Energy loss of 1 – 50 keV H, He, C, N, O, Ne, and Ar ions transmitted through thin carbon foils
Thin foils are used extensively in space plasma spectrometers, for example, for generation of a coincidence measurement via secondary electron emission in time-of-flight mass spectrometers and charge conversion of energetic neutral atoms (ENAs) in ENA imagers. An ion or neutral atom passing through...
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Veröffentlicht in: | Review of scientific instruments 2006-04, Vol.77 (4), p.044501-044501-7 |
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container_title | Review of scientific instruments |
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creator | Allegrini, F. McComas, D. J. Young, D. T. Berthelier, J.-J. Covinhes, J. Illiano, J.-M. Riou, J.-F. Funsten, H. O. Harper, R. W. |
description | Thin foils are used extensively in space plasma spectrometers, for example, for generation of a coincidence measurement via secondary electron emission in time-of-flight mass spectrometers and charge conversion of energetic neutral atoms (ENAs) in ENA imagers. An ion or neutral atom passing through the carbon foil experiences energy loss and straggling that can degrade the energy resolution or mass resolution. These effects need to be quantified in order to permit efficient instrument development and modeling. We present measurements of energy loss and energy loss straggling for H, He, C, N, O, Ne, and Ar ions between 1 and
50
keV
passing through carbon foils of different thicknesses (nominally between 0.5 and
3.0
μ
g
∕
cm
2
). We derive empirical relationships for the energy loss and energy loss straggling as a function of foil thickness, ion species, and ion energy. In particular, below
∼
10
keV
the energy loss of hydrogen seems to vary with foil thickness and the energy loss straggling seems to vary with the square root of the thickness. Our results apply equally well to ions and neutral atoms. |
doi_str_mv | 10.1063/1.2185490 |
format | Article |
fullrecord | <record><control><sourceid>scitation_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_20779206</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>rsi</sourcerecordid><originalsourceid>FETCH-LOGICAL-o302t-ac5cfc119cd5bed0f16e0232ec4db5753f6f2eef454f4bcf2fb52c39df8edd93</originalsourceid><addsrcrecordid>eNqNkM1KAzEQx4MoWKsH32DAm-zWfGz241hKtUKxl-I1ZPPRrrZJSaLgzXfwDX0St7TgTZzDDAO__8D8ELomeERwye7IiJKaFw0-QQOC6yavSspO0QBjVuRlVdTn6CLGF9wXJ2SA5NSZsPqAjY8RvAUC359fwDG8mmeYZTAzGUwyeMpg0fd-kU7DOEDnXYQUpIvbLiWjIa2Df1ut-9k5UDK03oH13SZeojMrN9FcHecQLe-ny8ksny8eHifjee4ZpimXiiurCGmU5q3R2JLSYMqoUYVuecWZLS01xha8sEWrLLUtp4o12tZG64YN0c3hrI-pE1F1yai18s4ZlQTFVdXQ3s8Q1QdqD8jUfyF2odvK8CEIFnuDgoijwYMZsTcjvO2jt_-O_gW_-_ALip227Afro4M7</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Energy loss of 1 – 50 keV H, He, C, N, O, Ne, and Ar ions transmitted through thin carbon foils</title><source>AIP Journals Complete</source><source>AIP Digital Archive</source><creator>Allegrini, F. ; McComas, D. J. ; Young, D. T. ; Berthelier, J.-J. ; Covinhes, J. ; Illiano, J.-M. ; Riou, J.-F. ; Funsten, H. O. ; Harper, R. W.</creator><creatorcontrib>Allegrini, F. ; McComas, D. J. ; Young, D. T. ; Berthelier, J.-J. ; Covinhes, J. ; Illiano, J.-M. ; Riou, J.-F. ; Funsten, H. O. ; Harper, R. W.</creatorcontrib><description>Thin foils are used extensively in space plasma spectrometers, for example, for generation of a coincidence measurement via secondary electron emission in time-of-flight mass spectrometers and charge conversion of energetic neutral atoms (ENAs) in ENA imagers. An ion or neutral atom passing through the carbon foil experiences energy loss and straggling that can degrade the energy resolution or mass resolution. These effects need to be quantified in order to permit efficient instrument development and modeling. We present measurements of energy loss and energy loss straggling for H, He, C, N, O, Ne, and Ar ions between 1 and
50
keV
passing through carbon foils of different thicknesses (nominally between 0.5 and
3.0
μ
g
∕
cm
2
). We derive empirical relationships for the energy loss and energy loss straggling as a function of foil thickness, ion species, and ion energy. In particular, below
∼
10
keV
the energy loss of hydrogen seems to vary with foil thickness and the energy loss straggling seems to vary with the square root of the thickness. Our results apply equally well to ions and neutral atoms.</description><identifier>ISSN: 0034-6748</identifier><identifier>EISSN: 1089-7623</identifier><identifier>DOI: 10.1063/1.2185490</identifier><identifier>CODEN: RSINAK</identifier><language>eng</language><publisher>United States: American Institute of Physics</publisher><subject>ARGON ; ARGON IONS ; ATOMS ; CARBON ; ELECTRON EMISSION ; ENERGY RESOLUTION ; FOILS ; HELIUM ; HYDROGEN ; INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY ; KEV RANGE 10-100 ; MASS RESOLUTION ; NEON ; NITROGEN ; OXYGEN ; THICKNESS ; TIME-OF-FLIGHT MASS SPECTROMETERS</subject><ispartof>Review of scientific instruments, 2006-04, Vol.77 (4), p.044501-044501-7</ispartof><rights>American Institute of Physics</rights><rights>2006 American Institute of Physics</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-o302t-ac5cfc119cd5bed0f16e0232ec4db5753f6f2eef454f4bcf2fb52c39df8edd93</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/10.1063/1.2185490$$EHTML$$P50$$Gscitation$$H</linktohtml><link.rule.ids>230,314,776,780,790,881,1553,4498,27901,27902,76353,76359</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/20779206$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Allegrini, F.</creatorcontrib><creatorcontrib>McComas, D. J.</creatorcontrib><creatorcontrib>Young, D. T.</creatorcontrib><creatorcontrib>Berthelier, J.-J.</creatorcontrib><creatorcontrib>Covinhes, J.</creatorcontrib><creatorcontrib>Illiano, J.-M.</creatorcontrib><creatorcontrib>Riou, J.-F.</creatorcontrib><creatorcontrib>Funsten, H. O.</creatorcontrib><creatorcontrib>Harper, R. W.</creatorcontrib><title>Energy loss of 1 – 50 keV H, He, C, N, O, Ne, and Ar ions transmitted through thin carbon foils</title><title>Review of scientific instruments</title><description>Thin foils are used extensively in space plasma spectrometers, for example, for generation of a coincidence measurement via secondary electron emission in time-of-flight mass spectrometers and charge conversion of energetic neutral atoms (ENAs) in ENA imagers. An ion or neutral atom passing through the carbon foil experiences energy loss and straggling that can degrade the energy resolution or mass resolution. These effects need to be quantified in order to permit efficient instrument development and modeling. We present measurements of energy loss and energy loss straggling for H, He, C, N, O, Ne, and Ar ions between 1 and
50
keV
passing through carbon foils of different thicknesses (nominally between 0.5 and
3.0
μ
g
∕
cm
2
). We derive empirical relationships for the energy loss and energy loss straggling as a function of foil thickness, ion species, and ion energy. In particular, below
∼
10
keV
the energy loss of hydrogen seems to vary with foil thickness and the energy loss straggling seems to vary with the square root of the thickness. Our results apply equally well to ions and neutral atoms.</description><subject>ARGON</subject><subject>ARGON IONS</subject><subject>ATOMS</subject><subject>CARBON</subject><subject>ELECTRON EMISSION</subject><subject>ENERGY RESOLUTION</subject><subject>FOILS</subject><subject>HELIUM</subject><subject>HYDROGEN</subject><subject>INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY</subject><subject>KEV RANGE 10-100</subject><subject>MASS RESOLUTION</subject><subject>NEON</subject><subject>NITROGEN</subject><subject>OXYGEN</subject><subject>THICKNESS</subject><subject>TIME-OF-FLIGHT MASS SPECTROMETERS</subject><issn>0034-6748</issn><issn>1089-7623</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2006</creationdate><recordtype>article</recordtype><recordid>eNqNkM1KAzEQx4MoWKsH32DAm-zWfGz241hKtUKxl-I1ZPPRrrZJSaLgzXfwDX0St7TgTZzDDAO__8D8ELomeERwye7IiJKaFw0-QQOC6yavSspO0QBjVuRlVdTn6CLGF9wXJ2SA5NSZsPqAjY8RvAUC359fwDG8mmeYZTAzGUwyeMpg0fd-kU7DOEDnXYQUpIvbLiWjIa2Df1ut-9k5UDK03oH13SZeojMrN9FcHecQLe-ny8ksny8eHifjee4ZpimXiiurCGmU5q3R2JLSYMqoUYVuecWZLS01xha8sEWrLLUtp4o12tZG64YN0c3hrI-pE1F1yai18s4ZlQTFVdXQ3s8Q1QdqD8jUfyF2odvK8CEIFnuDgoijwYMZsTcjvO2jt_-O_gW_-_ALip227Afro4M7</recordid><startdate>20060401</startdate><enddate>20060401</enddate><creator>Allegrini, F.</creator><creator>McComas, D. J.</creator><creator>Young, D. T.</creator><creator>Berthelier, J.-J.</creator><creator>Covinhes, J.</creator><creator>Illiano, J.-M.</creator><creator>Riou, J.-F.</creator><creator>Funsten, H. O.</creator><creator>Harper, R. W.</creator><general>American Institute of Physics</general><scope>OTOTI</scope></search><sort><creationdate>20060401</creationdate><title>Energy loss of 1 – 50 keV H, He, C, N, O, Ne, and Ar ions transmitted through thin carbon foils</title><author>Allegrini, F. ; McComas, D. J. ; Young, D. T. ; Berthelier, J.-J. ; Covinhes, J. ; Illiano, J.-M. ; Riou, J.-F. ; Funsten, H. O. ; Harper, R. W.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-o302t-ac5cfc119cd5bed0f16e0232ec4db5753f6f2eef454f4bcf2fb52c39df8edd93</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2006</creationdate><topic>ARGON</topic><topic>ARGON IONS</topic><topic>ATOMS</topic><topic>CARBON</topic><topic>ELECTRON EMISSION</topic><topic>ENERGY RESOLUTION</topic><topic>FOILS</topic><topic>HELIUM</topic><topic>HYDROGEN</topic><topic>INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY</topic><topic>KEV RANGE 10-100</topic><topic>MASS RESOLUTION</topic><topic>NEON</topic><topic>NITROGEN</topic><topic>OXYGEN</topic><topic>THICKNESS</topic><topic>TIME-OF-FLIGHT MASS SPECTROMETERS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Allegrini, F.</creatorcontrib><creatorcontrib>McComas, D. J.</creatorcontrib><creatorcontrib>Young, D. T.</creatorcontrib><creatorcontrib>Berthelier, J.-J.</creatorcontrib><creatorcontrib>Covinhes, J.</creatorcontrib><creatorcontrib>Illiano, J.-M.</creatorcontrib><creatorcontrib>Riou, J.-F.</creatorcontrib><creatorcontrib>Funsten, H. O.</creatorcontrib><creatorcontrib>Harper, R. W.</creatorcontrib><collection>OSTI.GOV</collection><jtitle>Review of scientific instruments</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Allegrini, F.</au><au>McComas, D. J.</au><au>Young, D. T.</au><au>Berthelier, J.-J.</au><au>Covinhes, J.</au><au>Illiano, J.-M.</au><au>Riou, J.-F.</au><au>Funsten, H. O.</au><au>Harper, R. W.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Energy loss of 1 – 50 keV H, He, C, N, O, Ne, and Ar ions transmitted through thin carbon foils</atitle><jtitle>Review of scientific instruments</jtitle><date>2006-04-01</date><risdate>2006</risdate><volume>77</volume><issue>4</issue><spage>044501</spage><epage>044501-7</epage><pages>044501-044501-7</pages><issn>0034-6748</issn><eissn>1089-7623</eissn><coden>RSINAK</coden><abstract>Thin foils are used extensively in space plasma spectrometers, for example, for generation of a coincidence measurement via secondary electron emission in time-of-flight mass spectrometers and charge conversion of energetic neutral atoms (ENAs) in ENA imagers. An ion or neutral atom passing through the carbon foil experiences energy loss and straggling that can degrade the energy resolution or mass resolution. These effects need to be quantified in order to permit efficient instrument development and modeling. We present measurements of energy loss and energy loss straggling for H, He, C, N, O, Ne, and Ar ions between 1 and
50
keV
passing through carbon foils of different thicknesses (nominally between 0.5 and
3.0
μ
g
∕
cm
2
). We derive empirical relationships for the energy loss and energy loss straggling as a function of foil thickness, ion species, and ion energy. In particular, below
∼
10
keV
the energy loss of hydrogen seems to vary with foil thickness and the energy loss straggling seems to vary with the square root of the thickness. Our results apply equally well to ions and neutral atoms.</abstract><cop>United States</cop><pub>American Institute of Physics</pub><doi>10.1063/1.2185490</doi><tpages>7</tpages></addata></record> |
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language | eng |
recordid | cdi_osti_scitechconnect_20779206 |
source | AIP Journals Complete; AIP Digital Archive |
subjects | ARGON ARGON IONS ATOMS CARBON ELECTRON EMISSION ENERGY RESOLUTION FOILS HELIUM HYDROGEN INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY KEV RANGE 10-100 MASS RESOLUTION NEON NITROGEN OXYGEN THICKNESS TIME-OF-FLIGHT MASS SPECTROMETERS |
title | Energy loss of 1 – 50 keV H, He, C, N, O, Ne, and Ar ions transmitted through thin carbon foils |
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