General parametric dependence of atmospheric pressure argon plasmas

Abstract Using a global model for atmospheric pressure plasma, we investigated general dependence of plasma properties on power density and plasma size. We built a global simulation for a pure argon cylindrical plasma and observed changes in plasma properties with the power density and plasma size....
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Jeong, Seokyong [verfasserIn] Lee, Jimo Yun, Gunsu

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2022

Schlagwörter:	Cold plasma Plasma modeling Plasma simulation Atmospheric pressure plasma

Anmerkung:	© The Korean Physical Society 2022. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.

Übergeordnetes Werk:	Enthalten in: Journal of the Korean Physical Society - Berlin : Springer, 1968, 82(2022), 1 vom: 13. Dez., Seite 32-39
Übergeordnetes Werk:	volume:82 ; year:2022 ; number:1 ; day:13 ; month:12 ; pages:32-39

Links:	Volltext

DOI / URN:	10.1007/s40042-022-00686-6

Katalog-ID:	SPR051325721

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520			\|a Abstract Using a global model for atmospheric pressure plasma, we investigated general dependence of plasma properties on power density and plasma size. We built a global simulation for a pure argon cylindrical plasma and observed changes in plasma properties with the power density and plasma size. The study of the power dependence shows that the density of excited species is in general proportional to the power when the power density is low, whereas the density becomes saturated when the power density becomes high enough. These trends are explained by a generalized form of particle balance equation, implying that the same trends for reactive species density would emerge in various plasma conditions. For the plasma size dependence, the electron density increases and the electron temperature decreases for increasing plasma size. Both become saturated when the plasma size becomes large enough. These trends of electron density and temperature are explained by the relative change of the diffusive loss. Our simulation results give a useful insight into the tendency of plasma properties over a wide range of plasma parameters.
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allfields	10.1007/s40042-022-00686-6 doi (DE-627)SPR051325721 (SPR)s40042-022-00686-6-e DE-627 ger DE-627 rakwb eng Jeong, Seokyong verfasserin aut General parametric dependence of atmospheric pressure argon plasmas 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Korean Physical Society 2022. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Abstract Using a global model for atmospheric pressure plasma, we investigated general dependence of plasma properties on power density and plasma size. We built a global simulation for a pure argon cylindrical plasma and observed changes in plasma properties with the power density and plasma size. The study of the power dependence shows that the density of excited species is in general proportional to the power when the power density is low, whereas the density becomes saturated when the power density becomes high enough. These trends are explained by a generalized form of particle balance equation, implying that the same trends for reactive species density would emerge in various plasma conditions. For the plasma size dependence, the electron density increases and the electron temperature decreases for increasing plasma size. Both become saturated when the plasma size becomes large enough. These trends of electron density and temperature are explained by the relative change of the diffusive loss. Our simulation results give a useful insight into the tendency of plasma properties over a wide range of plasma parameters. Cold plasma (dpeaa)DE-He213 Plasma modeling (dpeaa)DE-He213 Plasma simulation (dpeaa)DE-He213 Atmospheric pressure plasma (dpeaa)DE-He213 Lee, Jimo aut Yun, Gunsu aut Enthalten in Journal of the Korean Physical Society Berlin : Springer, 1968 82(2022), 1 vom: 13. Dez., Seite 32-39 (DE-627)328820865 (DE-600)2046361-3 1976-8524 nnns volume:82 year:2022 number:1 day:13 month:12 pages:32-39 https://dx.doi.org/10.1007/s40042-022-00686-6 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 82 2022 1 13 12 32-39
spelling	10.1007/s40042-022-00686-6 doi (DE-627)SPR051325721 (SPR)s40042-022-00686-6-e DE-627 ger DE-627 rakwb eng Jeong, Seokyong verfasserin aut General parametric dependence of atmospheric pressure argon plasmas 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Korean Physical Society 2022. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Abstract Using a global model for atmospheric pressure plasma, we investigated general dependence of plasma properties on power density and plasma size. We built a global simulation for a pure argon cylindrical plasma and observed changes in plasma properties with the power density and plasma size. The study of the power dependence shows that the density of excited species is in general proportional to the power when the power density is low, whereas the density becomes saturated when the power density becomes high enough. These trends are explained by a generalized form of particle balance equation, implying that the same trends for reactive species density would emerge in various plasma conditions. For the plasma size dependence, the electron density increases and the electron temperature decreases for increasing plasma size. Both become saturated when the plasma size becomes large enough. These trends of electron density and temperature are explained by the relative change of the diffusive loss. Our simulation results give a useful insight into the tendency of plasma properties over a wide range of plasma parameters. Cold plasma (dpeaa)DE-He213 Plasma modeling (dpeaa)DE-He213 Plasma simulation (dpeaa)DE-He213 Atmospheric pressure plasma (dpeaa)DE-He213 Lee, Jimo aut Yun, Gunsu aut Enthalten in Journal of the Korean Physical Society Berlin : Springer, 1968 82(2022), 1 vom: 13. Dez., Seite 32-39 (DE-627)328820865 (DE-600)2046361-3 1976-8524 nnns volume:82 year:2022 number:1 day:13 month:12 pages:32-39 https://dx.doi.org/10.1007/s40042-022-00686-6 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 82 2022 1 13 12 32-39
allfields_unstemmed	10.1007/s40042-022-00686-6 doi (DE-627)SPR051325721 (SPR)s40042-022-00686-6-e DE-627 ger DE-627 rakwb eng Jeong, Seokyong verfasserin aut General parametric dependence of atmospheric pressure argon plasmas 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Korean Physical Society 2022. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Abstract Using a global model for atmospheric pressure plasma, we investigated general dependence of plasma properties on power density and plasma size. We built a global simulation for a pure argon cylindrical plasma and observed changes in plasma properties with the power density and plasma size. The study of the power dependence shows that the density of excited species is in general proportional to the power when the power density is low, whereas the density becomes saturated when the power density becomes high enough. These trends are explained by a generalized form of particle balance equation, implying that the same trends for reactive species density would emerge in various plasma conditions. For the plasma size dependence, the electron density increases and the electron temperature decreases for increasing plasma size. Both become saturated when the plasma size becomes large enough. These trends of electron density and temperature are explained by the relative change of the diffusive loss. Our simulation results give a useful insight into the tendency of plasma properties over a wide range of plasma parameters. Cold plasma (dpeaa)DE-He213 Plasma modeling (dpeaa)DE-He213 Plasma simulation (dpeaa)DE-He213 Atmospheric pressure plasma (dpeaa)DE-He213 Lee, Jimo aut Yun, Gunsu aut Enthalten in Journal of the Korean Physical Society Berlin : Springer, 1968 82(2022), 1 vom: 13. Dez., Seite 32-39 (DE-627)328820865 (DE-600)2046361-3 1976-8524 nnns volume:82 year:2022 number:1 day:13 month:12 pages:32-39 https://dx.doi.org/10.1007/s40042-022-00686-6 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 82 2022 1 13 12 32-39
allfieldsGer	10.1007/s40042-022-00686-6 doi (DE-627)SPR051325721 (SPR)s40042-022-00686-6-e DE-627 ger DE-627 rakwb eng Jeong, Seokyong verfasserin aut General parametric dependence of atmospheric pressure argon plasmas 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Korean Physical Society 2022. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Abstract Using a global model for atmospheric pressure plasma, we investigated general dependence of plasma properties on power density and plasma size. We built a global simulation for a pure argon cylindrical plasma and observed changes in plasma properties with the power density and plasma size. The study of the power dependence shows that the density of excited species is in general proportional to the power when the power density is low, whereas the density becomes saturated when the power density becomes high enough. These trends are explained by a generalized form of particle balance equation, implying that the same trends for reactive species density would emerge in various plasma conditions. For the plasma size dependence, the electron density increases and the electron temperature decreases for increasing plasma size. Both become saturated when the plasma size becomes large enough. These trends of electron density and temperature are explained by the relative change of the diffusive loss. Our simulation results give a useful insight into the tendency of plasma properties over a wide range of plasma parameters. Cold plasma (dpeaa)DE-He213 Plasma modeling (dpeaa)DE-He213 Plasma simulation (dpeaa)DE-He213 Atmospheric pressure plasma (dpeaa)DE-He213 Lee, Jimo aut Yun, Gunsu aut Enthalten in Journal of the Korean Physical Society Berlin : Springer, 1968 82(2022), 1 vom: 13. Dez., Seite 32-39 (DE-627)328820865 (DE-600)2046361-3 1976-8524 nnns volume:82 year:2022 number:1 day:13 month:12 pages:32-39 https://dx.doi.org/10.1007/s40042-022-00686-6 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 82 2022 1 13 12 32-39
allfieldsSound	10.1007/s40042-022-00686-6 doi (DE-627)SPR051325721 (SPR)s40042-022-00686-6-e DE-627 ger DE-627 rakwb eng Jeong, Seokyong verfasserin aut General parametric dependence of atmospheric pressure argon plasmas 2022 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Korean Physical Society 2022. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Abstract Using a global model for atmospheric pressure plasma, we investigated general dependence of plasma properties on power density and plasma size. We built a global simulation for a pure argon cylindrical plasma and observed changes in plasma properties with the power density and plasma size. The study of the power dependence shows that the density of excited species is in general proportional to the power when the power density is low, whereas the density becomes saturated when the power density becomes high enough. These trends are explained by a generalized form of particle balance equation, implying that the same trends for reactive species density would emerge in various plasma conditions. For the plasma size dependence, the electron density increases and the electron temperature decreases for increasing plasma size. Both become saturated when the plasma size becomes large enough. These trends of electron density and temperature are explained by the relative change of the diffusive loss. Our simulation results give a useful insight into the tendency of plasma properties over a wide range of plasma parameters. Cold plasma (dpeaa)DE-He213 Plasma modeling (dpeaa)DE-He213 Plasma simulation (dpeaa)DE-He213 Atmospheric pressure plasma (dpeaa)DE-He213 Lee, Jimo aut Yun, Gunsu aut Enthalten in Journal of the Korean Physical Society Berlin : Springer, 1968 82(2022), 1 vom: 13. Dez., Seite 32-39 (DE-627)328820865 (DE-600)2046361-3 1976-8524 nnns volume:82 year:2022 number:1 day:13 month:12 pages:32-39 https://dx.doi.org/10.1007/s40042-022-00686-6 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 82 2022 1 13 12 32-39
language	English
source	Enthalten in Journal of the Korean Physical Society 82(2022), 1 vom: 13. Dez., Seite 32-39 volume:82 year:2022 number:1 day:13 month:12 pages:32-39
sourceStr	Enthalten in Journal of the Korean Physical Society 82(2022), 1 vom: 13. Dez., Seite 32-39 volume:82 year:2022 number:1 day:13 month:12 pages:32-39
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Cold plasma Plasma modeling Plasma simulation Atmospheric pressure plasma
isfreeaccess_bool	false
container_title	Journal of the Korean Physical Society
authorswithroles_txt_mv	Jeong, Seokyong @@aut@@ Lee, Jimo @@aut@@ Yun, Gunsu @@aut@@
publishDateDaySort_date	2022-12-13T00:00:00Z
hierarchy_top_id	328820865
id	SPR051325721
language_de	englisch
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author	Jeong, Seokyong
spellingShingle	Jeong, Seokyong misc Cold plasma misc Plasma modeling misc Plasma simulation misc Atmospheric pressure plasma General parametric dependence of atmospheric pressure argon plasmas
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topic_title	General parametric dependence of atmospheric pressure argon plasmas Cold plasma (dpeaa)DE-He213 Plasma modeling (dpeaa)DE-He213 Plasma simulation (dpeaa)DE-He213 Atmospheric pressure plasma (dpeaa)DE-He213
topic	misc Cold plasma misc Plasma modeling misc Plasma simulation misc Atmospheric pressure plasma
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title	General parametric dependence of atmospheric pressure argon plasmas
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title_full	General parametric dependence of atmospheric pressure argon plasmas
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author_browse	Jeong, Seokyong Lee, Jimo Yun, Gunsu
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doi_str_mv	10.1007/s40042-022-00686-6
title_sort	general parametric dependence of atmospheric pressure argon plasmas
title_auth	General parametric dependence of atmospheric pressure argon plasmas
abstract	Abstract Using a global model for atmospheric pressure plasma, we investigated general dependence of plasma properties on power density and plasma size. We built a global simulation for a pure argon cylindrical plasma and observed changes in plasma properties with the power density and plasma size. The study of the power dependence shows that the density of excited species is in general proportional to the power when the power density is low, whereas the density becomes saturated when the power density becomes high enough. These trends are explained by a generalized form of particle balance equation, implying that the same trends for reactive species density would emerge in various plasma conditions. For the plasma size dependence, the electron density increases and the electron temperature decreases for increasing plasma size. Both become saturated when the plasma size becomes large enough. These trends of electron density and temperature are explained by the relative change of the diffusive loss. Our simulation results give a useful insight into the tendency of plasma properties over a wide range of plasma parameters. © The Korean Physical Society 2022. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
abstractGer	Abstract Using a global model for atmospheric pressure plasma, we investigated general dependence of plasma properties on power density and plasma size. We built a global simulation for a pure argon cylindrical plasma and observed changes in plasma properties with the power density and plasma size. The study of the power dependence shows that the density of excited species is in general proportional to the power when the power density is low, whereas the density becomes saturated when the power density becomes high enough. These trends are explained by a generalized form of particle balance equation, implying that the same trends for reactive species density would emerge in various plasma conditions. For the plasma size dependence, the electron density increases and the electron temperature decreases for increasing plasma size. Both become saturated when the plasma size becomes large enough. These trends of electron density and temperature are explained by the relative change of the diffusive loss. Our simulation results give a useful insight into the tendency of plasma properties over a wide range of plasma parameters. © The Korean Physical Society 2022. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
abstract_unstemmed	Abstract Using a global model for atmospheric pressure plasma, we investigated general dependence of plasma properties on power density and plasma size. We built a global simulation for a pure argon cylindrical plasma and observed changes in plasma properties with the power density and plasma size. The study of the power dependence shows that the density of excited species is in general proportional to the power when the power density is low, whereas the density becomes saturated when the power density becomes high enough. These trends are explained by a generalized form of particle balance equation, implying that the same trends for reactive species density would emerge in various plasma conditions. For the plasma size dependence, the electron density increases and the electron temperature decreases for increasing plasma size. Both become saturated when the plasma size becomes large enough. These trends of electron density and temperature are explained by the relative change of the diffusive loss. Our simulation results give a useful insight into the tendency of plasma properties over a wide range of plasma parameters. © The Korean Physical Society 2022. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
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title_short	General parametric dependence of atmospheric pressure argon plasmas
url	https://dx.doi.org/10.1007/s40042-022-00686-6
remote_bool	true
author2	Lee, Jimo Yun, Gunsu
author2Str	Lee, Jimo Yun, Gunsu
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doi_str	10.1007/s40042-022-00686-6
up_date	2024-07-03T21:08:54.067Z
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Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Using a global model for atmospheric pressure plasma, we investigated general dependence of plasma properties on power density and plasma size. We built a global simulation for a pure argon cylindrical plasma and observed changes in plasma properties with the power density and plasma size. The study of the power dependence shows that the density of excited species is in general proportional to the power when the power density is low, whereas the density becomes saturated when the power density becomes high enough. 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