A HED Laboratory Astrophysics Testbed Comes of Age: JET Deflection via Cross Winds
Abstract We present new data from High-Energy Density (HED) laboratory experiments designed to explore the interaction of a heavy hypersonic radiative jet with a cross wind. The jets are generated with the MAGPIE pulsed power machine where converging conical plasma flows are produced from a cylindri...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Frank, A. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2005 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science + Business Media, Inc. 2005 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 298(2005), 1-2 vom: Juli, Seite 107-114 |
|---|---|
| Übergeordnetes Werk: |
volume:298 ; year:2005 ; number:1-2 ; month:07 ; pages:107-114 |
| Links: |
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| DOI / URN: |
10.1007/s10509-005-3919-z |
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| Katalog-ID: |
OLC2066245194 |
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| 245 | 1 | 0 | |a A HED Laboratory Astrophysics Testbed Comes of Age: JET Deflection via Cross Winds |
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| 520 | |a Abstract We present new data from High-Energy Density (HED) laboratory experiments designed to explore the interaction of a heavy hypersonic radiative jet with a cross wind. The jets are generated with the MAGPIE pulsed power machine where converging conical plasma flows are produced from a cylindrically symmetric array of inclined wires. Radiative hypersonic jets emerge from the convergence point. The cross wind is generated by ablation of a plastic foil via soft-X-rays from the plasma convergence region. Our experiments show that the jets are deflected by the action of the cross wind with the angle of deflection dependent on the proximity of the foil. Shocks within the jet beam are apparent in the data. Analysis of the data shows that the interaction of the jet and cross wind is collisional and therefore in the hydrodynamic regime. We consider the astrophysical relevance of these experiments applying published models of jet deflection developed for AGN and YSOs. We also present results of 3-D numerical simulations of jet deflection using a new astrophysical Adaptive Mesh Refinement code. These simulations show highly structured shocks occurring within the beam similar to what was observed in the experiments. | ||
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| 650 | 4 | |a methods: laboratory | |
| 650 | 4 | |a ISM: Herbig–Haro objects | |
| 650 | 4 | |a stars: winds | |
| 650 | 4 | |a outflows | |
| 700 | 1 | |a Blackman, E. G. |4 aut | |
| 700 | 1 | |a Cunningham, A. |4 aut | |
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| 700 | 1 | |a Ampleford, D. |4 aut | |
| 700 | 1 | |a Ciardi, A. |4 aut | |
| 700 | 1 | |a Bland, S. N. |4 aut | |
| 700 | 1 | |a Chittenden, J. P. |4 aut | |
| 700 | 1 | |a Haines, M. G. |4 aut | |
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10.1007/s10509-005-3919-z doi (DE-627)OLC2066245194 (DE-He213)s10509-005-3919-z-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Frank, A. verfasserin aut A HED Laboratory Astrophysics Testbed Comes of Age: JET Deflection via Cross Winds 2005 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science + Business Media, Inc. 2005 Abstract We present new data from High-Energy Density (HED) laboratory experiments designed to explore the interaction of a heavy hypersonic radiative jet with a cross wind. The jets are generated with the MAGPIE pulsed power machine where converging conical plasma flows are produced from a cylindrically symmetric array of inclined wires. Radiative hypersonic jets emerge from the convergence point. The cross wind is generated by ablation of a plastic foil via soft-X-rays from the plasma convergence region. Our experiments show that the jets are deflected by the action of the cross wind with the angle of deflection dependent on the proximity of the foil. Shocks within the jet beam are apparent in the data. Analysis of the data shows that the interaction of the jet and cross wind is collisional and therefore in the hydrodynamic regime. We consider the astrophysical relevance of these experiments applying published models of jet deflection developed for AGN and YSOs. We also present results of 3-D numerical simulations of jet deflection using a new astrophysical Adaptive Mesh Refinement code. These simulations show highly structured shocks occurring within the beam similar to what was observed in the experiments. hydrodynamics methods: laboratory ISM: Herbig–Haro objects stars: winds outflows Blackman, E. G. aut Cunningham, A. aut Lebedev, S. V. aut Ampleford, D. aut Ciardi, A. aut Bland, S. N. aut Chittenden, J. P. aut Haines, M. G. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 298(2005), 1-2 vom: Juli, Seite 107-114 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:298 year:2005 number:1-2 month:07 pages:107-114 https://doi.org/10.1007/s10509-005-3919-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 298 2005 1-2 07 107-114 |
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10.1007/s10509-005-3919-z doi (DE-627)OLC2066245194 (DE-He213)s10509-005-3919-z-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Frank, A. verfasserin aut A HED Laboratory Astrophysics Testbed Comes of Age: JET Deflection via Cross Winds 2005 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science + Business Media, Inc. 2005 Abstract We present new data from High-Energy Density (HED) laboratory experiments designed to explore the interaction of a heavy hypersonic radiative jet with a cross wind. The jets are generated with the MAGPIE pulsed power machine where converging conical plasma flows are produced from a cylindrically symmetric array of inclined wires. Radiative hypersonic jets emerge from the convergence point. The cross wind is generated by ablation of a plastic foil via soft-X-rays from the plasma convergence region. Our experiments show that the jets are deflected by the action of the cross wind with the angle of deflection dependent on the proximity of the foil. Shocks within the jet beam are apparent in the data. Analysis of the data shows that the interaction of the jet and cross wind is collisional and therefore in the hydrodynamic regime. We consider the astrophysical relevance of these experiments applying published models of jet deflection developed for AGN and YSOs. We also present results of 3-D numerical simulations of jet deflection using a new astrophysical Adaptive Mesh Refinement code. These simulations show highly structured shocks occurring within the beam similar to what was observed in the experiments. hydrodynamics methods: laboratory ISM: Herbig–Haro objects stars: winds outflows Blackman, E. G. aut Cunningham, A. aut Lebedev, S. V. aut Ampleford, D. aut Ciardi, A. aut Bland, S. N. aut Chittenden, J. P. aut Haines, M. G. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 298(2005), 1-2 vom: Juli, Seite 107-114 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:298 year:2005 number:1-2 month:07 pages:107-114 https://doi.org/10.1007/s10509-005-3919-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 298 2005 1-2 07 107-114 |
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10.1007/s10509-005-3919-z doi (DE-627)OLC2066245194 (DE-He213)s10509-005-3919-z-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Frank, A. verfasserin aut A HED Laboratory Astrophysics Testbed Comes of Age: JET Deflection via Cross Winds 2005 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science + Business Media, Inc. 2005 Abstract We present new data from High-Energy Density (HED) laboratory experiments designed to explore the interaction of a heavy hypersonic radiative jet with a cross wind. The jets are generated with the MAGPIE pulsed power machine where converging conical plasma flows are produced from a cylindrically symmetric array of inclined wires. Radiative hypersonic jets emerge from the convergence point. The cross wind is generated by ablation of a plastic foil via soft-X-rays from the plasma convergence region. Our experiments show that the jets are deflected by the action of the cross wind with the angle of deflection dependent on the proximity of the foil. Shocks within the jet beam are apparent in the data. Analysis of the data shows that the interaction of the jet and cross wind is collisional and therefore in the hydrodynamic regime. We consider the astrophysical relevance of these experiments applying published models of jet deflection developed for AGN and YSOs. We also present results of 3-D numerical simulations of jet deflection using a new astrophysical Adaptive Mesh Refinement code. These simulations show highly structured shocks occurring within the beam similar to what was observed in the experiments. hydrodynamics methods: laboratory ISM: Herbig–Haro objects stars: winds outflows Blackman, E. G. aut Cunningham, A. aut Lebedev, S. V. aut Ampleford, D. aut Ciardi, A. aut Bland, S. N. aut Chittenden, J. P. aut Haines, M. G. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 298(2005), 1-2 vom: Juli, Seite 107-114 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:298 year:2005 number:1-2 month:07 pages:107-114 https://doi.org/10.1007/s10509-005-3919-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 298 2005 1-2 07 107-114 |
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10.1007/s10509-005-3919-z doi (DE-627)OLC2066245194 (DE-He213)s10509-005-3919-z-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Frank, A. verfasserin aut A HED Laboratory Astrophysics Testbed Comes of Age: JET Deflection via Cross Winds 2005 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science + Business Media, Inc. 2005 Abstract We present new data from High-Energy Density (HED) laboratory experiments designed to explore the interaction of a heavy hypersonic radiative jet with a cross wind. The jets are generated with the MAGPIE pulsed power machine where converging conical plasma flows are produced from a cylindrically symmetric array of inclined wires. Radiative hypersonic jets emerge from the convergence point. The cross wind is generated by ablation of a plastic foil via soft-X-rays from the plasma convergence region. Our experiments show that the jets are deflected by the action of the cross wind with the angle of deflection dependent on the proximity of the foil. Shocks within the jet beam are apparent in the data. Analysis of the data shows that the interaction of the jet and cross wind is collisional and therefore in the hydrodynamic regime. We consider the astrophysical relevance of these experiments applying published models of jet deflection developed for AGN and YSOs. We also present results of 3-D numerical simulations of jet deflection using a new astrophysical Adaptive Mesh Refinement code. These simulations show highly structured shocks occurring within the beam similar to what was observed in the experiments. hydrodynamics methods: laboratory ISM: Herbig–Haro objects stars: winds outflows Blackman, E. G. aut Cunningham, A. aut Lebedev, S. V. aut Ampleford, D. aut Ciardi, A. aut Bland, S. N. aut Chittenden, J. P. aut Haines, M. G. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 298(2005), 1-2 vom: Juli, Seite 107-114 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:298 year:2005 number:1-2 month:07 pages:107-114 https://doi.org/10.1007/s10509-005-3919-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 298 2005 1-2 07 107-114 |
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10.1007/s10509-005-3919-z doi (DE-627)OLC2066245194 (DE-He213)s10509-005-3919-z-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Frank, A. verfasserin aut A HED Laboratory Astrophysics Testbed Comes of Age: JET Deflection via Cross Winds 2005 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science + Business Media, Inc. 2005 Abstract We present new data from High-Energy Density (HED) laboratory experiments designed to explore the interaction of a heavy hypersonic radiative jet with a cross wind. The jets are generated with the MAGPIE pulsed power machine where converging conical plasma flows are produced from a cylindrically symmetric array of inclined wires. Radiative hypersonic jets emerge from the convergence point. The cross wind is generated by ablation of a plastic foil via soft-X-rays from the plasma convergence region. Our experiments show that the jets are deflected by the action of the cross wind with the angle of deflection dependent on the proximity of the foil. Shocks within the jet beam are apparent in the data. Analysis of the data shows that the interaction of the jet and cross wind is collisional and therefore in the hydrodynamic regime. We consider the astrophysical relevance of these experiments applying published models of jet deflection developed for AGN and YSOs. We also present results of 3-D numerical simulations of jet deflection using a new astrophysical Adaptive Mesh Refinement code. These simulations show highly structured shocks occurring within the beam similar to what was observed in the experiments. hydrodynamics methods: laboratory ISM: Herbig–Haro objects stars: winds outflows Blackman, E. G. aut Cunningham, A. aut Lebedev, S. V. aut Ampleford, D. aut Ciardi, A. aut Bland, S. N. aut Chittenden, J. P. aut Haines, M. G. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 298(2005), 1-2 vom: Juli, Seite 107-114 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:298 year:2005 number:1-2 month:07 pages:107-114 https://doi.org/10.1007/s10509-005-3919-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 298 2005 1-2 07 107-114 |
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Enthalten in Astrophysics and space science 298(2005), 1-2 vom: Juli, Seite 107-114 volume:298 year:2005 number:1-2 month:07 pages:107-114 |
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a hed laboratory astrophysics testbed comes of age: jet deflection via cross winds |
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A HED Laboratory Astrophysics Testbed Comes of Age: JET Deflection via Cross Winds |
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Abstract We present new data from High-Energy Density (HED) laboratory experiments designed to explore the interaction of a heavy hypersonic radiative jet with a cross wind. The jets are generated with the MAGPIE pulsed power machine where converging conical plasma flows are produced from a cylindrically symmetric array of inclined wires. Radiative hypersonic jets emerge from the convergence point. The cross wind is generated by ablation of a plastic foil via soft-X-rays from the plasma convergence region. Our experiments show that the jets are deflected by the action of the cross wind with the angle of deflection dependent on the proximity of the foil. Shocks within the jet beam are apparent in the data. Analysis of the data shows that the interaction of the jet and cross wind is collisional and therefore in the hydrodynamic regime. We consider the astrophysical relevance of these experiments applying published models of jet deflection developed for AGN and YSOs. We also present results of 3-D numerical simulations of jet deflection using a new astrophysical Adaptive Mesh Refinement code. These simulations show highly structured shocks occurring within the beam similar to what was observed in the experiments. © Springer Science + Business Media, Inc. 2005 |
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Abstract We present new data from High-Energy Density (HED) laboratory experiments designed to explore the interaction of a heavy hypersonic radiative jet with a cross wind. The jets are generated with the MAGPIE pulsed power machine where converging conical plasma flows are produced from a cylindrically symmetric array of inclined wires. Radiative hypersonic jets emerge from the convergence point. The cross wind is generated by ablation of a plastic foil via soft-X-rays from the plasma convergence region. Our experiments show that the jets are deflected by the action of the cross wind with the angle of deflection dependent on the proximity of the foil. Shocks within the jet beam are apparent in the data. Analysis of the data shows that the interaction of the jet and cross wind is collisional and therefore in the hydrodynamic regime. We consider the astrophysical relevance of these experiments applying published models of jet deflection developed for AGN and YSOs. We also present results of 3-D numerical simulations of jet deflection using a new astrophysical Adaptive Mesh Refinement code. These simulations show highly structured shocks occurring within the beam similar to what was observed in the experiments. © Springer Science + Business Media, Inc. 2005 |
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Abstract We present new data from High-Energy Density (HED) laboratory experiments designed to explore the interaction of a heavy hypersonic radiative jet with a cross wind. The jets are generated with the MAGPIE pulsed power machine where converging conical plasma flows are produced from a cylindrically symmetric array of inclined wires. Radiative hypersonic jets emerge from the convergence point. The cross wind is generated by ablation of a plastic foil via soft-X-rays from the plasma convergence region. Our experiments show that the jets are deflected by the action of the cross wind with the angle of deflection dependent on the proximity of the foil. Shocks within the jet beam are apparent in the data. Analysis of the data shows that the interaction of the jet and cross wind is collisional and therefore in the hydrodynamic regime. We consider the astrophysical relevance of these experiments applying published models of jet deflection developed for AGN and YSOs. We also present results of 3-D numerical simulations of jet deflection using a new astrophysical Adaptive Mesh Refinement code. These simulations show highly structured shocks occurring within the beam similar to what was observed in the experiments. © Springer Science + Business Media, Inc. 2005 |
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