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
Autor*in: |
Frank, A. [verfasserIn] |
---|
Format: |
Artikel |
---|---|
Sprache: |
Englisch |
Erschienen: |
2005 |
---|
Schlagwörter: |
---|
Anmerkung: |
© Springer Science + Business Media, Inc. 2005 |
---|
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: |
---|
DOI / URN: |
10.1007/s10509-005-3919-z |
---|
Katalog-ID: |
OLC2066245194 |
---|
LEADER | 01000caa a22002652 4500 | ||
---|---|---|---|
001 | OLC2066245194 | ||
003 | DE-627 | ||
005 | 20230502213430.0 | ||
007 | tu | ||
008 | 200820s2005 xx ||||| 00| ||eng c | ||
024 | 7 | |a 10.1007/s10509-005-3919-z |2 doi | |
035 | |a (DE-627)OLC2066245194 | ||
035 | |a (DE-He213)s10509-005-3919-z-p | ||
040 | |a DE-627 |b ger |c DE-627 |e rakwb | ||
041 | |a eng | ||
082 | 0 | 4 | |a 520 |a 530 |a 620 |q VZ |
084 | |a 16,12 |2 ssgn | ||
100 | 1 | |a Frank, A. |e verfasserin |4 aut | |
245 | 1 | 0 | |a A HED Laboratory Astrophysics Testbed Comes of Age: JET Deflection via Cross Winds |
264 | 1 | |c 2005 | |
336 | |a Text |b txt |2 rdacontent | ||
337 | |a ohne Hilfsmittel zu benutzen |b n |2 rdamedia | ||
338 | |a Band |b nc |2 rdacarrier | ||
500 | |a © Springer Science + Business Media, Inc. 2005 | ||
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. | ||
650 | 4 | |a hydrodynamics | |
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 | |
700 | 1 | |a Lebedev, S. V. |4 aut | |
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 | |
773 | 0 | 8 | |i Enthalten in |t Astrophysics and space science |d Kluwer Academic Publishers, 1968 |g 298(2005), 1-2 vom: Juli, Seite 107-114 |w (DE-627)129062723 |w (DE-600)629-4 |w (DE-576)014393522 |x 0004-640X |7 nnns |
773 | 1 | 8 | |g volume:298 |g year:2005 |g number:1-2 |g month:07 |g pages:107-114 |
856 | 4 | 1 | |u https://doi.org/10.1007/s10509-005-3919-z |z lizenzpflichtig |3 Volltext |
912 | |a GBV_USEFLAG_A | ||
912 | |a SYSFLAG_A | ||
912 | |a GBV_OLC | ||
912 | |a SSG-OLC-TEC | ||
912 | |a SSG-OLC-PHY | ||
912 | |a SSG-OLC-AST | ||
912 | |a SSG-OPC-AST | ||
912 | |a GBV_ILN_11 | ||
912 | |a GBV_ILN_40 | ||
912 | |a GBV_ILN_47 | ||
912 | |a GBV_ILN_70 | ||
912 | |a GBV_ILN_2279 | ||
912 | |a GBV_ILN_2286 | ||
912 | |a GBV_ILN_4012 | ||
951 | |a AR | ||
952 | |d 298 |j 2005 |e 1-2 |c 07 |h 107-114 |
author_variant |
a f af e g b eg egb a c ac s v l sv svl d a da a c ac s n b sn snb j p c jp jpc m g h mg mgh |
---|---|
matchkey_str |
article:0004640X:2005----::hdaoaoysrpyisetecmsfgjtel |
hierarchy_sort_str |
2005 |
publishDate |
2005 |
allfields |
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 |
spelling |
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 |
allfields_unstemmed |
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 |
allfieldsGer |
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 |
allfieldsSound |
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 |
language |
English |
source |
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 |
sourceStr |
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 |
format_phy_str_mv |
Article |
institution |
findex.gbv.de |
topic_facet |
hydrodynamics methods: laboratory ISM: Herbig–Haro objects stars: winds outflows |
dewey-raw |
520 |
isfreeaccess_bool |
false |
container_title |
Astrophysics and space science |
authorswithroles_txt_mv |
Frank, A. @@aut@@ 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@@ |
publishDateDaySort_date |
2005-07-01T00:00:00Z |
hierarchy_top_id |
129062723 |
dewey-sort |
3520 |
id |
OLC2066245194 |
language_de |
englisch |
fullrecord |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2066245194</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230502213430.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s2005 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s10509-005-3919-z</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2066245194</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s10509-005-3919-z-p</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">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">16,12</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Frank, A.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">A HED Laboratory Astrophysics Testbed Comes of Age: JET Deflection via Cross Winds</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2005</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">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Springer Science + Business Media, Inc. 2005</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="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.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">hydrodynamics</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">methods: laboratory</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">ISM: Herbig–Haro objects</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">stars: winds</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">outflows</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Blackman, E. G.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Cunningham, A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Lebedev, S. V.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ampleford, D.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ciardi, A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bland, S. N.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Chittenden, J. P.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Haines, M. G.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Astrophysics and space science</subfield><subfield code="d">Kluwer Academic Publishers, 1968</subfield><subfield code="g">298(2005), 1-2 vom: Juli, Seite 107-114</subfield><subfield code="w">(DE-627)129062723</subfield><subfield code="w">(DE-600)629-4</subfield><subfield code="w">(DE-576)014393522</subfield><subfield code="x">0004-640X</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:298</subfield><subfield code="g">year:2005</subfield><subfield code="g">number:1-2</subfield><subfield code="g">month:07</subfield><subfield code="g">pages:107-114</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/s10509-005-3919-z</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-TEC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_47</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2279</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2286</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4012</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">298</subfield><subfield code="j">2005</subfield><subfield code="e">1-2</subfield><subfield code="c">07</subfield><subfield code="h">107-114</subfield></datafield></record></collection>
|
author |
Frank, A. |
spellingShingle |
Frank, A. ddc 520 ssgn 16,12 misc hydrodynamics misc methods: laboratory misc ISM: Herbig–Haro objects misc stars: winds misc outflows A HED Laboratory Astrophysics Testbed Comes of Age: JET Deflection via Cross Winds |
authorStr |
Frank, A. |
ppnlink_with_tag_str_mv |
@@773@@(DE-627)129062723 |
format |
Article |
dewey-ones |
520 - Astronomy & allied sciences 530 - Physics 620 - Engineering & allied operations |
delete_txt_mv |
keep |
author_role |
aut aut aut aut aut aut aut aut aut |
collection |
OLC |
remote_str |
false |
illustrated |
Not Illustrated |
issn |
0004-640X |
topic_title |
520 530 620 VZ 16,12 ssgn A HED Laboratory Astrophysics Testbed Comes of Age: JET Deflection via Cross Winds hydrodynamics methods: laboratory ISM: Herbig–Haro objects stars: winds outflows |
topic |
ddc 520 ssgn 16,12 misc hydrodynamics misc methods: laboratory misc ISM: Herbig–Haro objects misc stars: winds misc outflows |
topic_unstemmed |
ddc 520 ssgn 16,12 misc hydrodynamics misc methods: laboratory misc ISM: Herbig–Haro objects misc stars: winds misc outflows |
topic_browse |
ddc 520 ssgn 16,12 misc hydrodynamics misc methods: laboratory misc ISM: Herbig–Haro objects misc stars: winds misc outflows |
format_facet |
Aufsätze Gedruckte Aufsätze |
format_main_str_mv |
Text Zeitschrift/Artikel |
carriertype_str_mv |
nc |
hierarchy_parent_title |
Astrophysics and space science |
hierarchy_parent_id |
129062723 |
dewey-tens |
520 - Astronomy 530 - Physics 620 - Engineering |
hierarchy_top_title |
Astrophysics and space science |
isfreeaccess_txt |
false |
familylinks_str_mv |
(DE-627)129062723 (DE-600)629-4 (DE-576)014393522 |
title |
A HED Laboratory Astrophysics Testbed Comes of Age: JET Deflection via Cross Winds |
ctrlnum |
(DE-627)OLC2066245194 (DE-He213)s10509-005-3919-z-p |
title_full |
A HED Laboratory Astrophysics Testbed Comes of Age: JET Deflection via Cross Winds |
author_sort |
Frank, A. |
journal |
Astrophysics and space science |
journalStr |
Astrophysics and space science |
lang_code |
eng |
isOA_bool |
false |
dewey-hundreds |
500 - Science 600 - Technology |
recordtype |
marc |
publishDateSort |
2005 |
contenttype_str_mv |
txt |
container_start_page |
107 |
author_browse |
Frank, A. Blackman, E. G. Cunningham, A. Lebedev, S. V. Ampleford, D. Ciardi, A. Bland, S. N. Chittenden, J. P. Haines, M. G. |
container_volume |
298 |
class |
520 530 620 VZ 16,12 ssgn |
format_se |
Aufsätze |
author-letter |
Frank, A. |
doi_str_mv |
10.1007/s10509-005-3919-z |
dewey-full |
520 530 620 |
title_sort |
a hed laboratory astrophysics testbed comes of age: jet deflection via cross winds |
title_auth |
A HED Laboratory Astrophysics Testbed Comes of Age: JET Deflection via Cross Winds |
abstract |
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 |
abstractGer |
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 |
abstract_unstemmed |
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 |
collection_details |
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 |
container_issue |
1-2 |
title_short |
A HED Laboratory Astrophysics Testbed Comes of Age: JET Deflection via Cross Winds |
url |
https://doi.org/10.1007/s10509-005-3919-z |
remote_bool |
false |
author2 |
Blackman, E. G. Cunningham, A. Lebedev, S. V. Ampleford, D. Ciardi, A. Bland, S. N. Chittenden, J. P. Haines, M. G. |
author2Str |
Blackman, E. G. Cunningham, A. Lebedev, S. V. Ampleford, D. Ciardi, A. Bland, S. N. Chittenden, J. P. Haines, M. G. |
ppnlink |
129062723 |
mediatype_str_mv |
n |
isOA_txt |
false |
hochschulschrift_bool |
false |
doi_str |
10.1007/s10509-005-3919-z |
up_date |
2024-07-04T04:03:42.776Z |
_version_ |
1803619740189458432 |
fullrecord_marcxml |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2066245194</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230502213430.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s2005 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s10509-005-3919-z</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2066245194</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s10509-005-3919-z-p</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">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">16,12</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Frank, A.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">A HED Laboratory Astrophysics Testbed Comes of Age: JET Deflection via Cross Winds</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2005</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">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Springer Science + Business Media, Inc. 2005</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="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.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">hydrodynamics</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">methods: laboratory</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">ISM: Herbig–Haro objects</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">stars: winds</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">outflows</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Blackman, E. G.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Cunningham, A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Lebedev, S. V.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ampleford, D.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ciardi, A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bland, S. N.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Chittenden, J. P.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Haines, M. G.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Astrophysics and space science</subfield><subfield code="d">Kluwer Academic Publishers, 1968</subfield><subfield code="g">298(2005), 1-2 vom: Juli, Seite 107-114</subfield><subfield code="w">(DE-627)129062723</subfield><subfield code="w">(DE-600)629-4</subfield><subfield code="w">(DE-576)014393522</subfield><subfield code="x">0004-640X</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:298</subfield><subfield code="g">year:2005</subfield><subfield code="g">number:1-2</subfield><subfield code="g">month:07</subfield><subfield code="g">pages:107-114</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/s10509-005-3919-z</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-TEC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_47</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2279</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2286</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4012</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">298</subfield><subfield code="j">2005</subfield><subfield code="e">1-2</subfield><subfield code="c">07</subfield><subfield code="h">107-114</subfield></datafield></record></collection>
|
score |
7.399809 |