Design of a Ultra-Stable Low-Noise Space Camera Based on a Large Target CMOS Detector and Image Data Analysis

To detect faint target stars of 22nd magnitude and above, an astronomical exploration project requires its space camera’s readout noise to be less than 5e<sup<−</sup< with long-time working stability. Due to the limitation of satellite, the traditional CCD detector-based camera does not...
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Autor*in:	Chao Shen [verfasserIn] Caiwen Ma [verfasserIn] Wei Gao [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2022

Schlagwörter:	CMOS detector space camera low readout noise ultra-stable image data analysis

Übergeordnetes Werk:	In: Sensors - MDPI AG, 2003, 22(2022), 24, p 9991
Übergeordnetes Werk:	volume:22 ; year:2022 ; number:24, p 9991

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3390/s22249991

Katalog-ID:	DOAJ082979502

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spelling	10.3390/s22249991 doi (DE-627)DOAJ082979502 (DE-599)DOAJ043ab9317a1c415a8f64ad130141c247 DE-627 ger DE-627 rakwb eng TP1-1185 Chao Shen verfasserin aut Design of a Ultra-Stable Low-Noise Space Camera Based on a Large Target CMOS Detector and Image Data Analysis 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier To detect faint target stars of 22nd magnitude and above, an astronomical exploration project requires its space camera’s readout noise to be less than 5e<sup<−</sup< with long-time working stability. Due to the limitation of satellite, the traditional CCD detector-based camera does not meet the requirements, including volume, weight, and power consumption. Thereby, a low-noise ultra-stable camera based on 9 K × 9 K large target surface CMOS is designed to meet the needs. For the first time, the low-noise ultra-stable camera based on CMOS detector will be applied to space astronomy projects, remote sensing imaging, resource survey, atmospheric and oceanic observation and other fields. In this paper, the design of the camera is introduced in detail, and the camera is tested for several rounds at −40 °C; it also undergoes further testing and data analysis. Tests proved super stability and that the readout noise is lower than 4.5e<sup<−</sup<. Dark current, nonlinearity and PTC indicators meet the requirements of the astronomical exploration project. CMOS detector space camera low readout noise ultra-stable image data analysis Chemical technology Caiwen Ma verfasserin aut Wei Gao verfasserin aut In Sensors MDPI AG, 2003 22(2022), 24, p 9991 (DE-627)331640910 (DE-600)2052857-7 14248220 nnns volume:22 year:2022 number:24, p 9991 https://doi.org/10.3390/s22249991 kostenfrei https://doaj.org/article/043ab9317a1c415a8f64ad130141c247 kostenfrei https://www.mdpi.com/1424-8220/22/24/9991 kostenfrei https://doaj.org/toc/1424-8220 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2111 GBV_ILN_2507 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 22 2022 24, p 9991
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allfieldsSound	10.3390/s22249991 doi (DE-627)DOAJ082979502 (DE-599)DOAJ043ab9317a1c415a8f64ad130141c247 DE-627 ger DE-627 rakwb eng TP1-1185 Chao Shen verfasserin aut Design of a Ultra-Stable Low-Noise Space Camera Based on a Large Target CMOS Detector and Image Data Analysis 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier To detect faint target stars of 22nd magnitude and above, an astronomical exploration project requires its space camera’s readout noise to be less than 5e<sup<−</sup< with long-time working stability. Due to the limitation of satellite, the traditional CCD detector-based camera does not meet the requirements, including volume, weight, and power consumption. Thereby, a low-noise ultra-stable camera based on 9 K × 9 K large target surface CMOS is designed to meet the needs. For the first time, the low-noise ultra-stable camera based on CMOS detector will be applied to space astronomy projects, remote sensing imaging, resource survey, atmospheric and oceanic observation and other fields. In this paper, the design of the camera is introduced in detail, and the camera is tested for several rounds at −40 °C; it also undergoes further testing and data analysis. Tests proved super stability and that the readout noise is lower than 4.5e<sup<−</sup<. Dark current, nonlinearity and PTC indicators meet the requirements of the astronomical exploration project. CMOS detector space camera low readout noise ultra-stable image data analysis Chemical technology Caiwen Ma verfasserin aut Wei Gao verfasserin aut In Sensors MDPI AG, 2003 22(2022), 24, p 9991 (DE-627)331640910 (DE-600)2052857-7 14248220 nnns volume:22 year:2022 number:24, p 9991 https://doi.org/10.3390/s22249991 kostenfrei https://doaj.org/article/043ab9317a1c415a8f64ad130141c247 kostenfrei https://www.mdpi.com/1424-8220/22/24/9991 kostenfrei https://doaj.org/toc/1424-8220 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2111 GBV_ILN_2507 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 22 2022 24, p 9991
language	English
source	In Sensors 22(2022), 24, p 9991 volume:22 year:2022 number:24, p 9991
sourceStr	In Sensors 22(2022), 24, p 9991 volume:22 year:2022 number:24, p 9991
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	CMOS detector space camera low readout noise ultra-stable image data analysis Chemical technology
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container_title	Sensors
authorswithroles_txt_mv	Chao Shen @@aut@@ Caiwen Ma @@aut@@ Wei Gao @@aut@@
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callnumber-first	T - Technology
author	Chao Shen
spellingShingle	Chao Shen misc TP1-1185 misc CMOS detector misc space camera misc low readout noise misc ultra-stable misc image data analysis misc Chemical technology Design of a Ultra-Stable Low-Noise Space Camera Based on a Large Target CMOS Detector and Image Data Analysis
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topic_title	TP1-1185 Design of a Ultra-Stable Low-Noise Space Camera Based on a Large Target CMOS Detector and Image Data Analysis CMOS detector space camera low readout noise ultra-stable image data analysis
topic	misc TP1-1185 misc CMOS detector misc space camera misc low readout noise misc ultra-stable misc image data analysis misc Chemical technology
topic_unstemmed	misc TP1-1185 misc CMOS detector misc space camera misc low readout noise misc ultra-stable misc image data analysis misc Chemical technology
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title	Design of a Ultra-Stable Low-Noise Space Camera Based on a Large Target CMOS Detector and Image Data Analysis
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title_sort	design of a ultra-stable low-noise space camera based on a large target cmos detector and image data analysis
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title_auth	Design of a Ultra-Stable Low-Noise Space Camera Based on a Large Target CMOS Detector and Image Data Analysis
abstract	To detect faint target stars of 22nd magnitude and above, an astronomical exploration project requires its space camera’s readout noise to be less than 5e<sup<−</sup< with long-time working stability. Due to the limitation of satellite, the traditional CCD detector-based camera does not meet the requirements, including volume, weight, and power consumption. Thereby, a low-noise ultra-stable camera based on 9 K × 9 K large target surface CMOS is designed to meet the needs. For the first time, the low-noise ultra-stable camera based on CMOS detector will be applied to space astronomy projects, remote sensing imaging, resource survey, atmospheric and oceanic observation and other fields. In this paper, the design of the camera is introduced in detail, and the camera is tested for several rounds at −40 °C; it also undergoes further testing and data analysis. Tests proved super stability and that the readout noise is lower than 4.5e<sup<−</sup<. Dark current, nonlinearity and PTC indicators meet the requirements of the astronomical exploration project.
abstractGer	To detect faint target stars of 22nd magnitude and above, an astronomical exploration project requires its space camera’s readout noise to be less than 5e<sup<−</sup< with long-time working stability. Due to the limitation of satellite, the traditional CCD detector-based camera does not meet the requirements, including volume, weight, and power consumption. Thereby, a low-noise ultra-stable camera based on 9 K × 9 K large target surface CMOS is designed to meet the needs. For the first time, the low-noise ultra-stable camera based on CMOS detector will be applied to space astronomy projects, remote sensing imaging, resource survey, atmospheric and oceanic observation and other fields. In this paper, the design of the camera is introduced in detail, and the camera is tested for several rounds at −40 °C; it also undergoes further testing and data analysis. Tests proved super stability and that the readout noise is lower than 4.5e<sup<−</sup<. Dark current, nonlinearity and PTC indicators meet the requirements of the astronomical exploration project.
abstract_unstemmed	To detect faint target stars of 22nd magnitude and above, an astronomical exploration project requires its space camera’s readout noise to be less than 5e<sup<−</sup< with long-time working stability. Due to the limitation of satellite, the traditional CCD detector-based camera does not meet the requirements, including volume, weight, and power consumption. Thereby, a low-noise ultra-stable camera based on 9 K × 9 K large target surface CMOS is designed to meet the needs. For the first time, the low-noise ultra-stable camera based on CMOS detector will be applied to space astronomy projects, remote sensing imaging, resource survey, atmospheric and oceanic observation and other fields. In this paper, the design of the camera is introduced in detail, and the camera is tested for several rounds at −40 °C; it also undergoes further testing and data analysis. Tests proved super stability and that the readout noise is lower than 4.5e<sup<−</sup<. Dark current, nonlinearity and PTC indicators meet the requirements of the astronomical exploration project.
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title_short	Design of a Ultra-Stable Low-Noise Space Camera Based on a Large Target CMOS Detector and Image Data Analysis
url	https://doi.org/10.3390/s22249991 https://doaj.org/article/043ab9317a1c415a8f64ad130141c247 https://www.mdpi.com/1424-8220/22/24/9991 https://doaj.org/toc/1424-8220
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