Observations of the vacuum ultraviolet and x-ray brightness profiles of Fe, Ni, and Ge in magnetically confined fusion plasmas
The spatial brightness profiles of emission lines for the K-like through He-like ionization states of Fe, Ge, and Ni have been measured during a set of experiments in which Fe and Ge were introduced into FTU tokamak plasmas by using the laser blowoff technique. Nickel was an intrinsic impurity obser...
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container_title | Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics |
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creator | May, M J Finkenthal, M Moos, H W Fournier, K B Goldstein, W H Mattioli, M Pacella, D Mazzitelli, G Leigheb, M Gabellieri, L |
description | The spatial brightness profiles of emission lines for the K-like through He-like ionization states of Fe, Ge, and Ni have been measured during a set of experiments in which Fe and Ge were introduced into FTU tokamak plasmas by using the laser blowoff technique. Nickel was an intrinsic impurity observed during these experiments that was sputtered from the inconel limiter. The brightness profiles were measured by spatially scanable, photometrically calibrated vaccum ultraviolet and x-ray spectrometers that covered the 1 to 1700 A region. Simulations of these profiles and the time evolution of the laser blowoffs were performed with the MIST transport code using several sets of atomic physics compilations [ADPAK (originally in MIST), Arnaud and Raymond (AR92), Arnaud and Rothenflug (AR85), Mazzotta et al., and Mattioli (an extension to Mazzotta)]. The goal was to determine which set of available rates could best simulate the measured spatial brightness profiles and the charge state balance in the plasma. The Mazzotta et al. (for Fe and Ni), the Mattioli (for Ge), and the AR92 (for Fe only) rates adequately simulated the He-, Li-, Be-, Na-, Mg-like ionization states. The F- to B-like charge states could not be simulated by these compilations unless the relevant dielectronic rates were multiplied by a factor of 2. The ADPAK rates could not adequately predict any of the charge states of Fe, Ge, or Ni. |
doi_str_mv | 10.1103/physreve.64.036406 |
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Nickel was an intrinsic impurity observed during these experiments that was sputtered from the inconel limiter. The brightness profiles were measured by spatially scanable, photometrically calibrated vaccum ultraviolet and x-ray spectrometers that covered the 1 to 1700 A region. Simulations of these profiles and the time evolution of the laser blowoffs were performed with the MIST transport code using several sets of atomic physics compilations [ADPAK (originally in MIST), Arnaud and Raymond (AR92), Arnaud and Rothenflug (AR85), Mazzotta et al., and Mattioli (an extension to Mazzotta)]. The goal was to determine which set of available rates could best simulate the measured spatial brightness profiles and the charge state balance in the plasma. The Mazzotta et al. (for Fe and Ni), the Mattioli (for Ge), and the AR92 (for Fe only) rates adequately simulated the He-, Li-, Be-, Na-, Mg-like ionization states. The F- to B-like charge states could not be simulated by these compilations unless the relevant dielectronic rates were multiplied by a factor of 2. The ADPAK rates could not adequately predict any of the charge states of Fe, Ge, or Ni.</description><identifier>ISSN: 1539-3755</identifier><identifier>ISSN: 1063-651X</identifier><identifier>EISSN: 1095-3787</identifier><identifier>DOI: 10.1103/physreve.64.036406</identifier><identifier>PMID: 11580453</identifier><language>eng</language><publisher>United States: The American Physical Society</publisher><subject>ATOMIC PHYSICS ; BATTERY CHARGE STATE ; BRIGHTNESS ; CHARGE STATES ; ENERGY STORAGE ; IONIZATION ; LASERS ; NICKEL ; PLASMA ; TRANSPORT ; X-RAY SPECTROMETERS</subject><ispartof>Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics, 2001-09, Vol.64 (3 Pt 2), p.036406-036406, Article 036406</ispartof><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c463t-b0ad3e7b7749cc6239dc638465799c361840cd6cd876942439f923dbb3088a633</citedby><cites>FETCH-LOGICAL-c463t-b0ad3e7b7749cc6239dc638465799c361840cd6cd876942439f923dbb3088a633</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,777,781,882,2863,2864,27905,27906</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/11580453$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/40277122$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>May, M J</creatorcontrib><creatorcontrib>Finkenthal, M</creatorcontrib><creatorcontrib>Moos, H W</creatorcontrib><creatorcontrib>Fournier, K B</creatorcontrib><creatorcontrib>Goldstein, W H</creatorcontrib><creatorcontrib>Mattioli, M</creatorcontrib><creatorcontrib>Pacella, D</creatorcontrib><creatorcontrib>Mazzitelli, G</creatorcontrib><creatorcontrib>Leigheb, M</creatorcontrib><creatorcontrib>Gabellieri, L</creatorcontrib><title>Observations of the vacuum ultraviolet and x-ray brightness profiles of Fe, Ni, and Ge in magnetically confined fusion plasmas</title><title>Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics</title><addtitle>Phys Rev E Stat Nonlin Soft Matter Phys</addtitle><description>The spatial brightness profiles of emission lines for the K-like through He-like ionization states of Fe, Ge, and Ni have been measured during a set of experiments in which Fe and Ge were introduced into FTU tokamak plasmas by using the laser blowoff technique. Nickel was an intrinsic impurity observed during these experiments that was sputtered from the inconel limiter. The brightness profiles were measured by spatially scanable, photometrically calibrated vaccum ultraviolet and x-ray spectrometers that covered the 1 to 1700 A region. Simulations of these profiles and the time evolution of the laser blowoffs were performed with the MIST transport code using several sets of atomic physics compilations [ADPAK (originally in MIST), Arnaud and Raymond (AR92), Arnaud and Rothenflug (AR85), Mazzotta et al., and Mattioli (an extension to Mazzotta)]. The goal was to determine which set of available rates could best simulate the measured spatial brightness profiles and the charge state balance in the plasma. The Mazzotta et al. (for Fe and Ni), the Mattioli (for Ge), and the AR92 (for Fe only) rates adequately simulated the He-, Li-, Be-, Na-, Mg-like ionization states. The F- to B-like charge states could not be simulated by these compilations unless the relevant dielectronic rates were multiplied by a factor of 2. The ADPAK rates could not adequately predict any of the charge states of Fe, Ge, or Ni.</description><subject>ATOMIC PHYSICS</subject><subject>BATTERY CHARGE STATE</subject><subject>BRIGHTNESS</subject><subject>CHARGE STATES</subject><subject>ENERGY STORAGE</subject><subject>IONIZATION</subject><subject>LASERS</subject><subject>NICKEL</subject><subject>PLASMA</subject><subject>TRANSPORT</subject><subject>X-RAY SPECTROMETERS</subject><issn>1539-3755</issn><issn>1063-651X</issn><issn>1095-3787</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2001</creationdate><recordtype>article</recordtype><recordid>eNpFkU1v3CAQhlHVKN9_oIcKqVJP8QYMBnOsoiStFDVRlJwRxuMsFcZbwFb20t8ekl2pJ-bwvDPMPAh9oWRFKWGXm_U2RVhgJfiKMMGJ-ISOKVFNxWQrP5e6YarUTXOETlL6QwirWcsP0RGlTUt4w47Rv_suQVxMdlNIeBpwXgNejJ3nEc8-R7O4yUPGJvT4tYpmi7voXtY5QEp4E6fBefjI3cAF_u0uPsBbwC7g0bwEyM4a77fYTmFwAXo8zKmMwhtv0mjSGToYjE9wvn9P0fPN9dPVz-ru_vbX1Y-7ynLBctUR0zOQnZRcWStqpnoryiqikUpZJmjLie2F7VspFK85U4OqWd91jLStEYydom-7vlPKTifrMth1-VMAmzUntZS0rgv1fUeVxf7OkLIeXbLgvQkwzUkXiKhy-QLWO9DGKRUHg95EN5q41ZTodzf6obh5hOVaC653bkro67773I3Q_4_sZbA3D-SMhw</recordid><startdate>20010901</startdate><enddate>20010901</enddate><creator>May, M J</creator><creator>Finkenthal, M</creator><creator>Moos, H W</creator><creator>Fournier, K B</creator><creator>Goldstein, W H</creator><creator>Mattioli, M</creator><creator>Pacella, D</creator><creator>Mazzitelli, G</creator><creator>Leigheb, M</creator><creator>Gabellieri, L</creator><general>The American Physical Society</general><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7X8</scope><scope>OTOTI</scope></search><sort><creationdate>20010901</creationdate><title>Observations of the vacuum ultraviolet and x-ray brightness profiles of Fe, Ni, and Ge in magnetically confined fusion plasmas</title><author>May, M J ; Finkenthal, M ; Moos, H W ; Fournier, K B ; Goldstein, W H ; Mattioli, M ; Pacella, D ; Mazzitelli, G ; Leigheb, M ; Gabellieri, L</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c463t-b0ad3e7b7749cc6239dc638465799c361840cd6cd876942439f923dbb3088a633</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2001</creationdate><topic>ATOMIC PHYSICS</topic><topic>BATTERY CHARGE STATE</topic><topic>BRIGHTNESS</topic><topic>CHARGE STATES</topic><topic>ENERGY STORAGE</topic><topic>IONIZATION</topic><topic>LASERS</topic><topic>NICKEL</topic><topic>PLASMA</topic><topic>TRANSPORT</topic><topic>X-RAY SPECTROMETERS</topic><toplevel>online_resources</toplevel><creatorcontrib>May, M J</creatorcontrib><creatorcontrib>Finkenthal, M</creatorcontrib><creatorcontrib>Moos, H W</creatorcontrib><creatorcontrib>Fournier, K B</creatorcontrib><creatorcontrib>Goldstein, W H</creatorcontrib><creatorcontrib>Mattioli, M</creatorcontrib><creatorcontrib>Pacella, D</creatorcontrib><creatorcontrib>Mazzitelli, G</creatorcontrib><creatorcontrib>Leigheb, M</creatorcontrib><creatorcontrib>Gabellieri, L</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><collection>OSTI.GOV</collection><jtitle>Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>May, M J</au><au>Finkenthal, M</au><au>Moos, H W</au><au>Fournier, K B</au><au>Goldstein, W H</au><au>Mattioli, M</au><au>Pacella, D</au><au>Mazzitelli, G</au><au>Leigheb, M</au><au>Gabellieri, L</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Observations of the vacuum ultraviolet and x-ray brightness profiles of Fe, Ni, and Ge in magnetically confined fusion plasmas</atitle><jtitle>Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics</jtitle><addtitle>Phys Rev E Stat Nonlin Soft Matter Phys</addtitle><date>2001-09-01</date><risdate>2001</risdate><volume>64</volume><issue>3 Pt 2</issue><spage>036406</spage><epage>036406</epage><pages>036406-036406</pages><artnum>036406</artnum><issn>1539-3755</issn><issn>1063-651X</issn><eissn>1095-3787</eissn><abstract>The spatial brightness profiles of emission lines for the K-like through He-like ionization states of Fe, Ge, and Ni have been measured during a set of experiments in which Fe and Ge were introduced into FTU tokamak plasmas by using the laser blowoff technique. Nickel was an intrinsic impurity observed during these experiments that was sputtered from the inconel limiter. The brightness profiles were measured by spatially scanable, photometrically calibrated vaccum ultraviolet and x-ray spectrometers that covered the 1 to 1700 A region. Simulations of these profiles and the time evolution of the laser blowoffs were performed with the MIST transport code using several sets of atomic physics compilations [ADPAK (originally in MIST), Arnaud and Raymond (AR92), Arnaud and Rothenflug (AR85), Mazzotta et al., and Mattioli (an extension to Mazzotta)]. The goal was to determine which set of available rates could best simulate the measured spatial brightness profiles and the charge state balance in the plasma. The Mazzotta et al. (for Fe and Ni), the Mattioli (for Ge), and the AR92 (for Fe only) rates adequately simulated the He-, Li-, Be-, Na-, Mg-like ionization states. The F- to B-like charge states could not be simulated by these compilations unless the relevant dielectronic rates were multiplied by a factor of 2. The ADPAK rates could not adequately predict any of the charge states of Fe, Ge, or Ni.</abstract><cop>United States</cop><pub>The American Physical Society</pub><pmid>11580453</pmid><doi>10.1103/physreve.64.036406</doi><tpages>1</tpages></addata></record> |
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title | Observations of the vacuum ultraviolet and x-ray brightness profiles of Fe, Ni, and Ge in magnetically confined fusion plasmas |
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