Cosmic ray neutron induced upsets as a major contributor to the soft error rate of current and future generation DRAMs

The system soft error rate (SSER) of 4M/16M DRAMs has been shown to be dependent on the cosmic ray neutron flux. A simple model and accelerated soft error rate (ASER) measurements made with an intense, high energy neutron beam support this result. The model predicts that cosmic ray neutron induced s...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: McKee, W.R., McAdams, H.P., Smith, E.B., McPherson, J.W., Janzen, J.W., Ondrusek, J.C., Hyslop, A.E., Russell, D.E., Coy, R.A., Bergman, D.W., Nguyen, N.Q., Aton, T.J., Block, L.W., Huynh, V.C.
Format: Tagungsbericht
Sprache:eng
Schlagworte:
Online-Zugang:Volltext bestellen
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 6
container_issue
container_start_page 1
container_title
container_volume
creator McKee, W.R.
McAdams, H.P.
Smith, E.B.
McPherson, J.W.
Janzen, J.W.
Ondrusek, J.C.
Hyslop, A.E.
Russell, D.E.
Coy, R.A.
Bergman, D.W.
Nguyen, N.Q.
Aton, T.J.
Block, L.W.
Huynh, V.C.
description The system soft error rate (SSER) of 4M/16M DRAMs has been shown to be dependent on the cosmic ray neutron flux. A simple model and accelerated soft error rate (ASER) measurements made with an intense, high energy neutron beam support this result. The model predicts that cosmic ray neutron induced soft errors will become important at the 64M DRAM generation and beyond.
doi_str_mv 10.1109/RELPHY.1996.492052
format Conference Proceeding
fullrecord <record><control><sourceid>ieee_6IE</sourceid><recordid>TN_cdi_ieee_primary_492052</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><ieee_id>492052</ieee_id><sourcerecordid>492052</sourcerecordid><originalsourceid>FETCH-LOGICAL-i87t-8924fcdfa8ebd30273473943c56996276dfa668f8131db297619ac2ec935c8dd3</originalsourceid><addsrcrecordid>eNotUF1LAzEQDIig1v6BPu0faM0ll8vlsdRqhYpS-uJTSZONpthLyYfQf2-gXRZmmIFhZwmZNHTWNFQ9bZbrz9XXrFGqm7WKUcFuyAOVPeVMCi7uyDilA63TCsEkvyd_i5CO3kDUZxiw5BgG8IMtBi2UU8KcQNeFoz6ECCYMOfp9yZXnAPkHIQWXAWOsStQZITgwJUYcMujBgiu5RIRvHLDavqY_b-bv6ZHcOv2bcHzFEdm-LLeL1XT98fq2mK-nvpd52ivWOmOd7nFvOa0Ht5KrlhvR1YJMdtXqut71DW_sninZNUobhkZxYXpr-YhMLrEeEXen6I86nneXx_B_xxNbYQ</addsrcrecordid><sourcetype>Publisher</sourcetype><iscdi>true</iscdi><recordtype>conference_proceeding</recordtype></control><display><type>conference_proceeding</type><title>Cosmic ray neutron induced upsets as a major contributor to the soft error rate of current and future generation DRAMs</title><source>IEEE Electronic Library (IEL) Conference Proceedings</source><creator>McKee, W.R. ; McAdams, H.P. ; Smith, E.B. ; McPherson, J.W. ; Janzen, J.W. ; Ondrusek, J.C. ; Hyslop, A.E. ; Russell, D.E. ; Coy, R.A. ; Bergman, D.W. ; Nguyen, N.Q. ; Aton, T.J. ; Block, L.W. ; Huynh, V.C.</creator><creatorcontrib>McKee, W.R. ; McAdams, H.P. ; Smith, E.B. ; McPherson, J.W. ; Janzen, J.W. ; Ondrusek, J.C. ; Hyslop, A.E. ; Russell, D.E. ; Coy, R.A. ; Bergman, D.W. ; Nguyen, N.Q. ; Aton, T.J. ; Block, L.W. ; Huynh, V.C.</creatorcontrib><description>The system soft error rate (SSER) of 4M/16M DRAMs has been shown to be dependent on the cosmic ray neutron flux. A simple model and accelerated soft error rate (ASER) measurements made with an intense, high energy neutron beam support this result. The model predicts that cosmic ray neutron induced soft errors will become important at the 64M DRAM generation and beyond.</description><identifier>ISBN: 0780327535</identifier><identifier>ISBN: 9780780327535</identifier><identifier>DOI: 10.1109/RELPHY.1996.492052</identifier><language>eng</language><publisher>IEEE</publisher><subject>Aerospace electronics ; Aircraft ; Cosmic rays ; Electrons ; Error analysis ; Instruments ; Mesons ; Neutrons ; Protons ; Silicon</subject><ispartof>Proceedings of International Reliability Physics Symposium, 1996, p.1-6</ispartof><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://ieeexplore.ieee.org/document/492052$$EHTML$$P50$$Gieee$$H</linktohtml><link.rule.ids>309,310,776,780,785,786,2052,4036,4037,27902,54895</link.rule.ids><linktorsrc>$$Uhttps://ieeexplore.ieee.org/document/492052$$EView_record_in_IEEE$$FView_record_in_$$GIEEE</linktorsrc></links><search><creatorcontrib>McKee, W.R.</creatorcontrib><creatorcontrib>McAdams, H.P.</creatorcontrib><creatorcontrib>Smith, E.B.</creatorcontrib><creatorcontrib>McPherson, J.W.</creatorcontrib><creatorcontrib>Janzen, J.W.</creatorcontrib><creatorcontrib>Ondrusek, J.C.</creatorcontrib><creatorcontrib>Hyslop, A.E.</creatorcontrib><creatorcontrib>Russell, D.E.</creatorcontrib><creatorcontrib>Coy, R.A.</creatorcontrib><creatorcontrib>Bergman, D.W.</creatorcontrib><creatorcontrib>Nguyen, N.Q.</creatorcontrib><creatorcontrib>Aton, T.J.</creatorcontrib><creatorcontrib>Block, L.W.</creatorcontrib><creatorcontrib>Huynh, V.C.</creatorcontrib><title>Cosmic ray neutron induced upsets as a major contributor to the soft error rate of current and future generation DRAMs</title><title>Proceedings of International Reliability Physics Symposium</title><addtitle>RELPHY</addtitle><description>The system soft error rate (SSER) of 4M/16M DRAMs has been shown to be dependent on the cosmic ray neutron flux. A simple model and accelerated soft error rate (ASER) measurements made with an intense, high energy neutron beam support this result. The model predicts that cosmic ray neutron induced soft errors will become important at the 64M DRAM generation and beyond.</description><subject>Aerospace electronics</subject><subject>Aircraft</subject><subject>Cosmic rays</subject><subject>Electrons</subject><subject>Error analysis</subject><subject>Instruments</subject><subject>Mesons</subject><subject>Neutrons</subject><subject>Protons</subject><subject>Silicon</subject><isbn>0780327535</isbn><isbn>9780780327535</isbn><fulltext>true</fulltext><rsrctype>conference_proceeding</rsrctype><creationdate>1996</creationdate><recordtype>conference_proceeding</recordtype><sourceid>6IE</sourceid><sourceid>RIE</sourceid><recordid>eNotUF1LAzEQDIig1v6BPu0faM0ll8vlsdRqhYpS-uJTSZONpthLyYfQf2-gXRZmmIFhZwmZNHTWNFQ9bZbrz9XXrFGqm7WKUcFuyAOVPeVMCi7uyDilA63TCsEkvyd_i5CO3kDUZxiw5BgG8IMtBi2UU8KcQNeFoz6ECCYMOfp9yZXnAPkHIQWXAWOsStQZITgwJUYcMujBgiu5RIRvHLDavqY_b-bv6ZHcOv2bcHzFEdm-LLeL1XT98fq2mK-nvpd52ivWOmOd7nFvOa0Ht5KrlhvR1YJMdtXqut71DW_sninZNUobhkZxYXpr-YhMLrEeEXen6I86nneXx_B_xxNbYQ</recordid><startdate>1996</startdate><enddate>1996</enddate><creator>McKee, W.R.</creator><creator>McAdams, H.P.</creator><creator>Smith, E.B.</creator><creator>McPherson, J.W.</creator><creator>Janzen, J.W.</creator><creator>Ondrusek, J.C.</creator><creator>Hyslop, A.E.</creator><creator>Russell, D.E.</creator><creator>Coy, R.A.</creator><creator>Bergman, D.W.</creator><creator>Nguyen, N.Q.</creator><creator>Aton, T.J.</creator><creator>Block, L.W.</creator><creator>Huynh, V.C.</creator><general>IEEE</general><scope>6IE</scope><scope>6IL</scope><scope>CBEJK</scope><scope>RIE</scope><scope>RIL</scope></search><sort><creationdate>1996</creationdate><title>Cosmic ray neutron induced upsets as a major contributor to the soft error rate of current and future generation DRAMs</title><author>McKee, W.R. ; McAdams, H.P. ; Smith, E.B. ; McPherson, J.W. ; Janzen, J.W. ; Ondrusek, J.C. ; Hyslop, A.E. ; Russell, D.E. ; Coy, R.A. ; Bergman, D.W. ; Nguyen, N.Q. ; Aton, T.J. ; Block, L.W. ; Huynh, V.C.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-i87t-8924fcdfa8ebd30273473943c56996276dfa668f8131db297619ac2ec935c8dd3</frbrgroupid><rsrctype>conference_proceedings</rsrctype><prefilter>conference_proceedings</prefilter><language>eng</language><creationdate>1996</creationdate><topic>Aerospace electronics</topic><topic>Aircraft</topic><topic>Cosmic rays</topic><topic>Electrons</topic><topic>Error analysis</topic><topic>Instruments</topic><topic>Mesons</topic><topic>Neutrons</topic><topic>Protons</topic><topic>Silicon</topic><toplevel>online_resources</toplevel><creatorcontrib>McKee, W.R.</creatorcontrib><creatorcontrib>McAdams, H.P.</creatorcontrib><creatorcontrib>Smith, E.B.</creatorcontrib><creatorcontrib>McPherson, J.W.</creatorcontrib><creatorcontrib>Janzen, J.W.</creatorcontrib><creatorcontrib>Ondrusek, J.C.</creatorcontrib><creatorcontrib>Hyslop, A.E.</creatorcontrib><creatorcontrib>Russell, D.E.</creatorcontrib><creatorcontrib>Coy, R.A.</creatorcontrib><creatorcontrib>Bergman, D.W.</creatorcontrib><creatorcontrib>Nguyen, N.Q.</creatorcontrib><creatorcontrib>Aton, T.J.</creatorcontrib><creatorcontrib>Block, L.W.</creatorcontrib><creatorcontrib>Huynh, V.C.</creatorcontrib><collection>IEEE Electronic Library (IEL) Conference Proceedings</collection><collection>IEEE Proceedings Order Plan All Online (POP All Online) 1998-present by volume</collection><collection>IEEE Xplore All Conference Proceedings</collection><collection>IEEE Electronic Library (IEL)</collection><collection>IEEE Proceedings Order Plans (POP All) 1998-Present</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>McKee, W.R.</au><au>McAdams, H.P.</au><au>Smith, E.B.</au><au>McPherson, J.W.</au><au>Janzen, J.W.</au><au>Ondrusek, J.C.</au><au>Hyslop, A.E.</au><au>Russell, D.E.</au><au>Coy, R.A.</au><au>Bergman, D.W.</au><au>Nguyen, N.Q.</au><au>Aton, T.J.</au><au>Block, L.W.</au><au>Huynh, V.C.</au><format>book</format><genre>proceeding</genre><ristype>CONF</ristype><atitle>Cosmic ray neutron induced upsets as a major contributor to the soft error rate of current and future generation DRAMs</atitle><btitle>Proceedings of International Reliability Physics Symposium</btitle><stitle>RELPHY</stitle><date>1996</date><risdate>1996</risdate><spage>1</spage><epage>6</epage><pages>1-6</pages><isbn>0780327535</isbn><isbn>9780780327535</isbn><abstract>The system soft error rate (SSER) of 4M/16M DRAMs has been shown to be dependent on the cosmic ray neutron flux. A simple model and accelerated soft error rate (ASER) measurements made with an intense, high energy neutron beam support this result. The model predicts that cosmic ray neutron induced soft errors will become important at the 64M DRAM generation and beyond.</abstract><pub>IEEE</pub><doi>10.1109/RELPHY.1996.492052</doi><tpages>6</tpages></addata></record>
fulltext fulltext_linktorsrc
identifier ISBN: 0780327535
ispartof Proceedings of International Reliability Physics Symposium, 1996, p.1-6
issn
language eng
recordid cdi_ieee_primary_492052
source IEEE Electronic Library (IEL) Conference Proceedings
subjects Aerospace electronics
Aircraft
Cosmic rays
Electrons
Error analysis
Instruments
Mesons
Neutrons
Protons
Silicon
title Cosmic ray neutron induced upsets as a major contributor to the soft error rate of current and future generation DRAMs
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-30T00%3A56%3A56IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-ieee_6IE&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=proceeding&rft.atitle=Cosmic%20ray%20neutron%20induced%20upsets%20as%20a%20major%20contributor%20to%20the%20soft%20error%20rate%20of%20current%20and%20future%20generation%20DRAMs&rft.btitle=Proceedings%20of%20International%20Reliability%20Physics%20Symposium&rft.au=McKee,%20W.R.&rft.date=1996&rft.spage=1&rft.epage=6&rft.pages=1-6&rft.isbn=0780327535&rft.isbn_list=9780780327535&rft_id=info:doi/10.1109/RELPHY.1996.492052&rft_dat=%3Cieee_6IE%3E492052%3C/ieee_6IE%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rft_ieee_id=492052&rfr_iscdi=true