Simulations of the supersonic radiative jet propagation in plasmas
Abstract Supersonic plasma jets are ubiquitous in astrophysics. Our study focus on the jets emanated from Herbig-Haro (HH) objects. They have velocities of a few hundred km/s and are extending over the distances more than a parsec. Interaction of the jets with surrounding matter produces two specifi...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Ribeyre, X. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2008 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science+Business Media B.V. 2008 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Springer Netherlands, 1968, 322(2008), 1-4 vom: 06. Nov., Seite 85-90 |
|---|---|
| Übergeordnetes Werk: |
volume:322 ; year:2008 ; number:1-4 ; day:06 ; month:11 ; pages:85-90 |
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| DOI / URN: |
10.1007/s10509-008-9936-y |
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OLC2066256412 |
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| 520 | |a Abstract Supersonic plasma jets are ubiquitous in astrophysics. Our study focus on the jets emanated from Herbig-Haro (HH) objects. They have velocities of a few hundred km/s and are extending over the distances more than a parsec. Interaction of the jets with surrounding matter produces two specific structures in the jet head: the bow shock and the Mach disk. The radiative cooling of these shocks affects strongly the jet dynamics. A tool to understand the physics of these jets is the laboratory experiment. A supersonic jet interaction with surrounding plasma was studied on the PALS laser facility. A collimated high-Z plasma jet with a velocity exceeding 400 km/s was generated and propagated over a few millimeters length. Here we report on study the effect of radiative cooling on the head jet structure with a 2D radiative hydrodynamic code. The simulation results demonstrated the scalability of the experimental observations to the HH jets. | ||
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10.1007/s10509-008-9936-y doi (DE-627)OLC2066256412 (DE-He213)s10509-008-9936-y-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Ribeyre, X. verfasserin aut Simulations of the supersonic radiative jet propagation in plasmas 2008 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2008 Abstract Supersonic plasma jets are ubiquitous in astrophysics. Our study focus on the jets emanated from Herbig-Haro (HH) objects. They have velocities of a few hundred km/s and are extending over the distances more than a parsec. Interaction of the jets with surrounding matter produces two specific structures in the jet head: the bow shock and the Mach disk. The radiative cooling of these shocks affects strongly the jet dynamics. A tool to understand the physics of these jets is the laboratory experiment. A supersonic jet interaction with surrounding plasma was studied on the PALS laser facility. A collimated high-Z plasma jet with a velocity exceeding 400 km/s was generated and propagated over a few millimeters length. Here we report on study the effect of radiative cooling on the head jet structure with a 2D radiative hydrodynamic code. The simulation results demonstrated the scalability of the experimental observations to the HH jets. Hydrodynamics Plasmas jets Herbig-Haro object Nicolaï, P. aut Galera, S. aut Tikhonchuk, V. T. aut Enthalten in Astrophysics and space science Springer Netherlands, 1968 322(2008), 1-4 vom: 06. Nov., Seite 85-90 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:322 year:2008 number:1-4 day:06 month:11 pages:85-90 https://doi.org/10.1007/s10509-008-9936-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 322 2008 1-4 06 11 85-90 |
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10.1007/s10509-008-9936-y doi (DE-627)OLC2066256412 (DE-He213)s10509-008-9936-y-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Ribeyre, X. verfasserin aut Simulations of the supersonic radiative jet propagation in plasmas 2008 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2008 Abstract Supersonic plasma jets are ubiquitous in astrophysics. Our study focus on the jets emanated from Herbig-Haro (HH) objects. They have velocities of a few hundred km/s and are extending over the distances more than a parsec. Interaction of the jets with surrounding matter produces two specific structures in the jet head: the bow shock and the Mach disk. The radiative cooling of these shocks affects strongly the jet dynamics. A tool to understand the physics of these jets is the laboratory experiment. A supersonic jet interaction with surrounding plasma was studied on the PALS laser facility. A collimated high-Z plasma jet with a velocity exceeding 400 km/s was generated and propagated over a few millimeters length. Here we report on study the effect of radiative cooling on the head jet structure with a 2D radiative hydrodynamic code. The simulation results demonstrated the scalability of the experimental observations to the HH jets. Hydrodynamics Plasmas jets Herbig-Haro object Nicolaï, P. aut Galera, S. aut Tikhonchuk, V. T. aut Enthalten in Astrophysics and space science Springer Netherlands, 1968 322(2008), 1-4 vom: 06. Nov., Seite 85-90 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:322 year:2008 number:1-4 day:06 month:11 pages:85-90 https://doi.org/10.1007/s10509-008-9936-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 322 2008 1-4 06 11 85-90 |
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10.1007/s10509-008-9936-y doi (DE-627)OLC2066256412 (DE-He213)s10509-008-9936-y-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Ribeyre, X. verfasserin aut Simulations of the supersonic radiative jet propagation in plasmas 2008 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2008 Abstract Supersonic plasma jets are ubiquitous in astrophysics. Our study focus on the jets emanated from Herbig-Haro (HH) objects. They have velocities of a few hundred km/s and are extending over the distances more than a parsec. Interaction of the jets with surrounding matter produces two specific structures in the jet head: the bow shock and the Mach disk. The radiative cooling of these shocks affects strongly the jet dynamics. A tool to understand the physics of these jets is the laboratory experiment. A supersonic jet interaction with surrounding plasma was studied on the PALS laser facility. A collimated high-Z plasma jet with a velocity exceeding 400 km/s was generated and propagated over a few millimeters length. Here we report on study the effect of radiative cooling on the head jet structure with a 2D radiative hydrodynamic code. The simulation results demonstrated the scalability of the experimental observations to the HH jets. Hydrodynamics Plasmas jets Herbig-Haro object Nicolaï, P. aut Galera, S. aut Tikhonchuk, V. T. aut Enthalten in Astrophysics and space science Springer Netherlands, 1968 322(2008), 1-4 vom: 06. Nov., Seite 85-90 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:322 year:2008 number:1-4 day:06 month:11 pages:85-90 https://doi.org/10.1007/s10509-008-9936-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 322 2008 1-4 06 11 85-90 |
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10.1007/s10509-008-9936-y doi (DE-627)OLC2066256412 (DE-He213)s10509-008-9936-y-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Ribeyre, X. verfasserin aut Simulations of the supersonic radiative jet propagation in plasmas 2008 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media B.V. 2008 Abstract Supersonic plasma jets are ubiquitous in astrophysics. Our study focus on the jets emanated from Herbig-Haro (HH) objects. They have velocities of a few hundred km/s and are extending over the distances more than a parsec. Interaction of the jets with surrounding matter produces two specific structures in the jet head: the bow shock and the Mach disk. The radiative cooling of these shocks affects strongly the jet dynamics. A tool to understand the physics of these jets is the laboratory experiment. A supersonic jet interaction with surrounding plasma was studied on the PALS laser facility. A collimated high-Z plasma jet with a velocity exceeding 400 km/s was generated and propagated over a few millimeters length. Here we report on study the effect of radiative cooling on the head jet structure with a 2D radiative hydrodynamic code. The simulation results demonstrated the scalability of the experimental observations to the HH jets. Hydrodynamics Plasmas jets Herbig-Haro object Nicolaï, P. aut Galera, S. aut Tikhonchuk, V. T. aut Enthalten in Astrophysics and space science Springer Netherlands, 1968 322(2008), 1-4 vom: 06. Nov., Seite 85-90 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:322 year:2008 number:1-4 day:06 month:11 pages:85-90 https://doi.org/10.1007/s10509-008-9936-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4012 AR 322 2008 1-4 06 11 85-90 |
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Abstract Supersonic plasma jets are ubiquitous in astrophysics. Our study focus on the jets emanated from Herbig-Haro (HH) objects. They have velocities of a few hundred km/s and are extending over the distances more than a parsec. Interaction of the jets with surrounding matter produces two specific structures in the jet head: the bow shock and the Mach disk. The radiative cooling of these shocks affects strongly the jet dynamics. A tool to understand the physics of these jets is the laboratory experiment. A supersonic jet interaction with surrounding plasma was studied on the PALS laser facility. A collimated high-Z plasma jet with a velocity exceeding 400 km/s was generated and propagated over a few millimeters length. Here we report on study the effect of radiative cooling on the head jet structure with a 2D radiative hydrodynamic code. The simulation results demonstrated the scalability of the experimental observations to the HH jets. © Springer Science+Business Media B.V. 2008 |
| abstractGer |
Abstract Supersonic plasma jets are ubiquitous in astrophysics. Our study focus on the jets emanated from Herbig-Haro (HH) objects. They have velocities of a few hundred km/s and are extending over the distances more than a parsec. Interaction of the jets with surrounding matter produces two specific structures in the jet head: the bow shock and the Mach disk. The radiative cooling of these shocks affects strongly the jet dynamics. A tool to understand the physics of these jets is the laboratory experiment. A supersonic jet interaction with surrounding plasma was studied on the PALS laser facility. A collimated high-Z plasma jet with a velocity exceeding 400 km/s was generated and propagated over a few millimeters length. Here we report on study the effect of radiative cooling on the head jet structure with a 2D radiative hydrodynamic code. The simulation results demonstrated the scalability of the experimental observations to the HH jets. © Springer Science+Business Media B.V. 2008 |
| abstract_unstemmed |
Abstract Supersonic plasma jets are ubiquitous in astrophysics. Our study focus on the jets emanated from Herbig-Haro (HH) objects. They have velocities of a few hundred km/s and are extending over the distances more than a parsec. Interaction of the jets with surrounding matter produces two specific structures in the jet head: the bow shock and the Mach disk. The radiative cooling of these shocks affects strongly the jet dynamics. A tool to understand the physics of these jets is the laboratory experiment. A supersonic jet interaction with surrounding plasma was studied on the PALS laser facility. A collimated high-Z plasma jet with a velocity exceeding 400 km/s was generated and propagated over a few millimeters length. Here we report on study the effect of radiative cooling on the head jet structure with a 2D radiative hydrodynamic code. The simulation results demonstrated the scalability of the experimental observations to the HH jets. © Springer Science+Business Media B.V. 2008 |
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| title_short |
Simulations of the supersonic radiative jet propagation in plasmas |
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https://doi.org/10.1007/s10509-008-9936-y |
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Nicolaï, P. Galera, S. Tikhonchuk, V. T. |
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