Infrared emissivity of tin upon release of a 25 GPa shock into a lithium fluoride window
We measured the emissivity of a tin sample at its interface with a lithium-fluoride window upon release of a 25 GPa shock wave from the tin into the window. Measurements were made over four wavelength bands between 1.2 and 5.4 μm. Thermal emission backgrounds from the tin, glue, and lithium fluoride...
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Veröffentlicht in: | Journal of applied physics 2011-11, Vol.110 (10), p.103510-103510-8 |
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container_title | Journal of applied physics |
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creator | Turley, W. D. Holtkamp, D. B. Veeser, L. R. Stevens, G. D. Marshall, B. R. Seifter, A. Corrow, R. B. Stone, J. B. Young, J. A. Grover, M. |
description | We measured the emissivity of a tin sample at its interface with a lithium-fluoride window upon release of a 25 GPa shock wave from the tin into the window. Measurements were made over four wavelength bands between 1.2 and 5.4 μm. Thermal emission backgrounds from the tin, glue, and lithium fluoride were successfully removed from the reflectance signals. Emissivity changes for the sample, which was initially nearly specular, were small except for the longest wavelength band, where uncertainties were high because of poor signal-to-noise ratio at that wavelength. A thin glue layer, which bonds the sample to the window, was found to heat from reverberations of the shock wave between the tin and the lithium fluoride. At approximately 3.4 μm, the thermal emission from the glue was large compared to the tin, allowing a good estimate of the glue temperature from the thermal radiance. The glue appears to remain slightly colder than the tin, thereby minimizing heat conduction into or out of the tin immediately after the shock passage. |
doi_str_mv | 10.1063/1.3657465 |
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D. ; Holtkamp, D. B. ; Veeser, L. R. ; Stevens, G. D. ; Marshall, B. R. ; Seifter, A. ; Corrow, R. B. ; Stone, J. B. ; Young, J. A. ; Grover, M.</creator><creatorcontrib>Turley, W. D. ; Holtkamp, D. B. ; Veeser, L. R. ; Stevens, G. D. ; Marshall, B. R. ; Seifter, A. ; Corrow, R. B. ; Stone, J. B. ; Young, J. A. ; Grover, M.</creatorcontrib><description>We measured the emissivity of a tin sample at its interface with a lithium-fluoride window upon release of a 25 GPa shock wave from the tin into the window. Measurements were made over four wavelength bands between 1.2 and 5.4 μm. Thermal emission backgrounds from the tin, glue, and lithium fluoride were successfully removed from the reflectance signals. Emissivity changes for the sample, which was initially nearly specular, were small except for the longest wavelength band, where uncertainties were high because of poor signal-to-noise ratio at that wavelength. A thin glue layer, which bonds the sample to the window, was found to heat from reverberations of the shock wave between the tin and the lithium fluoride. At approximately 3.4 μm, the thermal emission from the glue was large compared to the tin, allowing a good estimate of the glue temperature from the thermal radiance. The glue appears to remain slightly colder than the tin, thereby minimizing heat conduction into or out of the tin immediately after the shock passage.</description><identifier>ISSN: 0021-8979</identifier><identifier>EISSN: 1089-7550</identifier><identifier>DOI: 10.1063/1.3657465</identifier><identifier>CODEN: JAPIAU</identifier><language>eng</language><publisher>American Institute of Physics</publisher><ispartof>Journal of applied physics, 2011-11, Vol.110 (10), p.103510-103510-8</ispartof><rights>2011 American Institute of Physics</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c283t-9a9b955387ecc2434640231c4c990e709b3e9265a2e689376953a40dcf8cb2d23</citedby><cites>FETCH-LOGICAL-c283t-9a9b955387ecc2434640231c4c990e709b3e9265a2e689376953a40dcf8cb2d23</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://pubs.aip.org/jap/article-lookup/doi/10.1063/1.3657465$$EHTML$$P50$$Gscitation$$H</linktohtml><link.rule.ids>314,776,780,790,1553,4498,27901,27902,76126,76132</link.rule.ids></links><search><creatorcontrib>Turley, W. D.</creatorcontrib><creatorcontrib>Holtkamp, D. B.</creatorcontrib><creatorcontrib>Veeser, L. R.</creatorcontrib><creatorcontrib>Stevens, G. D.</creatorcontrib><creatorcontrib>Marshall, B. R.</creatorcontrib><creatorcontrib>Seifter, A.</creatorcontrib><creatorcontrib>Corrow, R. B.</creatorcontrib><creatorcontrib>Stone, J. B.</creatorcontrib><creatorcontrib>Young, J. A.</creatorcontrib><creatorcontrib>Grover, M.</creatorcontrib><title>Infrared emissivity of tin upon release of a 25 GPa shock into a lithium fluoride window</title><title>Journal of applied physics</title><description>We measured the emissivity of a tin sample at its interface with a lithium-fluoride window upon release of a 25 GPa shock wave from the tin into the window. Measurements were made over four wavelength bands between 1.2 and 5.4 μm. Thermal emission backgrounds from the tin, glue, and lithium fluoride were successfully removed from the reflectance signals. Emissivity changes for the sample, which was initially nearly specular, were small except for the longest wavelength band, where uncertainties were high because of poor signal-to-noise ratio at that wavelength. A thin glue layer, which bonds the sample to the window, was found to heat from reverberations of the shock wave between the tin and the lithium fluoride. At approximately 3.4 μm, the thermal emission from the glue was large compared to the tin, allowing a good estimate of the glue temperature from the thermal radiance. The glue appears to remain slightly colder than the tin, thereby minimizing heat conduction into or out of the tin immediately after the shock passage.</description><issn>0021-8979</issn><issn>1089-7550</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2011</creationdate><recordtype>article</recordtype><recordid>eNp1kDFLAzEYhoMoWKuD_yCrw9UvySWXb3CQorVQ0EHB7UhzORq9XkqSWvrv29KKk9MLDw_v8BByy2DEQIl7NhJKVqWSZ2TAQGNRSQnnZADAWaGxwktyldIXAGNa4IB8Tvs2muga6pY-Jf_j85aGlmbf0_Uq9DS6zpnkDsxQLunkzdC0CPab-j6HPet8Xvj1krbdOkTfOLrxfRM21-SiNV1yN6cdko_np_fxSzF7nUzHj7PCci1ygQbnKKXQlbOWl6JUJXDBbGkRwVWAc-GQK2m4UxpFpVAKU0JjW23nvOFiSO6OvzaGlKJr61X0SxO3NYP6kKRm9SnJ3n04usn6bLIP_f_yb5f6r4vYAfD1Z4I</recordid><startdate>20111115</startdate><enddate>20111115</enddate><creator>Turley, W. D.</creator><creator>Holtkamp, D. B.</creator><creator>Veeser, L. R.</creator><creator>Stevens, G. D.</creator><creator>Marshall, B. R.</creator><creator>Seifter, A.</creator><creator>Corrow, R. B.</creator><creator>Stone, J. B.</creator><creator>Young, J. A.</creator><creator>Grover, M.</creator><general>American Institute of Physics</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>20111115</creationdate><title>Infrared emissivity of tin upon release of a 25 GPa shock into a lithium fluoride window</title><author>Turley, W. D. ; Holtkamp, D. B. ; Veeser, L. R. ; Stevens, G. D. ; Marshall, B. R. ; Seifter, A. ; Corrow, R. B. ; Stone, J. B. ; Young, J. A. ; Grover, M.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c283t-9a9b955387ecc2434640231c4c990e709b3e9265a2e689376953a40dcf8cb2d23</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2011</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Turley, W. D.</creatorcontrib><creatorcontrib>Holtkamp, D. B.</creatorcontrib><creatorcontrib>Veeser, L. R.</creatorcontrib><creatorcontrib>Stevens, G. D.</creatorcontrib><creatorcontrib>Marshall, B. R.</creatorcontrib><creatorcontrib>Seifter, A.</creatorcontrib><creatorcontrib>Corrow, R. B.</creatorcontrib><creatorcontrib>Stone, J. B.</creatorcontrib><creatorcontrib>Young, J. A.</creatorcontrib><creatorcontrib>Grover, M.</creatorcontrib><collection>CrossRef</collection><jtitle>Journal of applied physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Turley, W. D.</au><au>Holtkamp, D. B.</au><au>Veeser, L. R.</au><au>Stevens, G. D.</au><au>Marshall, B. R.</au><au>Seifter, A.</au><au>Corrow, R. B.</au><au>Stone, J. B.</au><au>Young, J. A.</au><au>Grover, M.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Infrared emissivity of tin upon release of a 25 GPa shock into a lithium fluoride window</atitle><jtitle>Journal of applied physics</jtitle><date>2011-11-15</date><risdate>2011</risdate><volume>110</volume><issue>10</issue><spage>103510</spage><epage>103510-8</epage><pages>103510-103510-8</pages><issn>0021-8979</issn><eissn>1089-7550</eissn><coden>JAPIAU</coden><abstract>We measured the emissivity of a tin sample at its interface with a lithium-fluoride window upon release of a 25 GPa shock wave from the tin into the window. Measurements were made over four wavelength bands between 1.2 and 5.4 μm. Thermal emission backgrounds from the tin, glue, and lithium fluoride were successfully removed from the reflectance signals. Emissivity changes for the sample, which was initially nearly specular, were small except for the longest wavelength band, where uncertainties were high because of poor signal-to-noise ratio at that wavelength. A thin glue layer, which bonds the sample to the window, was found to heat from reverberations of the shock wave between the tin and the lithium fluoride. At approximately 3.4 μm, the thermal emission from the glue was large compared to the tin, allowing a good estimate of the glue temperature from the thermal radiance. The glue appears to remain slightly colder than the tin, thereby minimizing heat conduction into or out of the tin immediately after the shock passage.</abstract><pub>American Institute of Physics</pub><doi>10.1063/1.3657465</doi></addata></record> |
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title | Infrared emissivity of tin upon release of a 25 GPa shock into a lithium fluoride window |
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