Observation of collapsing radiative shocks in laboratory experiments
This article reports the observation of the dense, collapsed layer produced by a radiative shock in a laboratory experiment. The experiment uses laser irradiation to accelerate a thin layer of solid-density material to above 100 km ∕ s , the first to probe such high velocities in a radiative shock....
Gespeichert in:
| Veröffentlicht in: | Physics of plasmas 2006-08, Vol.13 (8), p.082901-082901-5 |
|---|---|
| Hauptverfasser: | , , , , , , , , , , , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 082901-5 |
|---|---|
| container_issue | 8 |
| container_start_page | 082901 |
| container_title | Physics of plasmas |
| container_volume | 13 |
| creator | Reighard, A. B. Drake, R. P. Dannenberg, K. K. Kremer, D. J. Grosskopf, M. Harding, E. C. Leibrandt, D. R. Glendinning, S. G. Perry, T. S. Remington, B. A. Greenough, J. Knauer, J. Boehly, T. Bouquet, S. Boireau, L. Koenig, M. Vinci, T. |
| description | This article reports the observation of the dense, collapsed layer produced by a radiative shock in a laboratory experiment. The experiment uses laser irradiation to accelerate a thin layer of solid-density material to above
100
km
∕
s
, the first to probe such high velocities in a radiative shock. The layer in turn drives a shock wave through a cylindrical volume of Xe gas (at
∼
6
mg
∕
cm
3
). Radiation from the shocked Xe removes enough energy that the shocked layer increases in density and collapses spatially. This type of system is relevant to a number of astrophysical contexts, providing the potential to observe phenomena of interest to astrophysics and to test astrophysical computer codes. |
| doi_str_mv | 10.1063/1.2222294 |
| format | Article |
| fullrecord | <record><control><sourceid>hal_cross</sourceid><recordid>TN_cdi_crossref_primary_10_1063_1_2222294</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>oai_HAL_hal_03784918v1</sourcerecordid><originalsourceid>FETCH-LOGICAL-c517t-83b3a7756063aa4def328b7324842107084cbe390ad55c38e845b0e4eed307213</originalsourceid><addsrcrecordid>eNqNkE9LwzAYh4MoOKcHv0HBk0Jn0qRJehHG_DNhsIuCt5Cmb120NiUpxX172204L4q5JLw8-b0_HoTOCZ4QzOk1mSTDydgBGhEss1hwwQ6Ht8Ax5-zlGJ2E8IYxZjyVI3S7zAP4TrfW1ZErI-OqSjfB1q-R14Xt5x1EYeXMe4hsHVU6d163zq8j-GzA2w-o23CKjkpdBTjb3WP0fH_3NJvHi-XD42y6iE1KRBtLmlMtRMr7olqzAkqayFzQhEmWDAUlMznQDOsiTQ2VIFmaY2AABcUiIXSMLra5LrRWBWNbMCvj6hpMqxIsOSaZ7KnLLbXSlWr6itqvldNWzacLNcwwFZJlRHZkzxrvQvBQfn8gWA1CFVE7oT17s2WHxRthv8M_rCpXqo3VPuDq3wF_wZ3ze1A1RUm_AAoJmDE</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Observation of collapsing radiative shocks in laboratory experiments</title><source>AIP Journals Complete</source><source>AIP Digital Archive</source><creator>Reighard, A. B. ; Drake, R. P. ; Dannenberg, K. K. ; Kremer, D. J. ; Grosskopf, M. ; Harding, E. C. ; Leibrandt, D. R. ; Glendinning, S. G. ; Perry, T. S. ; Remington, B. A. ; Greenough, J. ; Knauer, J. ; Boehly, T. ; Bouquet, S. ; Boireau, L. ; Koenig, M. ; Vinci, T.</creator><creatorcontrib>Reighard, A. B. ; Drake, R. P. ; Dannenberg, K. K. ; Kremer, D. J. ; Grosskopf, M. ; Harding, E. C. ; Leibrandt, D. R. ; Glendinning, S. G. ; Perry, T. S. ; Remington, B. A. ; Greenough, J. ; Knauer, J. ; Boehly, T. ; Bouquet, S. ; Boireau, L. ; Koenig, M. ; Vinci, T.</creatorcontrib><description>This article reports the observation of the dense, collapsed layer produced by a radiative shock in a laboratory experiment. The experiment uses laser irradiation to accelerate a thin layer of solid-density material to above
100
km
∕
s
, the first to probe such high velocities in a radiative shock. The layer in turn drives a shock wave through a cylindrical volume of Xe gas (at
∼
6
mg
∕
cm
3
). Radiation from the shocked Xe removes enough energy that the shocked layer increases in density and collapses spatially. This type of system is relevant to a number of astrophysical contexts, providing the potential to observe phenomena of interest to astrophysics and to test astrophysical computer codes.</description><identifier>ISSN: 1070-664X</identifier><identifier>EISSN: 1089-7674</identifier><identifier>DOI: 10.1063/1.2222294</identifier><identifier>CODEN: PHPAEN</identifier><language>eng</language><publisher>United States: American Institute of Physics</publisher><subject>70 PLASMA PHYSICS AND FUSION TECHNOLOGY ; ASTROPHYSICS ; COMPUTER CODES ; CYLINDRICAL CONFIGURATION ; LASER RADIATION ; LAYERS ; LIGHT TRANSMISSION ; Physics ; PLASMA ; PLASMA DENSITY ; SHOCK WAVES ; THIN FILMS ; XENON</subject><ispartof>Physics of plasmas, 2006-08, Vol.13 (8), p.082901-082901-5</ispartof><rights>American Institute of Physics</rights><rights>2006 American Institute of Physics</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c517t-83b3a7756063aa4def328b7324842107084cbe390ad55c38e845b0e4eed307213</citedby><cites>FETCH-LOGICAL-c517t-83b3a7756063aa4def328b7324842107084cbe390ad55c38e845b0e4eed307213</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://pubs.aip.org/pop/article-lookup/doi/10.1063/1.2222294$$EHTML$$P50$$Gscitation$$H</linktohtml><link.rule.ids>230,314,776,780,790,881,1553,4497,27903,27904,76130,76136</link.rule.ids><backlink>$$Uhttps://hal.science/hal-03784918$$DView record in HAL$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/20860198$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Reighard, A. B.</creatorcontrib><creatorcontrib>Drake, R. P.</creatorcontrib><creatorcontrib>Dannenberg, K. K.</creatorcontrib><creatorcontrib>Kremer, D. J.</creatorcontrib><creatorcontrib>Grosskopf, M.</creatorcontrib><creatorcontrib>Harding, E. C.</creatorcontrib><creatorcontrib>Leibrandt, D. R.</creatorcontrib><creatorcontrib>Glendinning, S. G.</creatorcontrib><creatorcontrib>Perry, T. S.</creatorcontrib><creatorcontrib>Remington, B. A.</creatorcontrib><creatorcontrib>Greenough, J.</creatorcontrib><creatorcontrib>Knauer, J.</creatorcontrib><creatorcontrib>Boehly, T.</creatorcontrib><creatorcontrib>Bouquet, S.</creatorcontrib><creatorcontrib>Boireau, L.</creatorcontrib><creatorcontrib>Koenig, M.</creatorcontrib><creatorcontrib>Vinci, T.</creatorcontrib><title>Observation of collapsing radiative shocks in laboratory experiments</title><title>Physics of plasmas</title><description>This article reports the observation of the dense, collapsed layer produced by a radiative shock in a laboratory experiment. The experiment uses laser irradiation to accelerate a thin layer of solid-density material to above
100
km
∕
s
, the first to probe such high velocities in a radiative shock. The layer in turn drives a shock wave through a cylindrical volume of Xe gas (at
∼
6
mg
∕
cm
3
). Radiation from the shocked Xe removes enough energy that the shocked layer increases in density and collapses spatially. This type of system is relevant to a number of astrophysical contexts, providing the potential to observe phenomena of interest to astrophysics and to test astrophysical computer codes.</description><subject>70 PLASMA PHYSICS AND FUSION TECHNOLOGY</subject><subject>ASTROPHYSICS</subject><subject>COMPUTER CODES</subject><subject>CYLINDRICAL CONFIGURATION</subject><subject>LASER RADIATION</subject><subject>LAYERS</subject><subject>LIGHT TRANSMISSION</subject><subject>Physics</subject><subject>PLASMA</subject><subject>PLASMA DENSITY</subject><subject>SHOCK WAVES</subject><subject>THIN FILMS</subject><subject>XENON</subject><issn>1070-664X</issn><issn>1089-7674</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2006</creationdate><recordtype>article</recordtype><recordid>eNqNkE9LwzAYh4MoOKcHv0HBk0Jn0qRJehHG_DNhsIuCt5Cmb120NiUpxX172204L4q5JLw8-b0_HoTOCZ4QzOk1mSTDydgBGhEss1hwwQ6Ht8Ax5-zlGJ2E8IYxZjyVI3S7zAP4TrfW1ZErI-OqSjfB1q-R14Xt5x1EYeXMe4hsHVU6d163zq8j-GzA2w-o23CKjkpdBTjb3WP0fH_3NJvHi-XD42y6iE1KRBtLmlMtRMr7olqzAkqayFzQhEmWDAUlMznQDOsiTQ2VIFmaY2AABcUiIXSMLra5LrRWBWNbMCvj6hpMqxIsOSaZ7KnLLbXSlWr6itqvldNWzacLNcwwFZJlRHZkzxrvQvBQfn8gWA1CFVE7oT17s2WHxRthv8M_rCpXqo3VPuDq3wF_wZ3ze1A1RUm_AAoJmDE</recordid><startdate>20060801</startdate><enddate>20060801</enddate><creator>Reighard, A. B.</creator><creator>Drake, R. P.</creator><creator>Dannenberg, K. K.</creator><creator>Kremer, D. J.</creator><creator>Grosskopf, M.</creator><creator>Harding, E. C.</creator><creator>Leibrandt, D. R.</creator><creator>Glendinning, S. G.</creator><creator>Perry, T. S.</creator><creator>Remington, B. A.</creator><creator>Greenough, J.</creator><creator>Knauer, J.</creator><creator>Boehly, T.</creator><creator>Bouquet, S.</creator><creator>Boireau, L.</creator><creator>Koenig, M.</creator><creator>Vinci, T.</creator><general>American Institute of Physics</general><scope>AAYXX</scope><scope>CITATION</scope><scope>1XC</scope><scope>OTOTI</scope></search><sort><creationdate>20060801</creationdate><title>Observation of collapsing radiative shocks in laboratory experiments</title><author>Reighard, A. B. ; Drake, R. P. ; Dannenberg, K. K. ; Kremer, D. J. ; Grosskopf, M. ; Harding, E. C. ; Leibrandt, D. R. ; Glendinning, S. G. ; Perry, T. S. ; Remington, B. A. ; Greenough, J. ; Knauer, J. ; Boehly, T. ; Bouquet, S. ; Boireau, L. ; Koenig, M. ; Vinci, T.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c517t-83b3a7756063aa4def328b7324842107084cbe390ad55c38e845b0e4eed307213</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2006</creationdate><topic>70 PLASMA PHYSICS AND FUSION TECHNOLOGY</topic><topic>ASTROPHYSICS</topic><topic>COMPUTER CODES</topic><topic>CYLINDRICAL CONFIGURATION</topic><topic>LASER RADIATION</topic><topic>LAYERS</topic><topic>LIGHT TRANSMISSION</topic><topic>Physics</topic><topic>PLASMA</topic><topic>PLASMA DENSITY</topic><topic>SHOCK WAVES</topic><topic>THIN FILMS</topic><topic>XENON</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Reighard, A. B.</creatorcontrib><creatorcontrib>Drake, R. P.</creatorcontrib><creatorcontrib>Dannenberg, K. K.</creatorcontrib><creatorcontrib>Kremer, D. J.</creatorcontrib><creatorcontrib>Grosskopf, M.</creatorcontrib><creatorcontrib>Harding, E. C.</creatorcontrib><creatorcontrib>Leibrandt, D. R.</creatorcontrib><creatorcontrib>Glendinning, S. G.</creatorcontrib><creatorcontrib>Perry, T. S.</creatorcontrib><creatorcontrib>Remington, B. A.</creatorcontrib><creatorcontrib>Greenough, J.</creatorcontrib><creatorcontrib>Knauer, J.</creatorcontrib><creatorcontrib>Boehly, T.</creatorcontrib><creatorcontrib>Bouquet, S.</creatorcontrib><creatorcontrib>Boireau, L.</creatorcontrib><creatorcontrib>Koenig, M.</creatorcontrib><creatorcontrib>Vinci, T.</creatorcontrib><collection>CrossRef</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>OSTI.GOV</collection><jtitle>Physics of plasmas</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Reighard, A. B.</au><au>Drake, R. P.</au><au>Dannenberg, K. K.</au><au>Kremer, D. J.</au><au>Grosskopf, M.</au><au>Harding, E. C.</au><au>Leibrandt, D. R.</au><au>Glendinning, S. G.</au><au>Perry, T. S.</au><au>Remington, B. A.</au><au>Greenough, J.</au><au>Knauer, J.</au><au>Boehly, T.</au><au>Bouquet, S.</au><au>Boireau, L.</au><au>Koenig, M.</au><au>Vinci, T.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Observation of collapsing radiative shocks in laboratory experiments</atitle><jtitle>Physics of plasmas</jtitle><date>2006-08-01</date><risdate>2006</risdate><volume>13</volume><issue>8</issue><spage>082901</spage><epage>082901-5</epage><pages>082901-082901-5</pages><issn>1070-664X</issn><eissn>1089-7674</eissn><coden>PHPAEN</coden><abstract>This article reports the observation of the dense, collapsed layer produced by a radiative shock in a laboratory experiment. The experiment uses laser irradiation to accelerate a thin layer of solid-density material to above
100
km
∕
s
, the first to probe such high velocities in a radiative shock. The layer in turn drives a shock wave through a cylindrical volume of Xe gas (at
∼
6
mg
∕
cm
3
). Radiation from the shocked Xe removes enough energy that the shocked layer increases in density and collapses spatially. This type of system is relevant to a number of astrophysical contexts, providing the potential to observe phenomena of interest to astrophysics and to test astrophysical computer codes.</abstract><cop>United States</cop><pub>American Institute of Physics</pub><doi>10.1063/1.2222294</doi><tpages>5</tpages><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 1070-664X |
| ispartof | Physics of plasmas, 2006-08, Vol.13 (8), p.082901-082901-5 |
| issn | 1070-664X 1089-7674 |
| language | eng |
| recordid | cdi_crossref_primary_10_1063_1_2222294 |
| source | AIP Journals Complete; AIP Digital Archive |
| subjects | 70 PLASMA PHYSICS AND FUSION TECHNOLOGY ASTROPHYSICS COMPUTER CODES CYLINDRICAL CONFIGURATION LASER RADIATION LAYERS LIGHT TRANSMISSION Physics PLASMA PLASMA DENSITY SHOCK WAVES THIN FILMS XENON |
| title | Observation of collapsing radiative shocks in laboratory experiments |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-24T00%3A25%3A15IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-hal_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Observation%20of%20collapsing%20radiative%20shocks%20in%20laboratory%20experiments&rft.jtitle=Physics%20of%20plasmas&rft.au=Reighard,%20A.%20B.&rft.date=2006-08-01&rft.volume=13&rft.issue=8&rft.spage=082901&rft.epage=082901-5&rft.pages=082901-082901-5&rft.issn=1070-664X&rft.eissn=1089-7674&rft.coden=PHPAEN&rft_id=info:doi/10.1063/1.2222294&rft_dat=%3Chal_cross%3Eoai_HAL_hal_03784918v1%3C/hal_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |