Parametric dependencies of the experimental tungsten transport coefficients in ICRH and ECRH assisted ASDEX Upgrade H-modes
The profiles of the W transport coefficients have been experimentally calculated for a large database of identical ASDEX Upgrade H-mode discharges where only the radio-frequency (RF) power characteristics have been varied [Angioni et al., Nucl. Fusion 57, 056015 (2017)]. Central ion cyclotron resona...
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creator | Sertoli, M. Angioni, C. Odstrcil, T. |
description | The profiles of the W transport coefficients have been experimentally calculated for a
large database of identical ASDEX Upgrade H-mode discharges where only the radio-frequency
(RF) power characteristics have been varied [Angioni et al., Nucl. Fusion
57, 056015 (2017)]. Central ion cyclotron resonance heating (ICRH) in the
minority heating scheme has been compared with central and off-axis electron cyclotron
resonance heating (ECRH), using both localized and broad heat deposition profiles. The
transport coefficients have been calculated applying the gradient-flux relation to the
evolution of the intrinsic W density in-between sawtooth cycles as measured using the soft
X-ray diagnostic. For both ICRH and ECRH, the major player in reducing the central W
density peaking is found to be the reduction of inward pinch and, in the case of ECRH, the
rise of an outward convection. The impurity convection increases, from negative to
positive, almost linearly with RF-power, while no appreciable changes are observed in the
diffusion coefficient, which remains roughly at neoclassical levels independent of RF
power or background plasma conditions. The ratio
vW/DW
is consistent with the equilibrium
∇
n
W
/
n
W
prior to the sawtooth crash, corroborating the separate
estimates of diffusion and convection. These experimental findings are slightly different
from previous results obtained analysing the evolution of impurity injections over many
sawtooth cycles. Modelling performed using the drift-kinetic code NEO and the gyro-kinetic
code GKW (assuming axisymmetry) overestimates the diffusion coefficient and underestimates
the experimental positive convection. This is a further indication that
magneto-hydrodynamic/neoclassical models accounting for 3D effects may be needed to
characterize impurity transport in sawtoothing tokamak plasmas. |
doi_str_mv | 10.1063/1.4996412 |
format | Article |
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large database of identical ASDEX Upgrade H-mode discharges where only the radio-frequency
(RF) power characteristics have been varied [Angioni et al., Nucl. Fusion
57, 056015 (2017)]. Central ion cyclotron resonance heating (ICRH) in the
minority heating scheme has been compared with central and off-axis electron cyclotron
resonance heating (ECRH), using both localized and broad heat deposition profiles. The
transport coefficients have been calculated applying the gradient-flux relation to the
evolution of the intrinsic W density in-between sawtooth cycles as measured using the soft
X-ray diagnostic. For both ICRH and ECRH, the major player in reducing the central W
density peaking is found to be the reduction of inward pinch and, in the case of ECRH, the
rise of an outward convection. The impurity convection increases, from negative to
positive, almost linearly with RF-power, while no appreciable changes are observed in the
diffusion coefficient, which remains roughly at neoclassical levels independent of RF
power or background plasma conditions. The ratio
vW/DW
is consistent with the equilibrium
∇
n
W
/
n
W
prior to the sawtooth crash, corroborating the separate
estimates of diffusion and convection. These experimental findings are slightly different
from previous results obtained analysing the evolution of impurity injections over many
sawtooth cycles. Modelling performed using the drift-kinetic code NEO and the gyro-kinetic
code GKW (assuming axisymmetry) overestimates the diffusion coefficient and underestimates
the experimental positive convection. This is a further indication that
magneto-hydrodynamic/neoclassical models accounting for 3D effects may be needed to
characterize impurity transport in sawtoothing tokamak plasmas.</description><identifier>ISSN: 1070-664X</identifier><identifier>EISSN: 1089-7674</identifier><identifier>DOI: 10.1063/1.4996412</identifier><identifier>CODEN: PHPAEN</identifier><language>eng</language><publisher>Melville: American Institute of Physics</publisher><subject>Cyclotron resonance ; Diagnostic systems ; Diffusion coefficient ; Heating ; Impurities ; Plasma physics ; Plasmas (physics) ; Radio frequency ; Three dimensional models ; Tokamak devices ; Transport properties ; Tungsten</subject><ispartof>Physics of plasmas, 2017-11, Vol.24 (11)</ispartof><rights>EURATOM</rights><rights>2017 EURATOM</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c327t-cf2821b050486d13afc9f5539c3f716940331dd54c37019d6829ad868bf783</citedby><cites>FETCH-LOGICAL-c327t-cf2821b050486d13afc9f5539c3f716940331dd54c37019d6829ad868bf783</cites><orcidid>0000-0003-1528-6307 ; 0000-0003-0270-9630</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://pubs.aip.org/pop/article-lookup/doi/10.1063/1.4996412$$EHTML$$P50$$Gscitation$$H</linktohtml><link.rule.ids>314,776,780,790,4498,27901,27902,76127</link.rule.ids></links><search><creatorcontrib>Sertoli, M.</creatorcontrib><creatorcontrib>Angioni, C.</creatorcontrib><creatorcontrib>Odstrcil, T.</creatorcontrib><creatorcontrib>ASDEX Upgrade Team, and EUROFusion MST1 Team</creatorcontrib><title>Parametric dependencies of the experimental tungsten transport coefficients in ICRH and ECRH assisted ASDEX Upgrade H-modes</title><title>Physics of plasmas</title><description>The profiles of the W transport coefficients have been experimentally calculated for a
large database of identical ASDEX Upgrade H-mode discharges where only the radio-frequency
(RF) power characteristics have been varied [Angioni et al., Nucl. Fusion
57, 056015 (2017)]. Central ion cyclotron resonance heating (ICRH) in the
minority heating scheme has been compared with central and off-axis electron cyclotron
resonance heating (ECRH), using both localized and broad heat deposition profiles. The
transport coefficients have been calculated applying the gradient-flux relation to the
evolution of the intrinsic W density in-between sawtooth cycles as measured using the soft
X-ray diagnostic. For both ICRH and ECRH, the major player in reducing the central W
density peaking is found to be the reduction of inward pinch and, in the case of ECRH, the
rise of an outward convection. The impurity convection increases, from negative to
positive, almost linearly with RF-power, while no appreciable changes are observed in the
diffusion coefficient, which remains roughly at neoclassical levels independent of RF
power or background plasma conditions. The ratio
vW/DW
is consistent with the equilibrium
∇
n
W
/
n
W
prior to the sawtooth crash, corroborating the separate
estimates of diffusion and convection. These experimental findings are slightly different
from previous results obtained analysing the evolution of impurity injections over many
sawtooth cycles. Modelling performed using the drift-kinetic code NEO and the gyro-kinetic
code GKW (assuming axisymmetry) overestimates the diffusion coefficient and underestimates
the experimental positive convection. This is a further indication that
magneto-hydrodynamic/neoclassical models accounting for 3D effects may be needed to
characterize impurity transport in sawtoothing tokamak plasmas.</description><subject>Cyclotron resonance</subject><subject>Diagnostic systems</subject><subject>Diffusion coefficient</subject><subject>Heating</subject><subject>Impurities</subject><subject>Plasma physics</subject><subject>Plasmas (physics)</subject><subject>Radio frequency</subject><subject>Three dimensional models</subject><subject>Tokamak devices</subject><subject>Transport properties</subject><subject>Tungsten</subject><issn>1070-664X</issn><issn>1089-7674</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><recordid>eNp9kEFLAzEUhBdRsFYP_oOAJ4WtySab3T2WWm2hoFSF3kKavNQtbbImqSj-ebe26EHw9ObwzQxvkuSc4B7BnF6THqsqzkh2kHQILqu04AU73OoCp5yz2XFyEsISY8x4XnaSzwfp5RqirxXS0IDVYFUNATmD4gsgeG_A12uwUa5Q3NhFiGBR9NKGxvmIlANj6tZhY0C1RePBdISk1Wj4LUKoW4NG_ceb4Qw9NwsvNaBRunYawmlyZOQqwNn-dpPp7fBpMEon93fjQX-SKpoVMVUmKzMyxzlmJdeESqMqk-e0UtQUhFcMU0q0zpmiBSaV5mVWSV3ycm6KknaTi11o493rBkIUS7fxtu0TGSEcZzTnRUtd7ijlXQgejGjar6X_EASL7bCCiP2wLXu1Y4Oqo4y1sz_wm_O_oGi0-Q_-m_wFFNSGdQ</recordid><startdate>201711</startdate><enddate>201711</enddate><creator>Sertoli, M.</creator><creator>Angioni, C.</creator><creator>Odstrcil, T.</creator><general>American Institute of Physics</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0003-1528-6307</orcidid><orcidid>https://orcid.org/0000-0003-0270-9630</orcidid></search><sort><creationdate>201711</creationdate><title>Parametric dependencies of the experimental tungsten transport coefficients in ICRH and ECRH assisted ASDEX Upgrade H-modes</title><author>Sertoli, M. ; Angioni, C. ; Odstrcil, T.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c327t-cf2821b050486d13afc9f5539c3f716940331dd54c37019d6829ad868bf783</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Cyclotron resonance</topic><topic>Diagnostic systems</topic><topic>Diffusion coefficient</topic><topic>Heating</topic><topic>Impurities</topic><topic>Plasma physics</topic><topic>Plasmas (physics)</topic><topic>Radio frequency</topic><topic>Three dimensional models</topic><topic>Tokamak devices</topic><topic>Transport properties</topic><topic>Tungsten</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Sertoli, M.</creatorcontrib><creatorcontrib>Angioni, C.</creatorcontrib><creatorcontrib>Odstrcil, T.</creatorcontrib><creatorcontrib>ASDEX Upgrade Team, and EUROFusion MST1 Team</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Physics of plasmas</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Sertoli, M.</au><au>Angioni, C.</au><au>Odstrcil, T.</au><aucorp>ASDEX Upgrade Team, and EUROFusion MST1 Team</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Parametric dependencies of the experimental tungsten transport coefficients in ICRH and ECRH assisted ASDEX Upgrade H-modes</atitle><jtitle>Physics of plasmas</jtitle><date>2017-11</date><risdate>2017</risdate><volume>24</volume><issue>11</issue><issn>1070-664X</issn><eissn>1089-7674</eissn><coden>PHPAEN</coden><abstract>The profiles of the W transport coefficients have been experimentally calculated for a
large database of identical ASDEX Upgrade H-mode discharges where only the radio-frequency
(RF) power characteristics have been varied [Angioni et al., Nucl. Fusion
57, 056015 (2017)]. Central ion cyclotron resonance heating (ICRH) in the
minority heating scheme has been compared with central and off-axis electron cyclotron
resonance heating (ECRH), using both localized and broad heat deposition profiles. The
transport coefficients have been calculated applying the gradient-flux relation to the
evolution of the intrinsic W density in-between sawtooth cycles as measured using the soft
X-ray diagnostic. For both ICRH and ECRH, the major player in reducing the central W
density peaking is found to be the reduction of inward pinch and, in the case of ECRH, the
rise of an outward convection. The impurity convection increases, from negative to
positive, almost linearly with RF-power, while no appreciable changes are observed in the
diffusion coefficient, which remains roughly at neoclassical levels independent of RF
power or background plasma conditions. The ratio
vW/DW
is consistent with the equilibrium
∇
n
W
/
n
W
prior to the sawtooth crash, corroborating the separate
estimates of diffusion and convection. These experimental findings are slightly different
from previous results obtained analysing the evolution of impurity injections over many
sawtooth cycles. Modelling performed using the drift-kinetic code NEO and the gyro-kinetic
code GKW (assuming axisymmetry) overestimates the diffusion coefficient and underestimates
the experimental positive convection. This is a further indication that
magneto-hydrodynamic/neoclassical models accounting for 3D effects may be needed to
characterize impurity transport in sawtoothing tokamak plasmas.</abstract><cop>Melville</cop><pub>American Institute of Physics</pub><doi>10.1063/1.4996412</doi><tpages>16</tpages><orcidid>https://orcid.org/0000-0003-1528-6307</orcidid><orcidid>https://orcid.org/0000-0003-0270-9630</orcidid></addata></record> |
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source | AIP Journals Complete; Alma/SFX Local Collection |
subjects | Cyclotron resonance Diagnostic systems Diffusion coefficient Heating Impurities Plasma physics Plasmas (physics) Radio frequency Three dimensional models Tokamak devices Transport properties Tungsten |
title | Parametric dependencies of the experimental tungsten transport coefficients in ICRH and ECRH assisted ASDEX Upgrade H-modes |
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