Uniform fill improves K-shell power relative to annular fill for argon gas puffs on Saturn
Summary form only given. The radiation from uniform-fill argon gas puffs on the Saturn accelerator with a 4.5-cm diameter nozzle are compared with that generated from a previously optimized 2.5-cm diameter annular nozzle. The pressure range of the uniform fill spanned 1300 to 2900 Torr and that of t...
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| creator | Sanford, T.W.L. Marder, B.M. Spielman, R.B. Nash, T.J. Douglas, M. Deeney, C. Struve, K. Mock, R.C. Seamen, J.F. McGurn, J.S. Jobe, D. Gilliland, T.L. Vargas, M. Apruzese, J.P. Thornhill, J.W. Pulsifer, P.E. Whitney, K.G. Davis, J. Cochran, S.L. Velikovich, K.G. Weber, B.V. Peterson, G. Mosher, D. De Groot, J.S. Hammer, J.H. |
| description | Summary form only given. The radiation from uniform-fill argon gas puffs on the Saturn accelerator with a 4.5-cm diameter nozzle are compared with that generated from a previously optimized 2.5-cm diameter annular nozzle. The pressure range of the uniform fill spanned 1300 to 2900 Torr and that of the annular nozzle was set to 1650 Torr-the pressure that previously maximized the K-shell radiation yield. B-dot monitors measured current in the MITLs and 4.5 cm upstream of the load. A bolometer and duplicate sets of filtered XRDs and PCDs, spanning the energy range of 200 eV to 6 keV, monitored the temporal characteristics of the radiation. A suite of time-integrated and time-resolved, filtered, fast-framing, X-ray pinhole cameras, and crystal spectrometers monitored the spatial and spectral structure of the radiation. The radial density profile of the initial gas profile was measured on a test stand at NRL using a two-color interferometer. |
| doi_str_mv | 10.1109/PLASMA.1996.551486 |
| format | Conference Proceeding |
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The radiation from uniform-fill argon gas puffs on the Saturn accelerator with a 4.5-cm diameter nozzle are compared with that generated from a previously optimized 2.5-cm diameter annular nozzle. The pressure range of the uniform fill spanned 1300 to 2900 Torr and that of the annular nozzle was set to 1650 Torr-the pressure that previously maximized the K-shell radiation yield. B-dot monitors measured current in the MITLs and 4.5 cm upstream of the load. A bolometer and duplicate sets of filtered XRDs and PCDs, spanning the energy range of 200 eV to 6 keV, monitored the temporal characteristics of the radiation. A suite of time-integrated and time-resolved, filtered, fast-framing, X-ray pinhole cameras, and crystal spectrometers monitored the spatial and spectral structure of the radiation. 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The radiation from uniform-fill argon gas puffs on the Saturn accelerator with a 4.5-cm diameter nozzle are compared with that generated from a previously optimized 2.5-cm diameter annular nozzle. The pressure range of the uniform fill spanned 1300 to 2900 Torr and that of the annular nozzle was set to 1650 Torr-the pressure that previously maximized the K-shell radiation yield. B-dot monitors measured current in the MITLs and 4.5 cm upstream of the load. A bolometer and duplicate sets of filtered XRDs and PCDs, spanning the energy range of 200 eV to 6 keV, monitored the temporal characteristics of the radiation. A suite of time-integrated and time-resolved, filtered, fast-framing, X-ray pinhole cameras, and crystal spectrometers monitored the spatial and spectral structure of the radiation. The radial density profile of the initial gas profile was measured on a test stand at NRL using a two-color interferometer.</description><subject>07 ISOTOPE AND RADIATION SOURCE TECHNOLOGY</subject><subject>ACCELERATORS</subject><subject>Argon</subject><subject>Cameras</subject><subject>COMPARATIVE EVALUATIONS</subject><subject>Current measurement</subject><subject>Energy measurement</subject><subject>Geometry</subject><subject>Hydrodynamics</subject><subject>IMPLOSIONS</subject><subject>Laboratories</subject><subject>LONGITUDINAL PINCH</subject><subject>Physics</subject><subject>PRESSURE DEPENDENCE</subject><subject>Radiation monitoring</subject><subject>Saturn</subject><subject>X RADIATION</subject><subject>X-RAY SOURCES</subject><issn>0730-9244</issn><issn>2576-7208</issn><isbn>9780780333222</isbn><isbn>0780333225</isbn><fulltext>true</fulltext><rsrctype>conference_proceeding</rsrctype><creationdate>1996</creationdate><recordtype>conference_proceeding</recordtype><sourceid>6IE</sourceid><sourceid>RIE</sourceid><recordid>eNotUMtqwzAQFH1Ag5sfyEn9AKd6yzqG0BdNaSHNpRejOOtExbGMpKT07ytwl4VlhpllGIRmlMwpJeb-Y7VYvy3m1Bg1l5KKSl2gCZNalZqR6hJNja5IXs45Y-wKTYjmpDRMiBs0jfGb5BGSck4m6GvTu9aHI25d12F3HII_Q8SvZTxAJgb_AwEH6GxyZ8DJY9v3p86GUZ-d2Ia97_HeRjyc2jbiDNY2nUJ_i65b20WY_t8CbR4fPpfP5er96WW5WJWOUp5K2SjNLZHKcgWCEbaFHaMsZxbVTkhBoeGGMEsoA8alkXRrASpFKt2CloYX6G7862NydWxcgubQ-L6HJtVCGJGbKNBs1DgAqIfgjjb81mN5_A-nBV_f</recordid><startdate>1996</startdate><enddate>1996</enddate><creator>Sanford, T.W.L.</creator><creator>Marder, B.M.</creator><creator>Spielman, R.B.</creator><creator>Nash, T.J.</creator><creator>Douglas, M.</creator><creator>Deeney, C.</creator><creator>Struve, K.</creator><creator>Mock, R.C.</creator><creator>Seamen, J.F.</creator><creator>McGurn, J.S.</creator><creator>Jobe, D.</creator><creator>Gilliland, T.L.</creator><creator>Vargas, M.</creator><creator>Apruzese, J.P.</creator><creator>Thornhill, J.W.</creator><creator>Pulsifer, P.E.</creator><creator>Whitney, K.G.</creator><creator>Davis, J.</creator><creator>Cochran, S.L.</creator><creator>Velikovich, K.G.</creator><creator>Weber, B.V.</creator><creator>Peterson, G.</creator><creator>Mosher, D.</creator><creator>De Groot, J.S.</creator><creator>Hammer, J.H.</creator><general>IEEE</general><general>Institute of Electrical and Electronics Engineers, Inc., Piscataway, NJ (United States)</general><scope>6IE</scope><scope>6IL</scope><scope>CBEJK</scope><scope>RIE</scope><scope>RIL</scope><scope>OTOTI</scope></search><sort><creationdate>1996</creationdate><title>Uniform fill improves K-shell power relative to annular fill for argon gas puffs on Saturn</title><author>Sanford, T.W.L. ; Marder, B.M. ; Spielman, R.B. ; Nash, T.J. ; Douglas, M. ; Deeney, C. ; Struve, K. ; Mock, R.C. ; Seamen, J.F. ; McGurn, J.S. ; Jobe, D. ; Gilliland, T.L. ; Vargas, M. ; Apruzese, J.P. ; Thornhill, J.W. ; Pulsifer, P.E. ; Whitney, K.G. ; Davis, J. ; Cochran, S.L. ; Velikovich, K.G. ; Weber, B.V. ; Peterson, G. ; Mosher, D. ; De Groot, J.S. ; Hammer, J.H.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-i113t-5c673a056a36e4202bed21207348d4541ec3902a012e235951baee86087fe7593</frbrgroupid><rsrctype>conference_proceedings</rsrctype><prefilter>conference_proceedings</prefilter><language>eng</language><creationdate>1996</creationdate><topic>07 ISOTOPE AND RADIATION SOURCE TECHNOLOGY</topic><topic>ACCELERATORS</topic><topic>Argon</topic><topic>Cameras</topic><topic>COMPARATIVE EVALUATIONS</topic><topic>Current measurement</topic><topic>Energy measurement</topic><topic>Geometry</topic><topic>Hydrodynamics</topic><topic>IMPLOSIONS</topic><topic>Laboratories</topic><topic>LONGITUDINAL PINCH</topic><topic>Physics</topic><topic>PRESSURE DEPENDENCE</topic><topic>Radiation monitoring</topic><topic>Saturn</topic><topic>X RADIATION</topic><topic>X-RAY SOURCES</topic><toplevel>online_resources</toplevel><creatorcontrib>Sanford, T.W.L.</creatorcontrib><creatorcontrib>Marder, B.M.</creatorcontrib><creatorcontrib>Spielman, R.B.</creatorcontrib><creatorcontrib>Nash, T.J.</creatorcontrib><creatorcontrib>Douglas, M.</creatorcontrib><creatorcontrib>Deeney, C.</creatorcontrib><creatorcontrib>Struve, K.</creatorcontrib><creatorcontrib>Mock, R.C.</creatorcontrib><creatorcontrib>Seamen, J.F.</creatorcontrib><creatorcontrib>McGurn, J.S.</creatorcontrib><creatorcontrib>Jobe, D.</creatorcontrib><creatorcontrib>Gilliland, T.L.</creatorcontrib><creatorcontrib>Vargas, M.</creatorcontrib><creatorcontrib>Apruzese, J.P.</creatorcontrib><creatorcontrib>Thornhill, J.W.</creatorcontrib><creatorcontrib>Pulsifer, P.E.</creatorcontrib><creatorcontrib>Whitney, K.G.</creatorcontrib><creatorcontrib>Davis, J.</creatorcontrib><creatorcontrib>Cochran, S.L.</creatorcontrib><creatorcontrib>Velikovich, K.G.</creatorcontrib><creatorcontrib>Weber, B.V.</creatorcontrib><creatorcontrib>Peterson, G.</creatorcontrib><creatorcontrib>Mosher, D.</creatorcontrib><creatorcontrib>De Groot, J.S.</creatorcontrib><creatorcontrib>Hammer, J.H.</creatorcontrib><creatorcontrib>Sandia National Laboratory</creatorcontrib><collection>IEEE Electronic Library (IEL) Conference Proceedings</collection><collection>IEEE Proceedings Order Plan All Online (POP All Online) 1998-present by volume</collection><collection>IEEE Xplore All Conference Proceedings</collection><collection>IEEE Electronic Library (IEL)</collection><collection>IEEE Proceedings Order Plans (POP All) 1998-Present</collection><collection>OSTI.GOV</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Sanford, T.W.L.</au><au>Marder, B.M.</au><au>Spielman, R.B.</au><au>Nash, T.J.</au><au>Douglas, M.</au><au>Deeney, C.</au><au>Struve, K.</au><au>Mock, R.C.</au><au>Seamen, J.F.</au><au>McGurn, J.S.</au><au>Jobe, D.</au><au>Gilliland, T.L.</au><au>Vargas, M.</au><au>Apruzese, J.P.</au><au>Thornhill, J.W.</au><au>Pulsifer, P.E.</au><au>Whitney, K.G.</au><au>Davis, J.</au><au>Cochran, S.L.</au><au>Velikovich, K.G.</au><au>Weber, B.V.</au><au>Peterson, G.</au><au>Mosher, D.</au><au>De Groot, J.S.</au><au>Hammer, J.H.</au><aucorp>Sandia National Laboratory</aucorp><format>book</format><genre>proceeding</genre><ristype>CONF</ristype><atitle>Uniform fill improves K-shell power relative to annular fill for argon gas puffs on Saturn</atitle><btitle>IEEE Conference Record - Abstracts. 1996 IEEE International Conference on Plasma Science</btitle><stitle>PLASMA</stitle><date>1996</date><risdate>1996</risdate><spage>251</spage><pages>251-</pages><issn>0730-9244</issn><eissn>2576-7208</eissn><isbn>9780780333222</isbn><isbn>0780333225</isbn><abstract>Summary form only given. The radiation from uniform-fill argon gas puffs on the Saturn accelerator with a 4.5-cm diameter nozzle are compared with that generated from a previously optimized 2.5-cm diameter annular nozzle. The pressure range of the uniform fill spanned 1300 to 2900 Torr and that of the annular nozzle was set to 1650 Torr-the pressure that previously maximized the K-shell radiation yield. B-dot monitors measured current in the MITLs and 4.5 cm upstream of the load. A bolometer and duplicate sets of filtered XRDs and PCDs, spanning the energy range of 200 eV to 6 keV, monitored the temporal characteristics of the radiation. A suite of time-integrated and time-resolved, filtered, fast-framing, X-ray pinhole cameras, and crystal spectrometers monitored the spatial and spectral structure of the radiation. The radial density profile of the initial gas profile was measured on a test stand at NRL using a two-color interferometer.</abstract><cop>United States</cop><pub>IEEE</pub><doi>10.1109/PLASMA.1996.551486</doi></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | ISSN: 0730-9244 |
| ispartof | IEEE Conference Record - Abstracts. 1996 IEEE International Conference on Plasma Science, 1996, p.251 |
| issn | 0730-9244 2576-7208 |
| language | eng |
| recordid | cdi_ieee_primary_551486 |
| source | IEEE Electronic Library (IEL) Conference Proceedings |
| subjects | 07 ISOTOPE AND RADIATION SOURCE TECHNOLOGY ACCELERATORS Argon Cameras COMPARATIVE EVALUATIONS Current measurement Energy measurement Geometry Hydrodynamics IMPLOSIONS Laboratories LONGITUDINAL PINCH Physics PRESSURE DEPENDENCE Radiation monitoring Saturn X RADIATION X-RAY SOURCES |
| title | Uniform fill improves K-shell power relative to annular fill for argon gas puffs on Saturn |
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