Loading…

Response of X‐UV photodiodes to 1.5–17.5 keV x rays and MeV alpha particles

The absolute x‐ray response of three X‐UV photodiodes was measured over an energy range of 1.5–17.5 keV so that they could be used to calibrate x‐ray imaging systems for the ASCA satellite mission. An intense electron‐beam x‐ray generator was used to test both the dc and ac x‐ray response at 1.5, 4....

Full description

Saved in:
Bibliographic Details
Published in:Review of scientific instruments 1993-07, Vol.64 (7), p.1723-1733
Main Authors: Wenzel, Kevin W., Li, Chi‐Kang, Petrasso, Richard D., Lo, Daniel H., Bautz, Marshall W., Ricker, George R., Hsieh, Ed
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-c326t-90a0bc60be8995926e63c2d973ef62ba80a1d4ba6ed6ad6f665622a372f8064a3
cites cdi_FETCH-LOGICAL-c326t-90a0bc60be8995926e63c2d973ef62ba80a1d4ba6ed6ad6f665622a372f8064a3
container_end_page 1733
container_issue 7
container_start_page 1723
container_title Review of scientific instruments
container_volume 64
creator Wenzel, Kevin W.
Li, Chi‐Kang
Petrasso, Richard D.
Lo, Daniel H.
Bautz, Marshall W.
Ricker, George R.
Hsieh, Ed
description The absolute x‐ray response of three X‐UV photodiodes was measured over an energy range of 1.5–17.5 keV so that they could be used to calibrate x‐ray imaging systems for the ASCA satellite mission. An intense electron‐beam x‐ray generator was used to test both the dc and ac x‐ray response at 1.5, 4.5, 8.0, and 17.5 keV, and an 55Fe source was used to examine one of the photodiodes at 5.9 keV. The x‐ray response was determined by comparing the X‐UV diode signal to that of a previously calibrated silicon surface barrier diode (SBD). The X‐UV detector response was similar to the SBD response at low energies (1.5 and 4.5 keV). At 8 keV, the X‐UV detectors exhibited about 70% of the SBD response, and at 17.5 keV, about 50%. This result is surprising, because the X‐UV diodes actually have a greater silicon thickness than the SBD. In contrast to our findings for SBDs in the past, this implies that not the entire physical volume of these detectors comprises the active volume. The X‐UV detector x‐ray response was also examined as a function of the applied bias voltage. No significant bias voltage dependence of the x‐ray signal was found, which indicates that the depletion layer thickness does not determine the active volume either. However, the detector noise was found to decrease substantially as the applied bias was raised from zero to a few volts. Response of these detectors, operated in pulse mode, to 226Ra α particles indicated large charge carrier recombination in the bulk silicon. This feature renders these detectors unsuitable for most charged‐particle spectroscopy applications.
doi_str_mv 10.1063/1.1144000
format article
fullrecord <record><control><sourceid>scitation_pasca</sourceid><recordid>TN_cdi_scitation_primary_10_1063_1_1144000</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>rsi</sourcerecordid><originalsourceid>FETCH-LOGICAL-c326t-90a0bc60be8995926e63c2d973ef62ba80a1d4ba6ed6ad6f665622a372f8064a3</originalsourceid><addsrcrecordid>eNp90MtKw0AUBuBBFKzVhW8wCzcKiXPLJFlK8QaVgtjiLpzMhUZjZpgJYnd9BME37JPY0qILwdXhwHd-Dj9Cp5SklEh-SVNKhSCE7KEBJUWZ5JLxfTQghItE5qI4REcxvqwBySgdoMmjid510WBn8fNq-TmdYT93vdON0ybi3mGaZqvlF83TDL-aGf7AARYRQ6fxw3qF1s8Bewh9o1oTj9GBhTaak90counN9dPoLhlPbu9HV-NEcSb7pCRAaiVJbYqyzEomjeSK6TLnxkpWQ0GAalGDNFqCllbKTDIGPGe2IFIAH6Lzba4KLsZgbOVD8wZhUVFSbZqoaLVrYm3PttZDVNDaAJ1q4s-BKDLB8g272LKomh76xnU_5N2F37zKa_sf_vvAN4r4eEo</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Response of X‐UV photodiodes to 1.5–17.5 keV x rays and MeV alpha particles</title><source>American Institute of Physics (AIP) Publications</source><source>AIP Digital Archive</source><creator>Wenzel, Kevin W. ; Li, Chi‐Kang ; Petrasso, Richard D. ; Lo, Daniel H. ; Bautz, Marshall W. ; Ricker, George R. ; Hsieh, Ed</creator><creatorcontrib>Wenzel, Kevin W. ; Li, Chi‐Kang ; Petrasso, Richard D. ; Lo, Daniel H. ; Bautz, Marshall W. ; Ricker, George R. ; Hsieh, Ed</creatorcontrib><description>The absolute x‐ray response of three X‐UV photodiodes was measured over an energy range of 1.5–17.5 keV so that they could be used to calibrate x‐ray imaging systems for the ASCA satellite mission. An intense electron‐beam x‐ray generator was used to test both the dc and ac x‐ray response at 1.5, 4.5, 8.0, and 17.5 keV, and an 55Fe source was used to examine one of the photodiodes at 5.9 keV. The x‐ray response was determined by comparing the X‐UV diode signal to that of a previously calibrated silicon surface barrier diode (SBD). The X‐UV detector response was similar to the SBD response at low energies (1.5 and 4.5 keV). At 8 keV, the X‐UV detectors exhibited about 70% of the SBD response, and at 17.5 keV, about 50%. This result is surprising, because the X‐UV diodes actually have a greater silicon thickness than the SBD. In contrast to our findings for SBDs in the past, this implies that not the entire physical volume of these detectors comprises the active volume. The X‐UV detector x‐ray response was also examined as a function of the applied bias voltage. No significant bias voltage dependence of the x‐ray signal was found, which indicates that the depletion layer thickness does not determine the active volume either. However, the detector noise was found to decrease substantially as the applied bias was raised from zero to a few volts. Response of these detectors, operated in pulse mode, to 226Ra α particles indicated large charge carrier recombination in the bulk silicon. This feature renders these detectors unsuitable for most charged‐particle spectroscopy applications.</description><identifier>ISSN: 0034-6748</identifier><identifier>EISSN: 1089-7623</identifier><identifier>DOI: 10.1063/1.1144000</identifier><identifier>CODEN: RSINAK</identifier><language>eng</language><publisher>Woodbury, NY: American Institute of Physics</publisher><subject>Exact sciences and technology ; Instruments, apparatus, components and techniques common to several branches of physics and astronomy ; Physics ; X- and γ-ray instruments and techniques</subject><ispartof>Review of scientific instruments, 1993-07, Vol.64 (7), p.1723-1733</ispartof><rights>American Institute of Physics</rights><rights>1993 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c326t-90a0bc60be8995926e63c2d973ef62ba80a1d4ba6ed6ad6f665622a372f8064a3</citedby><cites>FETCH-LOGICAL-c326t-90a0bc60be8995926e63c2d973ef62ba80a1d4ba6ed6ad6f665622a372f8064a3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://pubs.aip.org/rsi/article-lookup/doi/10.1063/1.1144000$$EHTML$$P50$$Gscitation$$H</linktohtml><link.rule.ids>314,780,782,784,795,1559,27924,27925,76383,76390</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&amp;idt=4854270$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Wenzel, Kevin W.</creatorcontrib><creatorcontrib>Li, Chi‐Kang</creatorcontrib><creatorcontrib>Petrasso, Richard D.</creatorcontrib><creatorcontrib>Lo, Daniel H.</creatorcontrib><creatorcontrib>Bautz, Marshall W.</creatorcontrib><creatorcontrib>Ricker, George R.</creatorcontrib><creatorcontrib>Hsieh, Ed</creatorcontrib><title>Response of X‐UV photodiodes to 1.5–17.5 keV x rays and MeV alpha particles</title><title>Review of scientific instruments</title><description>The absolute x‐ray response of three X‐UV photodiodes was measured over an energy range of 1.5–17.5 keV so that they could be used to calibrate x‐ray imaging systems for the ASCA satellite mission. An intense electron‐beam x‐ray generator was used to test both the dc and ac x‐ray response at 1.5, 4.5, 8.0, and 17.5 keV, and an 55Fe source was used to examine one of the photodiodes at 5.9 keV. The x‐ray response was determined by comparing the X‐UV diode signal to that of a previously calibrated silicon surface barrier diode (SBD). The X‐UV detector response was similar to the SBD response at low energies (1.5 and 4.5 keV). At 8 keV, the X‐UV detectors exhibited about 70% of the SBD response, and at 17.5 keV, about 50%. This result is surprising, because the X‐UV diodes actually have a greater silicon thickness than the SBD. In contrast to our findings for SBDs in the past, this implies that not the entire physical volume of these detectors comprises the active volume. The X‐UV detector x‐ray response was also examined as a function of the applied bias voltage. No significant bias voltage dependence of the x‐ray signal was found, which indicates that the depletion layer thickness does not determine the active volume either. However, the detector noise was found to decrease substantially as the applied bias was raised from zero to a few volts. Response of these detectors, operated in pulse mode, to 226Ra α particles indicated large charge carrier recombination in the bulk silicon. This feature renders these detectors unsuitable for most charged‐particle spectroscopy applications.</description><subject>Exact sciences and technology</subject><subject>Instruments, apparatus, components and techniques common to several branches of physics and astronomy</subject><subject>Physics</subject><subject>X- and γ-ray instruments and techniques</subject><issn>0034-6748</issn><issn>1089-7623</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1993</creationdate><recordtype>article</recordtype><recordid>eNp90MtKw0AUBuBBFKzVhW8wCzcKiXPLJFlK8QaVgtjiLpzMhUZjZpgJYnd9BME37JPY0qILwdXhwHd-Dj9Cp5SklEh-SVNKhSCE7KEBJUWZ5JLxfTQghItE5qI4REcxvqwBySgdoMmjid510WBn8fNq-TmdYT93vdON0ybi3mGaZqvlF83TDL-aGf7AARYRQ6fxw3qF1s8Bewh9o1oTj9GBhTaak90counN9dPoLhlPbu9HV-NEcSb7pCRAaiVJbYqyzEomjeSK6TLnxkpWQ0GAalGDNFqCllbKTDIGPGe2IFIAH6Lzba4KLsZgbOVD8wZhUVFSbZqoaLVrYm3PttZDVNDaAJ1q4s-BKDLB8g272LKomh76xnU_5N2F37zKa_sf_vvAN4r4eEo</recordid><startdate>19930701</startdate><enddate>19930701</enddate><creator>Wenzel, Kevin W.</creator><creator>Li, Chi‐Kang</creator><creator>Petrasso, Richard D.</creator><creator>Lo, Daniel H.</creator><creator>Bautz, Marshall W.</creator><creator>Ricker, George R.</creator><creator>Hsieh, Ed</creator><general>American Institute of Physics</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>19930701</creationdate><title>Response of X‐UV photodiodes to 1.5–17.5 keV x rays and MeV alpha particles</title><author>Wenzel, Kevin W. ; Li, Chi‐Kang ; Petrasso, Richard D. ; Lo, Daniel H. ; Bautz, Marshall W. ; Ricker, George R. ; Hsieh, Ed</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c326t-90a0bc60be8995926e63c2d973ef62ba80a1d4ba6ed6ad6f665622a372f8064a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1993</creationdate><topic>Exact sciences and technology</topic><topic>Instruments, apparatus, components and techniques common to several branches of physics and astronomy</topic><topic>Physics</topic><topic>X- and γ-ray instruments and techniques</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Wenzel, Kevin W.</creatorcontrib><creatorcontrib>Li, Chi‐Kang</creatorcontrib><creatorcontrib>Petrasso, Richard D.</creatorcontrib><creatorcontrib>Lo, Daniel H.</creatorcontrib><creatorcontrib>Bautz, Marshall W.</creatorcontrib><creatorcontrib>Ricker, George R.</creatorcontrib><creatorcontrib>Hsieh, Ed</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><jtitle>Review of scientific instruments</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Wenzel, Kevin W.</au><au>Li, Chi‐Kang</au><au>Petrasso, Richard D.</au><au>Lo, Daniel H.</au><au>Bautz, Marshall W.</au><au>Ricker, George R.</au><au>Hsieh, Ed</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Response of X‐UV photodiodes to 1.5–17.5 keV x rays and MeV alpha particles</atitle><jtitle>Review of scientific instruments</jtitle><date>1993-07-01</date><risdate>1993</risdate><volume>64</volume><issue>7</issue><spage>1723</spage><epage>1733</epage><pages>1723-1733</pages><issn>0034-6748</issn><eissn>1089-7623</eissn><coden>RSINAK</coden><abstract>The absolute x‐ray response of three X‐UV photodiodes was measured over an energy range of 1.5–17.5 keV so that they could be used to calibrate x‐ray imaging systems for the ASCA satellite mission. An intense electron‐beam x‐ray generator was used to test both the dc and ac x‐ray response at 1.5, 4.5, 8.0, and 17.5 keV, and an 55Fe source was used to examine one of the photodiodes at 5.9 keV. The x‐ray response was determined by comparing the X‐UV diode signal to that of a previously calibrated silicon surface barrier diode (SBD). The X‐UV detector response was similar to the SBD response at low energies (1.5 and 4.5 keV). At 8 keV, the X‐UV detectors exhibited about 70% of the SBD response, and at 17.5 keV, about 50%. This result is surprising, because the X‐UV diodes actually have a greater silicon thickness than the SBD. In contrast to our findings for SBDs in the past, this implies that not the entire physical volume of these detectors comprises the active volume. The X‐UV detector x‐ray response was also examined as a function of the applied bias voltage. No significant bias voltage dependence of the x‐ray signal was found, which indicates that the depletion layer thickness does not determine the active volume either. However, the detector noise was found to decrease substantially as the applied bias was raised from zero to a few volts. Response of these detectors, operated in pulse mode, to 226Ra α particles indicated large charge carrier recombination in the bulk silicon. This feature renders these detectors unsuitable for most charged‐particle spectroscopy applications.</abstract><cop>Woodbury, NY</cop><pub>American Institute of Physics</pub><doi>10.1063/1.1144000</doi><tpages>11</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0034-6748
ispartof Review of scientific instruments, 1993-07, Vol.64 (7), p.1723-1733
issn 0034-6748
1089-7623
language eng
recordid cdi_scitation_primary_10_1063_1_1144000
source American Institute of Physics (AIP) Publications; AIP Digital Archive
subjects Exact sciences and technology
Instruments, apparatus, components and techniques common to several branches of physics and astronomy
Physics
X- and γ-ray instruments and techniques
title Response of X‐UV photodiodes to 1.5–17.5 keV x rays and MeV alpha particles
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-28T23%3A29%3A45IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-scitation_pasca&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Response%20of%20X%E2%80%90UV%20photodiodes%20to%201.5%E2%80%9317.5%20keV%20x%20rays%20and%20MeV%20alpha%20particles&rft.jtitle=Review%20of%20scientific%20instruments&rft.au=Wenzel,%20Kevin%20W.&rft.date=1993-07-01&rft.volume=64&rft.issue=7&rft.spage=1723&rft.epage=1733&rft.pages=1723-1733&rft.issn=0034-6748&rft.eissn=1089-7623&rft.coden=RSINAK&rft_id=info:doi/10.1063/1.1144000&rft_dat=%3Cscitation_pasca%3Ersi%3C/scitation_pasca%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c326t-90a0bc60be8995926e63c2d973ef62ba80a1d4ba6ed6ad6f665622a372f8064a3%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