An extreme ultraviolet radiation source for the simulation of the ionosphere

An extreme ultraviolet (EUV) radiation source for space simulation of plasma and other related phenomena in the laboratory has been developed. A total of forty‐eight small EUV lamps are put together to give a radiation diameter of more than 30 cm. The intensity of this lamp at the hydrogen Lyman‐alp...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Review of scientific instruments 1991-07, Vol.62 (7), p.1721-1726
Hauptverfasser: Oyama, K.‐I., Suzuki, K., Kawashima, N., Zalpuri, K. S., Teii, S., Nakamura, Y.
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 1726
container_issue 7
container_start_page 1721
container_title Review of scientific instruments
container_volume 62
creator Oyama, K.‐I.
Suzuki, K.
Kawashima, N.
Zalpuri, K. S.
Teii, S.
Nakamura, Y.
description An extreme ultraviolet (EUV) radiation source for space simulation of plasma and other related phenomena in the laboratory has been developed. A total of forty‐eight small EUV lamps are put together to give a radiation diameter of more than 30 cm. The intensity of this lamp at the hydrogen Lyman‐alpha line is more than twenty five times stronger than sunlight at the same wavelength and at a distance of about 30 cm from the source. The source is capable of emitting EUV radiations from 110 nm to the longer wavelengths, either continuously or in pulses, and has been used to produce a plasma of 105 els/cm3 when the pressure of NO gas in the chamber was 10−4 Torr. Since this plasma is extremely calm and fairly Maxwellian, it can be used to study the electron collection mechanism of a probe in a collision dominant medium. The source was also utilized to study the interaction between vibrationally excited nitrogen molecules and thermal electrons.
doi_str_mv 10.1063/1.1142412
format Article
fullrecord <record><control><sourceid>proquest_scita</sourceid><recordid>TN_cdi_scitation_primary_10_1063_1_1142412</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>25348810</sourcerecordid><originalsourceid>FETCH-LOGICAL-c357t-542668170a3f0c9b997c9dcb355008e8daeb3a4cb6dc318a4cfa2c9cd2970bdc3</originalsourceid><addsrcrecordid>eNp9kE9LxDAQxYMouK4e_AY9iKBQzTRpmxyXxX-w4EXPIU0TNtI2a5Iu-u2N20VPOpd5vPnNOzyEzgHfAK7ILdwA0IJCcYBmgBnP66ogh2iGMaF5VVN2jE5CeMNpSoAZWi2GTH9Er3udjV30cmtdp2PmZWtltG7Ighu90plxPotrnQXbj910cWbnJOnCZq29PkVHRnZBn-33HL3e370sH_PV88PTcrHKFSnrmJe0qCoGNZbEYMUbzmvFW9WQssSYadZK3RBJVVO1igBLyshCcdUWvMZN8ubocsrdePc-6hBFb4PSXScH7cYgipJQxgAn8GoClXcheG3Extte-k8BWHz3JUDs-0rsxT5UBiU74-WgbPh5oKkuzCFh1xMWlI27Hv7N_BPeOv8Lik1ryBeR9oaV</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>25348810</pqid></control><display><type>article</type><title>An extreme ultraviolet radiation source for the simulation of the ionosphere</title><source>AIP Digital Archive</source><creator>Oyama, K.‐I. ; Suzuki, K. ; Kawashima, N. ; Zalpuri, K. S. ; Teii, S. ; Nakamura, Y.</creator><creatorcontrib>Oyama, K.‐I. ; Suzuki, K. ; Kawashima, N. ; Zalpuri, K. S. ; Teii, S. ; Nakamura, Y.</creatorcontrib><description>An extreme ultraviolet (EUV) radiation source for space simulation of plasma and other related phenomena in the laboratory has been developed. A total of forty‐eight small EUV lamps are put together to give a radiation diameter of more than 30 cm. The intensity of this lamp at the hydrogen Lyman‐alpha line is more than twenty five times stronger than sunlight at the same wavelength and at a distance of about 30 cm from the source. The source is capable of emitting EUV radiations from 110 nm to the longer wavelengths, either continuously or in pulses, and has been used to produce a plasma of 105 els/cm3 when the pressure of NO gas in the chamber was 10−4 Torr. Since this plasma is extremely calm and fairly Maxwellian, it can be used to study the electron collection mechanism of a probe in a collision dominant medium. The source was also utilized to study the interaction between vibrationally excited nitrogen molecules and thermal electrons.</description><identifier>ISSN: 0034-6748</identifier><identifier>EISSN: 1089-7623</identifier><identifier>DOI: 10.1063/1.1142412</identifier><identifier>CODEN: RSINAK</identifier><language>eng</language><publisher>Woodbury, NY: American Institute of Physics</publisher><subject>Atmospheric optics ; Earth, ocean, space ; Exact sciences and technology ; External geophysics</subject><ispartof>Review of scientific instruments, 1991-07, Vol.62 (7), p.1721-1726</ispartof><rights>American Institute of Physics</rights><rights>1993 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c357t-542668170a3f0c9b997c9dcb355008e8daeb3a4cb6dc318a4cfa2c9cd2970bdc3</citedby><cites>FETCH-LOGICAL-c357t-542668170a3f0c9b997c9dcb355008e8daeb3a4cb6dc318a4cfa2c9cd2970bdc3</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/10.1063/1.1142412$$EHTML$$P50$$Gscitation$$H</linktohtml><link.rule.ids>314,776,780,1553,27901,27902,76132</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&amp;idt=4511091$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Oyama, K.‐I.</creatorcontrib><creatorcontrib>Suzuki, K.</creatorcontrib><creatorcontrib>Kawashima, N.</creatorcontrib><creatorcontrib>Zalpuri, K. S.</creatorcontrib><creatorcontrib>Teii, S.</creatorcontrib><creatorcontrib>Nakamura, Y.</creatorcontrib><title>An extreme ultraviolet radiation source for the simulation of the ionosphere</title><title>Review of scientific instruments</title><description>An extreme ultraviolet (EUV) radiation source for space simulation of plasma and other related phenomena in the laboratory has been developed. A total of forty‐eight small EUV lamps are put together to give a radiation diameter of more than 30 cm. The intensity of this lamp at the hydrogen Lyman‐alpha line is more than twenty five times stronger than sunlight at the same wavelength and at a distance of about 30 cm from the source. The source is capable of emitting EUV radiations from 110 nm to the longer wavelengths, either continuously or in pulses, and has been used to produce a plasma of 105 els/cm3 when the pressure of NO gas in the chamber was 10−4 Torr. Since this plasma is extremely calm and fairly Maxwellian, it can be used to study the electron collection mechanism of a probe in a collision dominant medium. The source was also utilized to study the interaction between vibrationally excited nitrogen molecules and thermal electrons.</description><subject>Atmospheric optics</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>External geophysics</subject><issn>0034-6748</issn><issn>1089-7623</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1991</creationdate><recordtype>article</recordtype><recordid>eNp9kE9LxDAQxYMouK4e_AY9iKBQzTRpmxyXxX-w4EXPIU0TNtI2a5Iu-u2N20VPOpd5vPnNOzyEzgHfAK7ILdwA0IJCcYBmgBnP66ogh2iGMaF5VVN2jE5CeMNpSoAZWi2GTH9Er3udjV30cmtdp2PmZWtltG7Ighu90plxPotrnQXbj910cWbnJOnCZq29PkVHRnZBn-33HL3e370sH_PV88PTcrHKFSnrmJe0qCoGNZbEYMUbzmvFW9WQssSYadZK3RBJVVO1igBLyshCcdUWvMZN8ubocsrdePc-6hBFb4PSXScH7cYgipJQxgAn8GoClXcheG3Extte-k8BWHz3JUDs-0rsxT5UBiU74-WgbPh5oKkuzCFh1xMWlI27Hv7N_BPeOv8Lik1ryBeR9oaV</recordid><startdate>19910701</startdate><enddate>19910701</enddate><creator>Oyama, K.‐I.</creator><creator>Suzuki, K.</creator><creator>Kawashima, N.</creator><creator>Zalpuri, K. S.</creator><creator>Teii, S.</creator><creator>Nakamura, Y.</creator><general>American Institute of Physics</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>19910701</creationdate><title>An extreme ultraviolet radiation source for the simulation of the ionosphere</title><author>Oyama, K.‐I. ; Suzuki, K. ; Kawashima, N. ; Zalpuri, K. S. ; Teii, S. ; Nakamura, Y.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c357t-542668170a3f0c9b997c9dcb355008e8daeb3a4cb6dc318a4cfa2c9cd2970bdc3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1991</creationdate><topic>Atmospheric optics</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>External geophysics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Oyama, K.‐I.</creatorcontrib><creatorcontrib>Suzuki, K.</creatorcontrib><creatorcontrib>Kawashima, N.</creatorcontrib><creatorcontrib>Zalpuri, K. S.</creatorcontrib><creatorcontrib>Teii, S.</creatorcontrib><creatorcontrib>Nakamura, Y.</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Review of scientific instruments</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Oyama, K.‐I.</au><au>Suzuki, K.</au><au>Kawashima, N.</au><au>Zalpuri, K. S.</au><au>Teii, S.</au><au>Nakamura, Y.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>An extreme ultraviolet radiation source for the simulation of the ionosphere</atitle><jtitle>Review of scientific instruments</jtitle><date>1991-07-01</date><risdate>1991</risdate><volume>62</volume><issue>7</issue><spage>1721</spage><epage>1726</epage><pages>1721-1726</pages><issn>0034-6748</issn><eissn>1089-7623</eissn><coden>RSINAK</coden><abstract>An extreme ultraviolet (EUV) radiation source for space simulation of plasma and other related phenomena in the laboratory has been developed. A total of forty‐eight small EUV lamps are put together to give a radiation diameter of more than 30 cm. The intensity of this lamp at the hydrogen Lyman‐alpha line is more than twenty five times stronger than sunlight at the same wavelength and at a distance of about 30 cm from the source. The source is capable of emitting EUV radiations from 110 nm to the longer wavelengths, either continuously or in pulses, and has been used to produce a plasma of 105 els/cm3 when the pressure of NO gas in the chamber was 10−4 Torr. Since this plasma is extremely calm and fairly Maxwellian, it can be used to study the electron collection mechanism of a probe in a collision dominant medium. The source was also utilized to study the interaction between vibrationally excited nitrogen molecules and thermal electrons.</abstract><cop>Woodbury, NY</cop><pub>American Institute of Physics</pub><doi>10.1063/1.1142412</doi><tpages>6</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0034-6748
ispartof Review of scientific instruments, 1991-07, Vol.62 (7), p.1721-1726
issn 0034-6748
1089-7623
language eng
recordid cdi_scitation_primary_10_1063_1_1142412
source AIP Digital Archive
subjects Atmospheric optics
Earth, ocean, space
Exact sciences and technology
External geophysics
title An extreme ultraviolet radiation source for the simulation of the ionosphere
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-05T22%3A37%3A06IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_scita&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=An%20extreme%20ultraviolet%20radiation%20source%20for%20the%20simulation%20of%20the%20ionosphere&rft.jtitle=Review%20of%20scientific%20instruments&rft.au=Oyama,%20K.%E2%80%90I.&rft.date=1991-07-01&rft.volume=62&rft.issue=7&rft.spage=1721&rft.epage=1726&rft.pages=1721-1726&rft.issn=0034-6748&rft.eissn=1089-7623&rft.coden=RSINAK&rft_id=info:doi/10.1063/1.1142412&rft_dat=%3Cproquest_scita%3E25348810%3C/proquest_scita%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=25348810&rft_id=info:pmid/&rfr_iscdi=true