microwave background radiation. LiteBIRD will carry about 2,000 detectors for measurements in five bands (60, 80, 100, 150, and 220 GHz). Microwave kinetic inductance detectors (MKIDs) that can be multiplexed in a single readout line are suitable for the large focal plane detector array. We develop an MKID readout system for LiteBIRD to monitor the amplitude, phase, and resonant frequency of each MKID resonator simultaneously and follow movements of the resonant frequency caused by changes in the input radiation intensity. This mechanism enables us to have a larger dynamic range for the MKIDs, compared with a system that monitors the amplitude and phase on the resonant frequency. We also propose an MKID having a half-wavelength resonator. This MKID transmits the resonant microwave signal from one feedline to another. It can offer clear microwaves passing through the resonators, even if the coupling and internal quality factors are mismatched. With this MKID, our readout system can track resonance frequency changes much more easily. We present the status of the readout system development and demonstrate the performance with the half-wavelength MKID. © Springer Science+Business Media, LLC 2012 |
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Abstract The satellite LiteBIRD (Light satellite for the studies of B-mode polarization and Inflation from cosmic background Radiation Detection) is being designed to detect the B-mode polarization of the cosmic microwave background radiation. LiteBIRD will carry about 2,000 detectors for measurements in five bands (60, 80, 100, 150, and 220 GHz). Microwave kinetic inductance detectors (MKIDs) that can be multiplexed in a single readout line are suitable for the large focal plane detector array. We develop an MKID readout system for LiteBIRD to monitor the amplitude, phase, and resonant frequency of each MKID resonator simultaneously and follow movements of the resonant frequency caused by changes in the input radiation intensity. This mechanism enables us to have a larger dynamic range for the MKIDs, compared with a system that monitors the amplitude and phase on the resonant frequency. We also propose an MKID having a half-wavelength resonator. This MKID transmits the resonant microwave signal from one feedline to another. It can offer clear microwaves passing through the resonators, even if the coupling and internal quality factors are mismatched. With this MKID, our readout system can track resonance frequency changes much more easily. We present the status of the readout system development and demonstrate the performance with the half-wavelength MKID. © Springer Science+Business Media, LLC 2012 |
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Abstract The satellite LiteBIRD (Light satellite for the studies of B-mode polarization and Inflation from cosmic background Radiation Detection) is being designed to detect the B-mode polarization of the cosmic microwave background radiation. LiteBIRD will carry about 2,000 detectors for measurements in five bands (60, 80, 100, 150, and 220 GHz). Microwave kinetic inductance detectors (MKIDs) that can be multiplexed in a single readout line are suitable for the large focal plane detector array. We develop an MKID readout system for LiteBIRD to monitor the amplitude, phase, and resonant frequency of each MKID resonator simultaneously and follow movements of the resonant frequency caused by changes in the input radiation intensity. This mechanism enables us to have a larger dynamic range for the MKIDs, compared with a system that monitors the amplitude and phase on the resonant frequency. We also propose an MKID having a half-wavelength resonator. This MKID transmits the resonant microwave signal from one feedline to another. It can offer clear microwaves passing through the resonators, even if the coupling and internal quality factors are mismatched. With this MKID, our readout system can track resonance frequency changes much more easily. We present the status of the readout system development and demonstrate the performance with the half-wavelength MKID. © Springer Science+Business Media, LLC 2012 |
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