Photon Counting Based on Solar-Blind Ultraviolet Intensified Complementary Metal-Oxide-Semiconductor (ICMOS) for Corona Detection
For the detection of weak signals, photon counting technology has attracted much attention. In this paper, a method based on photon counting is experimentally demonstrated to realize corona discharge detection at solar-blind ultraviolet (UV) wavelength. In our setup, a solar-blind UV optical filter...
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description | For the detection of weak signals, photon counting technology has attracted much attention. In this paper, a method based on photon counting is experimentally demonstrated to realize corona discharge detection at solar-blind ultraviolet (UV) wavelength. In our setup, a solar-blind UV optical filter and a Te-Cs cathode are used to eliminate the effects of light with undesired wavelengths, i.e., outside of the solar-blind band. A two-stage microchannel plate with a high voltage can achieve a gain of up to 10 6 . A phosphor screen coupled with a CMOS can capture complete images without image distortion. By using an ICMOS, the setup can detect single-photon events. Then, applying photon counting statistics, a theoretical probability model of the photon numbers is obtained. Meanwhile, through analyzing the structure of the photon events considering both pixel and temporal resolution, two photon counting algorithms are proposed. Through experiments with an UV light source, the algorithm based on temporal resolution is proved to be more accurate. Finally, through an experiment with a corona discharge device, a solar-blind photon counting image is captured, and the photon number is calculated through the proposed counting algorithm. The probability curve of the practical photon numbers is acquired via several experiments carried out at the same conditions, which proves the accuracy of the setup and algorithm when compared with the theoretical probability model. Therefore, the proposed method can provide a scientific evaluation for corona detection. |
doi_str_mv | 10.1109/JPHOT.2018.2876514 |
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In this paper, a method based on photon counting is experimentally demonstrated to realize corona discharge detection at solar-blind ultraviolet (UV) wavelength. In our setup, a solar-blind UV optical filter and a Te-Cs cathode are used to eliminate the effects of light with undesired wavelengths, i.e., outside of the solar-blind band. A two-stage microchannel plate with a high voltage can achieve a gain of up to 10 6 . A phosphor screen coupled with a CMOS can capture complete images without image distortion. By using an ICMOS, the setup can detect single-photon events. Then, applying photon counting statistics, a theoretical probability model of the photon numbers is obtained. Meanwhile, through analyzing the structure of the photon events considering both pixel and temporal resolution, two photon counting algorithms are proposed. Through experiments with an UV light source, the algorithm based on temporal resolution is proved to be more accurate. Finally, through an experiment with a corona discharge device, a solar-blind photon counting image is captured, and the photon number is calculated through the proposed counting algorithm. The probability curve of the practical photon numbers is acquired via several experiments carried out at the same conditions, which proves the accuracy of the setup and algorithm when compared with the theoretical probability model. Therefore, the proposed method can provide a scientific evaluation for corona detection.</description><identifier>ISSN: 1943-0655</identifier><identifier>EISSN: 1943-0647</identifier><identifier>DOI: 10.1109/JPHOT.2018.2876514</identifier><identifier>CODEN: PJHOC3</identifier><language>eng</language><publisher>Piscataway: IEEE</publisher><subject>Algorithms ; Cathodes ; CMOS ; Corona ; Discharge ; High voltages ; Image analysis ; Image detection ; Image intensifiers ; imaging system ; Lenses ; Metal oxide semiconductors ; Microchannel plates ; Microchannels ; Optical filters ; Phosphors ; photon counting ; Photonics ; Plates (structural members) ; Solar corona ; Stellar coronas ; Temporal resolution ; Ultraviolet radiation</subject><ispartof>IEEE photonics journal, 2018-12, Vol.10 (6), p.1-19</ispartof><rights>Copyright The Institute of Electrical and Electronics Engineers, Inc. (IEEE) 2018</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c454t-7d7b66e1af68823374d8f6b71007d02fde69400168f2f96ddfbb2b09b62d0d833</citedby><cites>FETCH-LOGICAL-c454t-7d7b66e1af68823374d8f6b71007d02fde69400168f2f96ddfbb2b09b62d0d833</cites><orcidid>0000-0002-7397-3597 ; 0000-0002-5471-3220</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://ieeexplore.ieee.org/document/8494829$$EHTML$$P50$$Gieee$$Hfree_for_read</linktohtml><link.rule.ids>314,780,784,864,2102,27633,27924,27925,54933</link.rule.ids></links><search><creatorcontrib>Wang, Yan</creatorcontrib><creatorcontrib>Qian, Yunsheng</creatorcontrib><creatorcontrib>Kong, Xiangyu</creatorcontrib><title>Photon Counting Based on Solar-Blind Ultraviolet Intensified Complementary Metal-Oxide-Semiconductor (ICMOS) for Corona Detection</title><title>IEEE photonics journal</title><addtitle>JPHOT</addtitle><description>For the detection of weak signals, photon counting technology has attracted much attention. In this paper, a method based on photon counting is experimentally demonstrated to realize corona discharge detection at solar-blind ultraviolet (UV) wavelength. In our setup, a solar-blind UV optical filter and a Te-Cs cathode are used to eliminate the effects of light with undesired wavelengths, i.e., outside of the solar-blind band. A two-stage microchannel plate with a high voltage can achieve a gain of up to 10 6 . A phosphor screen coupled with a CMOS can capture complete images without image distortion. By using an ICMOS, the setup can detect single-photon events. Then, applying photon counting statistics, a theoretical probability model of the photon numbers is obtained. Meanwhile, through analyzing the structure of the photon events considering both pixel and temporal resolution, two photon counting algorithms are proposed. Through experiments with an UV light source, the algorithm based on temporal resolution is proved to be more accurate. Finally, through an experiment with a corona discharge device, a solar-blind photon counting image is captured, and the photon number is calculated through the proposed counting algorithm. The probability curve of the practical photon numbers is acquired via several experiments carried out at the same conditions, which proves the accuracy of the setup and algorithm when compared with the theoretical probability model. Therefore, the proposed method can provide a scientific evaluation for corona detection.</description><subject>Algorithms</subject><subject>Cathodes</subject><subject>CMOS</subject><subject>Corona</subject><subject>Discharge</subject><subject>High voltages</subject><subject>Image analysis</subject><subject>Image detection</subject><subject>Image intensifiers</subject><subject>imaging system</subject><subject>Lenses</subject><subject>Metal oxide semiconductors</subject><subject>Microchannel plates</subject><subject>Microchannels</subject><subject>Optical filters</subject><subject>Phosphors</subject><subject>photon counting</subject><subject>Photonics</subject><subject>Plates (structural members)</subject><subject>Solar corona</subject><subject>Stellar coronas</subject><subject>Temporal resolution</subject><subject>Ultraviolet radiation</subject><issn>1943-0655</issn><issn>1943-0647</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><sourceid>ESBDL</sourceid><sourceid>RIE</sourceid><sourceid>DOA</sourceid><recordid>eNo9UUtvEzEYXCEqUVr-AFwscYHDBr_WjyNdHg1qlUppz5Z3_bk42tjB61TlyD_HbaqcvtFoZr6RpmneE7wgBOsvv24uV7cLiolaUCVFR_ir5pRozlosuHx9xF33pnk7zxuMhSadPm3-3fxOJUXUp30sId6jCzuDQ5VZp8nm9mIK0aG7qWT7ENIEBS1jgTgHH6qsT9vdBFuIxea_6BqKndrVY3DQrmEbxhTdfiwpo0_L_nq1_ox8xX3KKVr0DQqMJaR43px4O83w7uWeNXc_vt_2l-3V6uey_3rVjrzjpZVODkIAsV4oRRmT3CkvBkkwlg5T70BojjERylOvhXN-GOiA9SCow04xdtYsD7ku2Y3Z5bCtnU2ywTwTKd8bm0sYJzDCUalHNSirBcdDxdIxP3LLuOTKQc36eMja5fRnD3Mxm7TPsdY3lDAssCBMVBU9qMac5jmDP34l2DzNZp5nM0-zmZfZqunDwRQA4GhQXHNFNfsP7ESUaw</recordid><startdate>20181201</startdate><enddate>20181201</enddate><creator>Wang, Yan</creator><creator>Qian, Yunsheng</creator><creator>Kong, Xiangyu</creator><general>IEEE</general><general>The Institute of Electrical and Electronics Engineers, Inc. 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In this paper, a method based on photon counting is experimentally demonstrated to realize corona discharge detection at solar-blind ultraviolet (UV) wavelength. In our setup, a solar-blind UV optical filter and a Te-Cs cathode are used to eliminate the effects of light with undesired wavelengths, i.e., outside of the solar-blind band. A two-stage microchannel plate with a high voltage can achieve a gain of up to 10 6 . A phosphor screen coupled with a CMOS can capture complete images without image distortion. By using an ICMOS, the setup can detect single-photon events. Then, applying photon counting statistics, a theoretical probability model of the photon numbers is obtained. Meanwhile, through analyzing the structure of the photon events considering both pixel and temporal resolution, two photon counting algorithms are proposed. Through experiments with an UV light source, the algorithm based on temporal resolution is proved to be more accurate. Finally, through an experiment with a corona discharge device, a solar-blind photon counting image is captured, and the photon number is calculated through the proposed counting algorithm. The probability curve of the practical photon numbers is acquired via several experiments carried out at the same conditions, which proves the accuracy of the setup and algorithm when compared with the theoretical probability model. Therefore, the proposed method can provide a scientific evaluation for corona detection.</abstract><cop>Piscataway</cop><pub>IEEE</pub><doi>10.1109/JPHOT.2018.2876514</doi><tpages>19</tpages><orcidid>https://orcid.org/0000-0002-7397-3597</orcidid><orcidid>https://orcid.org/0000-0002-5471-3220</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Algorithms Cathodes CMOS Corona Discharge High voltages Image analysis Image detection Image intensifiers imaging system Lenses Metal oxide semiconductors Microchannel plates Microchannels Optical filters Phosphors photon counting Photonics Plates (structural members) Solar corona Stellar coronas Temporal resolution Ultraviolet radiation |
title | Photon Counting Based on Solar-Blind Ultraviolet Intensified Complementary Metal-Oxide-Semiconductor (ICMOS) for Corona Detection |
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