3D MHD Simulations of Laboratory Plasma Jets
Abstract Jets and outflows are thought to be an integral part of accretion phenomena and are associated with a large variety of objects. In these systems, the interaction of magnetic fields with an accretion disk and/or a magnetized central object is thought to be responsible for the acceleration an...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Ciardi, A. [verfasserIn] Lebedev, S. V. [verfasserIn] Frank, A. [verfasserIn] Blackman, E. G. [verfasserIn] Ampleford, D. J. [verfasserIn] Jennings, C. A. [verfasserIn] Chittenden, J. P. [verfasserIn] Lery, T. [verfasserIn] Bland, S. N. [verfasserIn] Bott, S. C. [verfasserIn] Hall, G. N. [verfasserIn] Rapley, J. [verfasserIn] Vidal, F. A. Suzuki [verfasserIn] Marocchino, A. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2006 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Dordrecht [u.a.] : Springer Science + Business Media B.V, 1968, 307(2006), 1-3 vom: 15. Nov., Seite 17-22 |
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| Übergeordnetes Werk: |
volume:307 ; year:2006 ; number:1-3 ; day:15 ; month:11 ; pages:17-22 |
| Links: |
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| DOI / URN: |
10.1007/s10509-006-9215-8 |
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| Katalog-ID: |
SPR010570969 |
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| 520 | |a Abstract Jets and outflows are thought to be an integral part of accretion phenomena and are associated with a large variety of objects. In these systems, the interaction of magnetic fields with an accretion disk and/or a magnetized central object is thought to be responsible for the acceleration and collimation of plasma into jets and wider angle flows. In this paper we present three-dimensional MHD simulations of magnetically driven, radiatively cooled laboratory jets that are produced on the MAGPIE experimental facility. The general outflow structure comprises an expanding magnetic cavity which is collimated by the pressure of an extended plasma background medium, and a magnetically confined jet which develops within the magnetic cavity. Although this structure is intrinsically transient and instabilities in the jet and disruption of the magnetic cavity ultimately lead to its break-up, a well collimated, “knotty” jet still emerges from the system; such clumpy morphology is reminiscent of that observed in many astrophysical jets. The possible introduction in the experiments of angular momentum and axial magnetic field will also be discussed. | ||
| 650 | 4 | |a MHD plasmas |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Accretion |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Accretion discs |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Laboratory astrophysics |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Winds |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Jets and outflows |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Lebedev, S. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Frank, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Blackman, E. G. |e verfasserin |4 aut | |
| 700 | 1 | |a Ampleford, D. J. |e verfasserin |4 aut | |
| 700 | 1 | |a Jennings, C. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Chittenden, J. P. |e verfasserin |4 aut | |
| 700 | 1 | |a Lery, T. |e verfasserin |4 aut | |
| 700 | 1 | |a Bland, S. N. |e verfasserin |4 aut | |
| 700 | 1 | |a Bott, S. C. |e verfasserin |4 aut | |
| 700 | 1 | |a Hall, G. N. |e verfasserin |4 aut | |
| 700 | 1 | |a Rapley, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Vidal, F. A. Suzuki |e verfasserin |4 aut | |
| 700 | 1 | |a Marocchino, A. |e verfasserin |4 aut | |
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10.1007/s10509-006-9215-8 doi (DE-627)SPR010570969 (SPR)s10509-006-9215-8-e DE-627 ger DE-627 rakwb eng 520 530 620 ASE 39.00 bkl 39.22 bkl Ciardi, A. verfasserin aut 3D MHD Simulations of Laboratory Plasma Jets 2006 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Jets and outflows are thought to be an integral part of accretion phenomena and are associated with a large variety of objects. In these systems, the interaction of magnetic fields with an accretion disk and/or a magnetized central object is thought to be responsible for the acceleration and collimation of plasma into jets and wider angle flows. In this paper we present three-dimensional MHD simulations of magnetically driven, radiatively cooled laboratory jets that are produced on the MAGPIE experimental facility. The general outflow structure comprises an expanding magnetic cavity which is collimated by the pressure of an extended plasma background medium, and a magnetically confined jet which develops within the magnetic cavity. Although this structure is intrinsically transient and instabilities in the jet and disruption of the magnetic cavity ultimately lead to its break-up, a well collimated, “knotty” jet still emerges from the system; such clumpy morphology is reminiscent of that observed in many astrophysical jets. The possible introduction in the experiments of angular momentum and axial magnetic field will also be discussed. MHD plasmas (dpeaa)DE-He213 Accretion (dpeaa)DE-He213 Accretion discs (dpeaa)DE-He213 Laboratory astrophysics (dpeaa)DE-He213 Winds (dpeaa)DE-He213 Jets and outflows (dpeaa)DE-He213 Lebedev, S. V. verfasserin aut Frank, A. verfasserin aut Blackman, E. G. verfasserin aut Ampleford, D. J. verfasserin aut Jennings, C. A. verfasserin aut Chittenden, J. P. verfasserin aut Lery, T. verfasserin aut Bland, S. N. verfasserin aut Bott, S. C. verfasserin aut Hall, G. N. verfasserin aut Rapley, J. verfasserin aut Vidal, F. A. Suzuki verfasserin aut Marocchino, A. verfasserin aut Enthalten in Astrophysics and space science Dordrecht [u.a.] : Springer Science + Business Media B.V, 1968 307(2006), 1-3 vom: 15. Nov., Seite 17-22 (DE-627)268755868 (DE-600)1472548-4 1572-946X nnns volume:307 year:2006 number:1-3 day:15 month:11 pages:17-22 https://dx.doi.org/10.1007/s10509-006-9215-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE 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_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_206 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_2070 GBV_ILN_2086 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_2116 GBV_ILN_2118 GBV_ILN_2119 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_4012 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_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE 39.22 ASE AR 307 2006 1-3 15 11 17-22 |
| spelling |
10.1007/s10509-006-9215-8 doi (DE-627)SPR010570969 (SPR)s10509-006-9215-8-e DE-627 ger DE-627 rakwb eng 520 530 620 ASE 39.00 bkl 39.22 bkl Ciardi, A. verfasserin aut 3D MHD Simulations of Laboratory Plasma Jets 2006 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Jets and outflows are thought to be an integral part of accretion phenomena and are associated with a large variety of objects. In these systems, the interaction of magnetic fields with an accretion disk and/or a magnetized central object is thought to be responsible for the acceleration and collimation of plasma into jets and wider angle flows. In this paper we present three-dimensional MHD simulations of magnetically driven, radiatively cooled laboratory jets that are produced on the MAGPIE experimental facility. The general outflow structure comprises an expanding magnetic cavity which is collimated by the pressure of an extended plasma background medium, and a magnetically confined jet which develops within the magnetic cavity. Although this structure is intrinsically transient and instabilities in the jet and disruption of the magnetic cavity ultimately lead to its break-up, a well collimated, “knotty” jet still emerges from the system; such clumpy morphology is reminiscent of that observed in many astrophysical jets. The possible introduction in the experiments of angular momentum and axial magnetic field will also be discussed. MHD plasmas (dpeaa)DE-He213 Accretion (dpeaa)DE-He213 Accretion discs (dpeaa)DE-He213 Laboratory astrophysics (dpeaa)DE-He213 Winds (dpeaa)DE-He213 Jets and outflows (dpeaa)DE-He213 Lebedev, S. V. verfasserin aut Frank, A. verfasserin aut Blackman, E. G. verfasserin aut Ampleford, D. J. verfasserin aut Jennings, C. A. verfasserin aut Chittenden, J. P. verfasserin aut Lery, T. verfasserin aut Bland, S. N. verfasserin aut Bott, S. C. verfasserin aut Hall, G. N. verfasserin aut Rapley, J. verfasserin aut Vidal, F. A. Suzuki verfasserin aut Marocchino, A. verfasserin aut Enthalten in Astrophysics and space science Dordrecht [u.a.] : Springer Science + Business Media B.V, 1968 307(2006), 1-3 vom: 15. Nov., Seite 17-22 (DE-627)268755868 (DE-600)1472548-4 1572-946X nnns volume:307 year:2006 number:1-3 day:15 month:11 pages:17-22 https://dx.doi.org/10.1007/s10509-006-9215-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE 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_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_206 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_2070 GBV_ILN_2086 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_2116 GBV_ILN_2118 GBV_ILN_2119 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_4012 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_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE 39.22 ASE AR 307 2006 1-3 15 11 17-22 |
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10.1007/s10509-006-9215-8 doi (DE-627)SPR010570969 (SPR)s10509-006-9215-8-e DE-627 ger DE-627 rakwb eng 520 530 620 ASE 39.00 bkl 39.22 bkl Ciardi, A. verfasserin aut 3D MHD Simulations of Laboratory Plasma Jets 2006 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Jets and outflows are thought to be an integral part of accretion phenomena and are associated with a large variety of objects. In these systems, the interaction of magnetic fields with an accretion disk and/or a magnetized central object is thought to be responsible for the acceleration and collimation of plasma into jets and wider angle flows. In this paper we present three-dimensional MHD simulations of magnetically driven, radiatively cooled laboratory jets that are produced on the MAGPIE experimental facility. The general outflow structure comprises an expanding magnetic cavity which is collimated by the pressure of an extended plasma background medium, and a magnetically confined jet which develops within the magnetic cavity. Although this structure is intrinsically transient and instabilities in the jet and disruption of the magnetic cavity ultimately lead to its break-up, a well collimated, “knotty” jet still emerges from the system; such clumpy morphology is reminiscent of that observed in many astrophysical jets. The possible introduction in the experiments of angular momentum and axial magnetic field will also be discussed. MHD plasmas (dpeaa)DE-He213 Accretion (dpeaa)DE-He213 Accretion discs (dpeaa)DE-He213 Laboratory astrophysics (dpeaa)DE-He213 Winds (dpeaa)DE-He213 Jets and outflows (dpeaa)DE-He213 Lebedev, S. V. verfasserin aut Frank, A. verfasserin aut Blackman, E. G. verfasserin aut Ampleford, D. J. verfasserin aut Jennings, C. A. verfasserin aut Chittenden, J. P. verfasserin aut Lery, T. verfasserin aut Bland, S. N. verfasserin aut Bott, S. C. verfasserin aut Hall, G. N. verfasserin aut Rapley, J. verfasserin aut Vidal, F. A. Suzuki verfasserin aut Marocchino, A. verfasserin aut Enthalten in Astrophysics and space science Dordrecht [u.a.] : Springer Science + Business Media B.V, 1968 307(2006), 1-3 vom: 15. Nov., Seite 17-22 (DE-627)268755868 (DE-600)1472548-4 1572-946X nnns volume:307 year:2006 number:1-3 day:15 month:11 pages:17-22 https://dx.doi.org/10.1007/s10509-006-9215-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE 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_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_206 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_2070 GBV_ILN_2086 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_2116 GBV_ILN_2118 GBV_ILN_2119 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_4012 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_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE 39.22 ASE AR 307 2006 1-3 15 11 17-22 |
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10.1007/s10509-006-9215-8 doi (DE-627)SPR010570969 (SPR)s10509-006-9215-8-e DE-627 ger DE-627 rakwb eng 520 530 620 ASE 39.00 bkl 39.22 bkl Ciardi, A. verfasserin aut 3D MHD Simulations of Laboratory Plasma Jets 2006 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Jets and outflows are thought to be an integral part of accretion phenomena and are associated with a large variety of objects. In these systems, the interaction of magnetic fields with an accretion disk and/or a magnetized central object is thought to be responsible for the acceleration and collimation of plasma into jets and wider angle flows. In this paper we present three-dimensional MHD simulations of magnetically driven, radiatively cooled laboratory jets that are produced on the MAGPIE experimental facility. The general outflow structure comprises an expanding magnetic cavity which is collimated by the pressure of an extended plasma background medium, and a magnetically confined jet which develops within the magnetic cavity. Although this structure is intrinsically transient and instabilities in the jet and disruption of the magnetic cavity ultimately lead to its break-up, a well collimated, “knotty” jet still emerges from the system; such clumpy morphology is reminiscent of that observed in many astrophysical jets. The possible introduction in the experiments of angular momentum and axial magnetic field will also be discussed. MHD plasmas (dpeaa)DE-He213 Accretion (dpeaa)DE-He213 Accretion discs (dpeaa)DE-He213 Laboratory astrophysics (dpeaa)DE-He213 Winds (dpeaa)DE-He213 Jets and outflows (dpeaa)DE-He213 Lebedev, S. V. verfasserin aut Frank, A. verfasserin aut Blackman, E. G. verfasserin aut Ampleford, D. J. verfasserin aut Jennings, C. A. verfasserin aut Chittenden, J. P. verfasserin aut Lery, T. verfasserin aut Bland, S. N. verfasserin aut Bott, S. C. verfasserin aut Hall, G. N. verfasserin aut Rapley, J. verfasserin aut Vidal, F. A. Suzuki verfasserin aut Marocchino, A. verfasserin aut Enthalten in Astrophysics and space science Dordrecht [u.a.] : Springer Science + Business Media B.V, 1968 307(2006), 1-3 vom: 15. Nov., Seite 17-22 (DE-627)268755868 (DE-600)1472548-4 1572-946X nnns volume:307 year:2006 number:1-3 day:15 month:11 pages:17-22 https://dx.doi.org/10.1007/s10509-006-9215-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE 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_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_206 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_2070 GBV_ILN_2086 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_2116 GBV_ILN_2118 GBV_ILN_2119 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_4012 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_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE 39.22 ASE AR 307 2006 1-3 15 11 17-22 |
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10.1007/s10509-006-9215-8 doi (DE-627)SPR010570969 (SPR)s10509-006-9215-8-e DE-627 ger DE-627 rakwb eng 520 530 620 ASE 39.00 bkl 39.22 bkl Ciardi, A. verfasserin aut 3D MHD Simulations of Laboratory Plasma Jets 2006 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Jets and outflows are thought to be an integral part of accretion phenomena and are associated with a large variety of objects. In these systems, the interaction of magnetic fields with an accretion disk and/or a magnetized central object is thought to be responsible for the acceleration and collimation of plasma into jets and wider angle flows. In this paper we present three-dimensional MHD simulations of magnetically driven, radiatively cooled laboratory jets that are produced on the MAGPIE experimental facility. The general outflow structure comprises an expanding magnetic cavity which is collimated by the pressure of an extended plasma background medium, and a magnetically confined jet which develops within the magnetic cavity. Although this structure is intrinsically transient and instabilities in the jet and disruption of the magnetic cavity ultimately lead to its break-up, a well collimated, “knotty” jet still emerges from the system; such clumpy morphology is reminiscent of that observed in many astrophysical jets. The possible introduction in the experiments of angular momentum and axial magnetic field will also be discussed. MHD plasmas (dpeaa)DE-He213 Accretion (dpeaa)DE-He213 Accretion discs (dpeaa)DE-He213 Laboratory astrophysics (dpeaa)DE-He213 Winds (dpeaa)DE-He213 Jets and outflows (dpeaa)DE-He213 Lebedev, S. V. verfasserin aut Frank, A. verfasserin aut Blackman, E. G. verfasserin aut Ampleford, D. J. verfasserin aut Jennings, C. A. verfasserin aut Chittenden, J. P. verfasserin aut Lery, T. verfasserin aut Bland, S. N. verfasserin aut Bott, S. C. verfasserin aut Hall, G. N. verfasserin aut Rapley, J. verfasserin aut Vidal, F. A. Suzuki verfasserin aut Marocchino, A. verfasserin aut Enthalten in Astrophysics and space science Dordrecht [u.a.] : Springer Science + Business Media B.V, 1968 307(2006), 1-3 vom: 15. Nov., Seite 17-22 (DE-627)268755868 (DE-600)1472548-4 1572-946X nnns volume:307 year:2006 number:1-3 day:15 month:11 pages:17-22 https://dx.doi.org/10.1007/s10509-006-9215-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE 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_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_206 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_2070 GBV_ILN_2086 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_2116 GBV_ILN_2118 GBV_ILN_2119 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_4012 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_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE 39.22 ASE AR 307 2006 1-3 15 11 17-22 |
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Enthalten in Astrophysics and space science 307(2006), 1-3 vom: 15. Nov., Seite 17-22 volume:307 year:2006 number:1-3 day:15 month:11 pages:17-22 |
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Enthalten in Astrophysics and space science 307(2006), 1-3 vom: 15. Nov., Seite 17-22 volume:307 year:2006 number:1-3 day:15 month:11 pages:17-22 |
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MHD plasmas Accretion Accretion discs Laboratory astrophysics Winds Jets and outflows |
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Ciardi, A. @@aut@@ Lebedev, S. V. @@aut@@ Frank, A. @@aut@@ Blackman, E. G. @@aut@@ Ampleford, D. J. @@aut@@ Jennings, C. A. @@aut@@ Chittenden, J. P. @@aut@@ Lery, T. @@aut@@ Bland, S. N. @@aut@@ Bott, S. C. @@aut@@ Hall, G. N. @@aut@@ Rapley, J. @@aut@@ Vidal, F. A. Suzuki @@aut@@ Marocchino, A. @@aut@@ |
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2006-11-15T00:00:00Z |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">SPR010570969</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20220110221325.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">201005s2006 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s10509-006-9215-8</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)SPR010570969</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(SPR)s10509-006-9215-8-e</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">520</subfield><subfield code="a">530</subfield><subfield code="a">620</subfield><subfield code="q">ASE</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">39.00</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">39.22</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Ciardi, A.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">3D MHD Simulations of Laboratory Plasma Jets</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2006</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Jets and outflows are thought to be an integral part of accretion phenomena and are associated with a large variety of objects. In these systems, the interaction of magnetic fields with an accretion disk and/or a magnetized central object is thought to be responsible for the acceleration and collimation of plasma into jets and wider angle flows. In this paper we present three-dimensional MHD simulations of magnetically driven, radiatively cooled laboratory jets that are produced on the MAGPIE experimental facility. The general outflow structure comprises an expanding magnetic cavity which is collimated by the pressure of an extended plasma background medium, and a magnetically confined jet which develops within the magnetic cavity. Although this structure is intrinsically transient and instabilities in the jet and disruption of the magnetic cavity ultimately lead to its break-up, a well collimated, “knotty” jet still emerges from the system; such clumpy morphology is reminiscent of that observed in many astrophysical jets. The possible introduction in the experiments of angular momentum and axial magnetic field will also be discussed.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">MHD plasmas</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Accretion</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Accretion discs</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Laboratory astrophysics</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Winds</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Jets and outflows</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Lebedev, S. V.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Frank, A.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Blackman, E. G.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ampleford, D. J.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Jennings, C. A.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Chittenden, J. 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|
| author |
Ciardi, A. |
| spellingShingle |
Ciardi, A. ddc 520 bkl 39.00 bkl 39.22 misc MHD plasmas misc Accretion misc Accretion discs misc Laboratory astrophysics misc Winds misc Jets and outflows 3D MHD Simulations of Laboratory Plasma Jets |
| authorStr |
Ciardi, A. |
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@@773@@(DE-627)268755868 |
| format |
electronic Article |
| dewey-ones |
520 - Astronomy & allied sciences 530 - Physics 620 - Engineering & allied operations |
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keep |
| author_role |
aut aut aut aut aut aut aut aut aut aut aut aut aut aut |
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springer |
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true |
| illustrated |
Not Illustrated |
| issn |
1572-946X |
| topic_title |
520 530 620 ASE 39.00 bkl 39.22 bkl 3D MHD Simulations of Laboratory Plasma Jets MHD plasmas (dpeaa)DE-He213 Accretion (dpeaa)DE-He213 Accretion discs (dpeaa)DE-He213 Laboratory astrophysics (dpeaa)DE-He213 Winds (dpeaa)DE-He213 Jets and outflows (dpeaa)DE-He213 |
| topic |
ddc 520 bkl 39.00 bkl 39.22 misc MHD plasmas misc Accretion misc Accretion discs misc Laboratory astrophysics misc Winds misc Jets and outflows |
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3D MHD Simulations of Laboratory Plasma Jets |
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3D MHD Simulations of Laboratory Plasma Jets |
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Ciardi, A. Lebedev, S. V. Frank, A. Blackman, E. G. Ampleford, D. J. Jennings, C. A. Chittenden, J. P. Lery, T. Bland, S. N. Bott, S. C. Hall, G. N. Rapley, J. Vidal, F. A. Suzuki Marocchino, A. |
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3d mhd simulations of laboratory plasma jets |
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3D MHD Simulations of Laboratory Plasma Jets |
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Abstract Jets and outflows are thought to be an integral part of accretion phenomena and are associated with a large variety of objects. In these systems, the interaction of magnetic fields with an accretion disk and/or a magnetized central object is thought to be responsible for the acceleration and collimation of plasma into jets and wider angle flows. In this paper we present three-dimensional MHD simulations of magnetically driven, radiatively cooled laboratory jets that are produced on the MAGPIE experimental facility. The general outflow structure comprises an expanding magnetic cavity which is collimated by the pressure of an extended plasma background medium, and a magnetically confined jet which develops within the magnetic cavity. Although this structure is intrinsically transient and instabilities in the jet and disruption of the magnetic cavity ultimately lead to its break-up, a well collimated, “knotty” jet still emerges from the system; such clumpy morphology is reminiscent of that observed in many astrophysical jets. The possible introduction in the experiments of angular momentum and axial magnetic field will also be discussed. |
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Abstract Jets and outflows are thought to be an integral part of accretion phenomena and are associated with a large variety of objects. In these systems, the interaction of magnetic fields with an accretion disk and/or a magnetized central object is thought to be responsible for the acceleration and collimation of plasma into jets and wider angle flows. In this paper we present three-dimensional MHD simulations of magnetically driven, radiatively cooled laboratory jets that are produced on the MAGPIE experimental facility. The general outflow structure comprises an expanding magnetic cavity which is collimated by the pressure of an extended plasma background medium, and a magnetically confined jet which develops within the magnetic cavity. Although this structure is intrinsically transient and instabilities in the jet and disruption of the magnetic cavity ultimately lead to its break-up, a well collimated, “knotty” jet still emerges from the system; such clumpy morphology is reminiscent of that observed in many astrophysical jets. The possible introduction in the experiments of angular momentum and axial magnetic field will also be discussed. |
| abstract_unstemmed |
Abstract Jets and outflows are thought to be an integral part of accretion phenomena and are associated with a large variety of objects. In these systems, the interaction of magnetic fields with an accretion disk and/or a magnetized central object is thought to be responsible for the acceleration and collimation of plasma into jets and wider angle flows. In this paper we present three-dimensional MHD simulations of magnetically driven, radiatively cooled laboratory jets that are produced on the MAGPIE experimental facility. The general outflow structure comprises an expanding magnetic cavity which is collimated by the pressure of an extended plasma background medium, and a magnetically confined jet which develops within the magnetic cavity. Although this structure is intrinsically transient and instabilities in the jet and disruption of the magnetic cavity ultimately lead to its break-up, a well collimated, “knotty” jet still emerges from the system; such clumpy morphology is reminiscent of that observed in many astrophysical jets. The possible introduction in the experiments of angular momentum and axial magnetic field will also be discussed. |
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| score |
7.4013014 |