Loading…

HgCdTe APDs for time-resolved space applications

The use of HgCdTe avalanche photodiodes (APDs) for resolving the temporal variation of faint light level signals is analyzed. The analysis is based on the performance characteristics such as the gain, the response time, and dark currents in the APDs, measured as a function of operating temperature a...

Full description

Saved in:
Bibliographic Details
Published in:CEAS space journal 2017-12, Vol.9 (4), p.507-516
Main Authors: Rothman, J., Lasfargues, G., Delacourt, B., Dumas, A., Gibert, F., Bardoux, A., Boutillier, M.
Format: Article
Language:English
Subjects:
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c323t-45ec7ef2f871eb11fb290e9f7490468b6e790563729d4f829da285f817198b953
cites cdi_FETCH-LOGICAL-c323t-45ec7ef2f871eb11fb290e9f7490468b6e790563729d4f829da285f817198b953
container_end_page 516
container_issue 4
container_start_page 507
container_title CEAS space journal
container_volume 9
creator Rothman, J.
Lasfargues, G.
Delacourt, B.
Dumas, A.
Gibert, F.
Bardoux, A.
Boutillier, M.
description The use of HgCdTe avalanche photodiodes (APDs) for resolving the temporal variation of faint light level signals is analyzed. The analysis is based on the performance characteristics such as the gain, the response time, and dark currents in the APDs, measured as a function of operating temperature and Cd composition, and on recently developed detector demonstrator modules. The choice of Cd composition in the APDs is strongly dependent on the application needs in terms of electrical bandwidth and signal-to-noise ratio. A performance model has been developed and used to predict the performance of the future detector modules for different applications such as high bandwidth and/or deep space free space optical telecommunications and lidar, associated with sensitivities down to single photon level at low operating temperature and close to single-photon operation at bandwidth of 10 GHz at room temperature. The predictions are corroborated by the results obtained on detector modules that have been developed and used in lidar and deep space optical communications. In a first lidar prototype, integrating a 200 µm APD, we obtained a maximum sensitivity of 25 fW/√Hz at T  = 190 K operating temperature. The detector has been used for differential absorption lidar estimations of the absorption due to presence of CO 2 in the atmosphere. A random error of 3–10% was obtained for the estimation of the optical thickness at a distance of 100–3000 m, for a range resolution of 100 m and using and averaging time of 4 s. The pursuit of this development is pending on the space qualification of the technology. Results from first proton and irradiation tests are reported that shows on a close to constant performance during and after the irradiation and endurance tests.
doi_str_mv 10.1007/s12567-017-0169-1
format article
fullrecord <record><control><sourceid>crossref_sprin</sourceid><recordid>TN_cdi_crossref_primary_10_1007_s12567_017_0169_1</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>10_1007_s12567_017_0169_1</sourcerecordid><originalsourceid>FETCH-LOGICAL-c323t-45ec7ef2f871eb11fb290e9f7490468b6e790563729d4f829da285f817198b953</originalsourceid><addsrcrecordid>eNp9j01PwzAMhiMEEtPYD-DWPxCw06RJjlP5GNIkOIxz1A9n6tS1VVKQ-Pe0KuK4g-334Mfyw9g9wgMC6MeIQmWaA86VWY5XbIUmM1wohOv_DOKWbWI8AYBACSBxxWB3zOsDJduPp5j4PiRjcyYeKPbtN9VJHIqKkmIY2qYqxqbv4h278UUbafM31-zz5fmQ7_j-_fUt3-55lYp05FJRpckLbzRSiehLYYGs19KCzEyZkbagslQLW0tvpl4Io7xBjdaUVqVrhsvdKvQxBvJuCM25CD8Owc3WbrF2k7WbrR1OjFiYOO12Rwru1H-FbnrzAvQLUNJX7A</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>HgCdTe APDs for time-resolved space applications</title><source>Springer Nature:Jisc Collections:Springer Nature Read and Publish 2023-2025: Springer Reading List</source><creator>Rothman, J. ; Lasfargues, G. ; Delacourt, B. ; Dumas, A. ; Gibert, F. ; Bardoux, A. ; Boutillier, M.</creator><creatorcontrib>Rothman, J. ; Lasfargues, G. ; Delacourt, B. ; Dumas, A. ; Gibert, F. ; Bardoux, A. ; Boutillier, M.</creatorcontrib><description>The use of HgCdTe avalanche photodiodes (APDs) for resolving the temporal variation of faint light level signals is analyzed. The analysis is based on the performance characteristics such as the gain, the response time, and dark currents in the APDs, measured as a function of operating temperature and Cd composition, and on recently developed detector demonstrator modules. The choice of Cd composition in the APDs is strongly dependent on the application needs in terms of electrical bandwidth and signal-to-noise ratio. A performance model has been developed and used to predict the performance of the future detector modules for different applications such as high bandwidth and/or deep space free space optical telecommunications and lidar, associated with sensitivities down to single photon level at low operating temperature and close to single-photon operation at bandwidth of 10 GHz at room temperature. The predictions are corroborated by the results obtained on detector modules that have been developed and used in lidar and deep space optical communications. In a first lidar prototype, integrating a 200 µm APD, we obtained a maximum sensitivity of 25 fW/√Hz at T  = 190 K operating temperature. The detector has been used for differential absorption lidar estimations of the absorption due to presence of CO 2 in the atmosphere. A random error of 3–10% was obtained for the estimation of the optical thickness at a distance of 100–3000 m, for a range resolution of 100 m and using and averaging time of 4 s. The pursuit of this development is pending on the space qualification of the technology. Results from first proton and irradiation tests are reported that shows on a close to constant performance during and after the irradiation and endurance tests.</description><identifier>ISSN: 1868-2502</identifier><identifier>EISSN: 1868-2510</identifier><identifier>DOI: 10.1007/s12567-017-0169-1</identifier><language>eng</language><publisher>Vienna: Springer Vienna</publisher><subject>Aerospace Technology and Astronautics ; Engineering ; Original Paper</subject><ispartof>CEAS space journal, 2017-12, Vol.9 (4), p.507-516</ispartof><rights>CEAS 2017</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c323t-45ec7ef2f871eb11fb290e9f7490468b6e790563729d4f829da285f817198b953</citedby><cites>FETCH-LOGICAL-c323t-45ec7ef2f871eb11fb290e9f7490468b6e790563729d4f829da285f817198b953</cites><orcidid>0000-0003-0916-8961</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27903,27904</link.rule.ids></links><search><creatorcontrib>Rothman, J.</creatorcontrib><creatorcontrib>Lasfargues, G.</creatorcontrib><creatorcontrib>Delacourt, B.</creatorcontrib><creatorcontrib>Dumas, A.</creatorcontrib><creatorcontrib>Gibert, F.</creatorcontrib><creatorcontrib>Bardoux, A.</creatorcontrib><creatorcontrib>Boutillier, M.</creatorcontrib><title>HgCdTe APDs for time-resolved space applications</title><title>CEAS space journal</title><addtitle>CEAS Space J</addtitle><description>The use of HgCdTe avalanche photodiodes (APDs) for resolving the temporal variation of faint light level signals is analyzed. The analysis is based on the performance characteristics such as the gain, the response time, and dark currents in the APDs, measured as a function of operating temperature and Cd composition, and on recently developed detector demonstrator modules. The choice of Cd composition in the APDs is strongly dependent on the application needs in terms of electrical bandwidth and signal-to-noise ratio. A performance model has been developed and used to predict the performance of the future detector modules for different applications such as high bandwidth and/or deep space free space optical telecommunications and lidar, associated with sensitivities down to single photon level at low operating temperature and close to single-photon operation at bandwidth of 10 GHz at room temperature. The predictions are corroborated by the results obtained on detector modules that have been developed and used in lidar and deep space optical communications. In a first lidar prototype, integrating a 200 µm APD, we obtained a maximum sensitivity of 25 fW/√Hz at T  = 190 K operating temperature. The detector has been used for differential absorption lidar estimations of the absorption due to presence of CO 2 in the atmosphere. A random error of 3–10% was obtained for the estimation of the optical thickness at a distance of 100–3000 m, for a range resolution of 100 m and using and averaging time of 4 s. The pursuit of this development is pending on the space qualification of the technology. Results from first proton and irradiation tests are reported that shows on a close to constant performance during and after the irradiation and endurance tests.</description><subject>Aerospace Technology and Astronautics</subject><subject>Engineering</subject><subject>Original Paper</subject><issn>1868-2502</issn><issn>1868-2510</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><recordid>eNp9j01PwzAMhiMEEtPYD-DWPxCw06RJjlP5GNIkOIxz1A9n6tS1VVKQ-Pe0KuK4g-334Mfyw9g9wgMC6MeIQmWaA86VWY5XbIUmM1wohOv_DOKWbWI8AYBACSBxxWB3zOsDJduPp5j4PiRjcyYeKPbtN9VJHIqKkmIY2qYqxqbv4h278UUbafM31-zz5fmQ7_j-_fUt3-55lYp05FJRpckLbzRSiehLYYGs19KCzEyZkbagslQLW0tvpl4Io7xBjdaUVqVrhsvdKvQxBvJuCM25CD8Owc3WbrF2k7WbrR1OjFiYOO12Rwru1H-FbnrzAvQLUNJX7A</recordid><startdate>20171201</startdate><enddate>20171201</enddate><creator>Rothman, J.</creator><creator>Lasfargues, G.</creator><creator>Delacourt, B.</creator><creator>Dumas, A.</creator><creator>Gibert, F.</creator><creator>Bardoux, A.</creator><creator>Boutillier, M.</creator><general>Springer Vienna</general><scope>AAYXX</scope><scope>CITATION</scope><orcidid>https://orcid.org/0000-0003-0916-8961</orcidid></search><sort><creationdate>20171201</creationdate><title>HgCdTe APDs for time-resolved space applications</title><author>Rothman, J. ; Lasfargues, G. ; Delacourt, B. ; Dumas, A. ; Gibert, F. ; Bardoux, A. ; Boutillier, M.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c323t-45ec7ef2f871eb11fb290e9f7490468b6e790563729d4f829da285f817198b953</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Aerospace Technology and Astronautics</topic><topic>Engineering</topic><topic>Original Paper</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Rothman, J.</creatorcontrib><creatorcontrib>Lasfargues, G.</creatorcontrib><creatorcontrib>Delacourt, B.</creatorcontrib><creatorcontrib>Dumas, A.</creatorcontrib><creatorcontrib>Gibert, F.</creatorcontrib><creatorcontrib>Bardoux, A.</creatorcontrib><creatorcontrib>Boutillier, M.</creatorcontrib><collection>CrossRef</collection><jtitle>CEAS space journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Rothman, J.</au><au>Lasfargues, G.</au><au>Delacourt, B.</au><au>Dumas, A.</au><au>Gibert, F.</au><au>Bardoux, A.</au><au>Boutillier, M.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>HgCdTe APDs for time-resolved space applications</atitle><jtitle>CEAS space journal</jtitle><stitle>CEAS Space J</stitle><date>2017-12-01</date><risdate>2017</risdate><volume>9</volume><issue>4</issue><spage>507</spage><epage>516</epage><pages>507-516</pages><issn>1868-2502</issn><eissn>1868-2510</eissn><abstract>The use of HgCdTe avalanche photodiodes (APDs) for resolving the temporal variation of faint light level signals is analyzed. The analysis is based on the performance characteristics such as the gain, the response time, and dark currents in the APDs, measured as a function of operating temperature and Cd composition, and on recently developed detector demonstrator modules. The choice of Cd composition in the APDs is strongly dependent on the application needs in terms of electrical bandwidth and signal-to-noise ratio. A performance model has been developed and used to predict the performance of the future detector modules for different applications such as high bandwidth and/or deep space free space optical telecommunications and lidar, associated with sensitivities down to single photon level at low operating temperature and close to single-photon operation at bandwidth of 10 GHz at room temperature. The predictions are corroborated by the results obtained on detector modules that have been developed and used in lidar and deep space optical communications. In a first lidar prototype, integrating a 200 µm APD, we obtained a maximum sensitivity of 25 fW/√Hz at T  = 190 K operating temperature. The detector has been used for differential absorption lidar estimations of the absorption due to presence of CO 2 in the atmosphere. A random error of 3–10% was obtained for the estimation of the optical thickness at a distance of 100–3000 m, for a range resolution of 100 m and using and averaging time of 4 s. The pursuit of this development is pending on the space qualification of the technology. Results from first proton and irradiation tests are reported that shows on a close to constant performance during and after the irradiation and endurance tests.</abstract><cop>Vienna</cop><pub>Springer Vienna</pub><doi>10.1007/s12567-017-0169-1</doi><tpages>10</tpages><orcidid>https://orcid.org/0000-0003-0916-8961</orcidid></addata></record>
fulltext fulltext
identifier ISSN: 1868-2502
ispartof CEAS space journal, 2017-12, Vol.9 (4), p.507-516
issn 1868-2502
1868-2510
language eng
recordid cdi_crossref_primary_10_1007_s12567_017_0169_1
source Springer Nature:Jisc Collections:Springer Nature Read and Publish 2023-2025: Springer Reading List
subjects Aerospace Technology and Astronautics
Engineering
Original Paper
title HgCdTe APDs for time-resolved space applications
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-23T01%3A05%3A17IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-crossref_sprin&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=HgCdTe%20APDs%20for%20time-resolved%20space%20applications&rft.jtitle=CEAS%20space%20journal&rft.au=Rothman,%20J.&rft.date=2017-12-01&rft.volume=9&rft.issue=4&rft.spage=507&rft.epage=516&rft.pages=507-516&rft.issn=1868-2502&rft.eissn=1868-2510&rft_id=info:doi/10.1007/s12567-017-0169-1&rft_dat=%3Ccrossref_sprin%3E10_1007_s12567_017_0169_1%3C/crossref_sprin%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c323t-45ec7ef2f871eb11fb290e9f7490468b6e790563729d4f829da285f817198b953%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true