Structure of a Magnetic Flux Annihilation Layer Formed by the Collision of Supersonic, Magnetized Plasma Flows

We present experiments characterizing the detailed structure of a current layer, generated by the collision of two counterstreaming, supersonic and magnetized aluminum plasma flows. The antiparallel magnetic fields advected by the flows are found to be mutually annihilated inside the layer, giving r...
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Autor*in:	Suttle, L G [verfasserIn] Hare, J D Lebedev, S V Swadling, G F Burdiak, G C Ciardi, A Chittenden, J P Loureiro, N F Niasse, N Suzuki-Vidal, F Wu, J Yang, Q Clayson, T Frank, A Robinson, T S Smith, R A Stuart, N

Format:	Artikel
Sprache:	Englisch

Erschienen:	2016

Systematik:	UA 1000

Übergeordnetes Werk:	Enthalten in: Physical review letters - Ridge, NY : American Physical Society, 1958, 116(2016), 22
Übergeordnetes Werk:	volume:116 ; year:2016 ; number:22

Links:	Volltext Link aufrufen

DOI / URN:	10.1103/PhysRevLett.116.225001

Katalog-ID:	OLC1976633583

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520			\|a We present experiments characterizing the detailed structure of a current layer, generated by the collision of two counterstreaming, supersonic and magnetized aluminum plasma flows. The antiparallel magnetic fields advected by the flows are found to be mutually annihilated inside the layer, giving rise to a bifurcated current structure-two narrow current sheets running along the outside surfaces of the layer. Measurements with Thomson scattering show a fast outflow of plasma along the layer and a high ion temperature (T_{i}∼Z[over ¯]T_{e}, with average ionization Z[over ¯]=7). Analysis of the spatially resolved plasma parameters indicates that the advection and subsequent annihilation of the inflowing magnetic flux determines the structure of the layer, while the ion heating could be due to the development of kinetic, current-driven instabilities.
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700	1		\|a Suzuki-Vidal, F \|4 oth
700	1		\|a Wu, J \|4 oth
700	1		\|a Yang, Q \|4 oth
700	1		\|a Clayson, T \|4 oth
700	1		\|a Frank, A \|4 oth
700	1		\|a Robinson, T S \|4 oth
700	1		\|a Smith, R A \|4 oth
700	1		\|a Stuart, N \|4 oth
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allfields	10.1103/PhysRevLett.116.225001 doi PQ20160719 (DE-627)OLC1976633583 (DE-599)GBVOLC1976633583 (PRQ)c1303-33a6d703d88380798b46fd347c47bec2d6d89185f8548bdeb2d1b1ce42de71d20 (KEY)0009201020160000116002200000structureofamagneticfluxannihilationlayerformedbyt DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk Suttle, L G verfasserin aut Structure of a Magnetic Flux Annihilation Layer Formed by the Collision of Supersonic, Magnetized Plasma Flows 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier We present experiments characterizing the detailed structure of a current layer, generated by the collision of two counterstreaming, supersonic and magnetized aluminum plasma flows. The antiparallel magnetic fields advected by the flows are found to be mutually annihilated inside the layer, giving rise to a bifurcated current structure-two narrow current sheets running along the outside surfaces of the layer. Measurements with Thomson scattering show a fast outflow of plasma along the layer and a high ion temperature (T_{i}∼Z[over ¯]T_{e}, with average ionization Z[over ¯]=7). Analysis of the spatially resolved plasma parameters indicates that the advection and subsequent annihilation of the inflowing magnetic flux determines the structure of the layer, while the ion heating could be due to the development of kinetic, current-driven instabilities. Hare, J D oth Lebedev, S V oth Swadling, G F oth Burdiak, G C oth Ciardi, A oth Chittenden, J P oth Loureiro, N F oth Niasse, N oth Suzuki-Vidal, F oth Wu, J oth Yang, Q oth Clayson, T oth Frank, A oth Robinson, T S oth Smith, R A oth Stuart, N oth Enthalten in Physical review letters Ridge, NY : American Physical Society, 1958 116(2016), 22 (DE-627)129503959 (DE-600)208853-8 (DE-576)014907267 0031-9007 nnns volume:116 year:2016 number:22 http://dx.doi.org/10.1103/PhysRevLett.116.225001 Volltext http://www.ncbi.nlm.nih.gov/pubmed/27314720 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2004 GBV_ILN_2016 GBV_ILN_2095 GBV_ILN_2192 GBV_ILN_2279 GBV_ILN_2286 UA 1000 AR 116 2016 22
spelling	10.1103/PhysRevLett.116.225001 doi PQ20160719 (DE-627)OLC1976633583 (DE-599)GBVOLC1976633583 (PRQ)c1303-33a6d703d88380798b46fd347c47bec2d6d89185f8548bdeb2d1b1ce42de71d20 (KEY)0009201020160000116002200000structureofamagneticfluxannihilationlayerformedbyt DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk Suttle, L G verfasserin aut Structure of a Magnetic Flux Annihilation Layer Formed by the Collision of Supersonic, Magnetized Plasma Flows 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier We present experiments characterizing the detailed structure of a current layer, generated by the collision of two counterstreaming, supersonic and magnetized aluminum plasma flows. The antiparallel magnetic fields advected by the flows are found to be mutually annihilated inside the layer, giving rise to a bifurcated current structure-two narrow current sheets running along the outside surfaces of the layer. Measurements with Thomson scattering show a fast outflow of plasma along the layer and a high ion temperature (T_{i}∼Z[over ¯]T_{e}, with average ionization Z[over ¯]=7). Analysis of the spatially resolved plasma parameters indicates that the advection and subsequent annihilation of the inflowing magnetic flux determines the structure of the layer, while the ion heating could be due to the development of kinetic, current-driven instabilities. Hare, J D oth Lebedev, S V oth Swadling, G F oth Burdiak, G C oth Ciardi, A oth Chittenden, J P oth Loureiro, N F oth Niasse, N oth Suzuki-Vidal, F oth Wu, J oth Yang, Q oth Clayson, T oth Frank, A oth Robinson, T S oth Smith, R A oth Stuart, N oth Enthalten in Physical review letters Ridge, NY : American Physical Society, 1958 116(2016), 22 (DE-627)129503959 (DE-600)208853-8 (DE-576)014907267 0031-9007 nnns volume:116 year:2016 number:22 http://dx.doi.org/10.1103/PhysRevLett.116.225001 Volltext http://www.ncbi.nlm.nih.gov/pubmed/27314720 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2004 GBV_ILN_2016 GBV_ILN_2095 GBV_ILN_2192 GBV_ILN_2279 GBV_ILN_2286 UA 1000 AR 116 2016 22
allfields_unstemmed	10.1103/PhysRevLett.116.225001 doi PQ20160719 (DE-627)OLC1976633583 (DE-599)GBVOLC1976633583 (PRQ)c1303-33a6d703d88380798b46fd347c47bec2d6d89185f8548bdeb2d1b1ce42de71d20 (KEY)0009201020160000116002200000structureofamagneticfluxannihilationlayerformedbyt DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk Suttle, L G verfasserin aut Structure of a Magnetic Flux Annihilation Layer Formed by the Collision of Supersonic, Magnetized Plasma Flows 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier We present experiments characterizing the detailed structure of a current layer, generated by the collision of two counterstreaming, supersonic and magnetized aluminum plasma flows. The antiparallel magnetic fields advected by the flows are found to be mutually annihilated inside the layer, giving rise to a bifurcated current structure-two narrow current sheets running along the outside surfaces of the layer. Measurements with Thomson scattering show a fast outflow of plasma along the layer and a high ion temperature (T_{i}∼Z[over ¯]T_{e}, with average ionization Z[over ¯]=7). Analysis of the spatially resolved plasma parameters indicates that the advection and subsequent annihilation of the inflowing magnetic flux determines the structure of the layer, while the ion heating could be due to the development of kinetic, current-driven instabilities. Hare, J D oth Lebedev, S V oth Swadling, G F oth Burdiak, G C oth Ciardi, A oth Chittenden, J P oth Loureiro, N F oth Niasse, N oth Suzuki-Vidal, F oth Wu, J oth Yang, Q oth Clayson, T oth Frank, A oth Robinson, T S oth Smith, R A oth Stuart, N oth Enthalten in Physical review letters Ridge, NY : American Physical Society, 1958 116(2016), 22 (DE-627)129503959 (DE-600)208853-8 (DE-576)014907267 0031-9007 nnns volume:116 year:2016 number:22 http://dx.doi.org/10.1103/PhysRevLett.116.225001 Volltext http://www.ncbi.nlm.nih.gov/pubmed/27314720 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2004 GBV_ILN_2016 GBV_ILN_2095 GBV_ILN_2192 GBV_ILN_2279 GBV_ILN_2286 UA 1000 AR 116 2016 22
allfieldsGer	10.1103/PhysRevLett.116.225001 doi PQ20160719 (DE-627)OLC1976633583 (DE-599)GBVOLC1976633583 (PRQ)c1303-33a6d703d88380798b46fd347c47bec2d6d89185f8548bdeb2d1b1ce42de71d20 (KEY)0009201020160000116002200000structureofamagneticfluxannihilationlayerformedbyt DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk Suttle, L G verfasserin aut Structure of a Magnetic Flux Annihilation Layer Formed by the Collision of Supersonic, Magnetized Plasma Flows 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier We present experiments characterizing the detailed structure of a current layer, generated by the collision of two counterstreaming, supersonic and magnetized aluminum plasma flows. The antiparallel magnetic fields advected by the flows are found to be mutually annihilated inside the layer, giving rise to a bifurcated current structure-two narrow current sheets running along the outside surfaces of the layer. Measurements with Thomson scattering show a fast outflow of plasma along the layer and a high ion temperature (T_{i}∼Z[over ¯]T_{e}, with average ionization Z[over ¯]=7). Analysis of the spatially resolved plasma parameters indicates that the advection and subsequent annihilation of the inflowing magnetic flux determines the structure of the layer, while the ion heating could be due to the development of kinetic, current-driven instabilities. Hare, J D oth Lebedev, S V oth Swadling, G F oth Burdiak, G C oth Ciardi, A oth Chittenden, J P oth Loureiro, N F oth Niasse, N oth Suzuki-Vidal, F oth Wu, J oth Yang, Q oth Clayson, T oth Frank, A oth Robinson, T S oth Smith, R A oth Stuart, N oth Enthalten in Physical review letters Ridge, NY : American Physical Society, 1958 116(2016), 22 (DE-627)129503959 (DE-600)208853-8 (DE-576)014907267 0031-9007 nnns volume:116 year:2016 number:22 http://dx.doi.org/10.1103/PhysRevLett.116.225001 Volltext http://www.ncbi.nlm.nih.gov/pubmed/27314720 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2004 GBV_ILN_2016 GBV_ILN_2095 GBV_ILN_2192 GBV_ILN_2279 GBV_ILN_2286 UA 1000 AR 116 2016 22
allfieldsSound	10.1103/PhysRevLett.116.225001 doi PQ20160719 (DE-627)OLC1976633583 (DE-599)GBVOLC1976633583 (PRQ)c1303-33a6d703d88380798b46fd347c47bec2d6d89185f8548bdeb2d1b1ce42de71d20 (KEY)0009201020160000116002200000structureofamagneticfluxannihilationlayerformedbyt DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk Suttle, L G verfasserin aut Structure of a Magnetic Flux Annihilation Layer Formed by the Collision of Supersonic, Magnetized Plasma Flows 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier We present experiments characterizing the detailed structure of a current layer, generated by the collision of two counterstreaming, supersonic and magnetized aluminum plasma flows. The antiparallel magnetic fields advected by the flows are found to be mutually annihilated inside the layer, giving rise to a bifurcated current structure-two narrow current sheets running along the outside surfaces of the layer. Measurements with Thomson scattering show a fast outflow of plasma along the layer and a high ion temperature (T_{i}∼Z[over ¯]T_{e}, with average ionization Z[over ¯]=7). Analysis of the spatially resolved plasma parameters indicates that the advection and subsequent annihilation of the inflowing magnetic flux determines the structure of the layer, while the ion heating could be due to the development of kinetic, current-driven instabilities. Hare, J D oth Lebedev, S V oth Swadling, G F oth Burdiak, G C oth Ciardi, A oth Chittenden, J P oth Loureiro, N F oth Niasse, N oth Suzuki-Vidal, F oth Wu, J oth Yang, Q oth Clayson, T oth Frank, A oth Robinson, T S oth Smith, R A oth Stuart, N oth Enthalten in Physical review letters Ridge, NY : American Physical Society, 1958 116(2016), 22 (DE-627)129503959 (DE-600)208853-8 (DE-576)014907267 0031-9007 nnns volume:116 year:2016 number:22 http://dx.doi.org/10.1103/PhysRevLett.116.225001 Volltext http://www.ncbi.nlm.nih.gov/pubmed/27314720 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2004 GBV_ILN_2016 GBV_ILN_2095 GBV_ILN_2192 GBV_ILN_2279 GBV_ILN_2286 UA 1000 AR 116 2016 22
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author	Suttle, L G
spellingShingle	Suttle, L G ddc 550 rvk UA 1000 Structure of a Magnetic Flux Annihilation Layer Formed by the Collision of Supersonic, Magnetized Plasma Flows
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topic_title	550 DNB UA 1000 AVZ rvk Structure of a Magnetic Flux Annihilation Layer Formed by the Collision of Supersonic, Magnetized Plasma Flows
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title	Structure of a Magnetic Flux Annihilation Layer Formed by the Collision of Supersonic, Magnetized Plasma Flows
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title_full	Structure of a Magnetic Flux Annihilation Layer Formed by the Collision of Supersonic, Magnetized Plasma Flows
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title_sort	structure of a magnetic flux annihilation layer formed by the collision of supersonic, magnetized plasma flows
title_auth	Structure of a Magnetic Flux Annihilation Layer Formed by the Collision of Supersonic, Magnetized Plasma Flows
abstract	We present experiments characterizing the detailed structure of a current layer, generated by the collision of two counterstreaming, supersonic and magnetized aluminum plasma flows. The antiparallel magnetic fields advected by the flows are found to be mutually annihilated inside the layer, giving rise to a bifurcated current structure-two narrow current sheets running along the outside surfaces of the layer. Measurements with Thomson scattering show a fast outflow of plasma along the layer and a high ion temperature (T_{i}∼Z[over ¯]T_{e}, with average ionization Z[over ¯]=7). Analysis of the spatially resolved plasma parameters indicates that the advection and subsequent annihilation of the inflowing magnetic flux determines the structure of the layer, while the ion heating could be due to the development of kinetic, current-driven instabilities.
abstractGer	We present experiments characterizing the detailed structure of a current layer, generated by the collision of two counterstreaming, supersonic and magnetized aluminum plasma flows. The antiparallel magnetic fields advected by the flows are found to be mutually annihilated inside the layer, giving rise to a bifurcated current structure-two narrow current sheets running along the outside surfaces of the layer. Measurements with Thomson scattering show a fast outflow of plasma along the layer and a high ion temperature (T_{i}∼Z[over ¯]T_{e}, with average ionization Z[over ¯]=7). Analysis of the spatially resolved plasma parameters indicates that the advection and subsequent annihilation of the inflowing magnetic flux determines the structure of the layer, while the ion heating could be due to the development of kinetic, current-driven instabilities.
abstract_unstemmed	We present experiments characterizing the detailed structure of a current layer, generated by the collision of two counterstreaming, supersonic and magnetized aluminum plasma flows. The antiparallel magnetic fields advected by the flows are found to be mutually annihilated inside the layer, giving rise to a bifurcated current structure-two narrow current sheets running along the outside surfaces of the layer. Measurements with Thomson scattering show a fast outflow of plasma along the layer and a high ion temperature (T_{i}∼Z[over ¯]T_{e}, with average ionization Z[over ¯]=7). Analysis of the spatially resolved plasma parameters indicates that the advection and subsequent annihilation of the inflowing magnetic flux determines the structure of the layer, while the ion heating could be due to the development of kinetic, current-driven instabilities.
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container_issue	22
title_short	Structure of a Magnetic Flux Annihilation Layer Formed by the Collision of Supersonic, Magnetized Plasma Flows
url	http://dx.doi.org/10.1103/PhysRevLett.116.225001 http://www.ncbi.nlm.nih.gov/pubmed/27314720
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author2	Hare, J D Lebedev, S V Swadling, G F Burdiak, G C Ciardi, A Chittenden, J P Loureiro, N F Niasse, N Suzuki-Vidal, F Wu, J Yang, Q Clayson, T Frank, A Robinson, T S Smith, R A Stuart, N
author2Str	Hare, J D Lebedev, S V Swadling, G F Burdiak, G C Ciardi, A Chittenden, J P Loureiro, N F Niasse, N Suzuki-Vidal, F Wu, J Yang, Q Clayson, T Frank, A Robinson, T S Smith, R A Stuart, N
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doi_str	10.1103/PhysRevLett.116.225001
up_date	2024-07-03T16:15:42.818Z
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