Publications

Struve, Kenneth W.; McGurn, John S.

Abstract not provided.

Nielsen, D.S.; Rochau, G.A.; Bailey, James E.; Chandler, Gordon A.; McGurn, John S.; Nash, Thomas J.

Abstract not provided.

Proposed for publication in Physical Review E.

Stygar, William A.; Leeper, Ramon J.; Mazarakis, Michael G.; McDaniel, Dillon H.; Mckenney, John M.; Mills, Jerry A.; Ruggles, Larry R.; Seamen, Johann F.; Simpson, Walter W.; Dropinski, Steven D.; Warne, Larry K.; York, Matthew W.; McGurn, John S.; Bryce, Edwin A.; Chandler, Gordon A.; Cuneo, M.E.; Johnson, William Arthur.; Jorgenson, Roy E.

We have developed a diagnostic system that measures the spectrally integrated (i.e. the total) energy and power radiated by a pulsed blackbody x-ray source. The total-energy-and-power (TEP) diagnostic system is optimized for blackbody temperatures between 50 and 350 eV. The system can view apertured sources that radiate energies and powers as high as 2 MJ and 200 TW, respectively, and has been successfully tested at 0.84 MJ and 73 TW on the Z pulsed-power accelerator. The TEP system consists of two pinhole arrays, two silicon-diode detectors, and two thin-film nickel bolometers. Each of the two pinhole arrays is paired with a single silicon diode. Each array consists of a 38 x 38 square array of 10-{micro}m-diameter pinholes in a 50-{micro}m-thick tantalum plate. The arrays achromatically attenuate the x-ray flux by a factor of {approx}1800. The use of such arrays for the attenuation of soft x rays was first proposed by Turner and co-workers [Rev. Sci. Instrum. 70, 656 (1999)RSINAK0034-674810.1063/1.1149385]. The attenuated flux from each array illuminates its associated diode; the diode's output current is recorded by a data-acquisition system with 0.6-ns time resolution. The arrays and diodes are located 19 and 24 m from the source, respectively. Because the diodes are designed to have an approximately flat spectral sensitivity, the output current from each diode is proportional to the x-ray power. The nickel bolometers are fielded at a slightly different angle from the array-diode combinations, and view (without pinhole attenuation) the same x-ray source. The bolometers measure the total x-ray energy radiated by the source and--on every shot--provide an in situ calibration of the array-diode combinations. Two array-diode pairs and two bolometers are fielded to reduce random uncertainties. An analytic model (which accounts for pinhole-diffraction effects) of the sensitivity of an array-diode combination is presented.

Journal of Quantitative Spectroscopy and Radiative Transfer

Nash, Thomas J.; Sanford, T.W.L.; Mock, R.C.; Leeper, Ramon J.; Chandler, Gordon A.; Bailey, James E.; Mckenney, John M.; Mehlhorn, Thomas A.; Seaman, J.F.; McGurn, John S.; Schroen, D.; Russell, C.; Lake, P.E.; Jobe, D.O.; Gilliland, Terrance L.; Nielsen, D.S.; Lucas, J.; Moore, T.; Torres, J.A.; Macfarlane, Joseph J.; Apruzese, J.P.; Chrien, R.; Idzorek, G.; Peterson, D.L.; Watt, R.

We present results from crystal spectroscopic analysis of silicon aero-gel foams heated by dynamic hohlraums on Z. The dynamic hohlraum on Z creates a radiation source with a 230-eV average temperature over a 2.4-mm diameter. In these experiments silicon aero-gel foams with 10 - mg/cm3 densities and 1.7-mm lengths were placed on both ends of the dynamic hohlraum. Several crystal spectrometers were placed both above and below the z-pinch to diagnose the temperature of the silicon aero-gel foam using the K-shell lines of silicon. The crystal spectrometers were (1) temporally integrated and spatially resolved, (2) temporally resolved and spatially integrated, and (3) both temporally and spatially resolved. The results indicate that the dynamic hohlraum heats the silicon aero-gel to approximately 150-eV at peak power. As the dynamic hohlraum source cools after peak power the silicon aero-gel continues to heat and jets axially at an average velocity of approximately 50-cm/μs. The spectroscopy has also shown that the reason for the up/down asymmetry in radiated power on Z is that tungsten enters the line-of-sight on the bottom of the machine much more than on the top. © 2004 Elsevier Ltd. All rights reserved.

Proposed for publication in Physics of Plasmas.

Vesey, Roger A.; Yu, Edmund Y.; Nash, Thomas J.; Bliss, David E.; Bennett, Guy R.; Sinars, Daniel S.; Simpson, Walter W.; Ruggles, Larry R.; Wenger, D.F.; Garasi, Christopher J.; Aragon, Rafael A.; Fowler, William E.; Johnson, Drew J.; Keller, Keith L.; McGurn, John S.; Mehlhorn, Thomas A.; Speas, Christopher S.; Struve, Kenneth W.; Stygar, William A.; Chandler, Gordon A.

Abstract not provided.

Nash, Thomas J.; Lake, Patrick W.; Moore, T.C.; Schroen, D.G.; Seamen, Johann F.; McGurn, John S.; Jobe, Daniel O.; Mock, Raymond M.; Sanford, Thomas W.; Nielsen, D.S.; Nash, Thomas J.; Hawn, Rona E.; Chandler, Gordon A.; Bailey, James E.; Slutz, Stephen A.; Mehlhorn, Thomas A.; Leeper, Ramon J.; Ruiz, Carlos L.; Cooper, Gary W.

Abstract not provided.

Leeper, Ramon J.; Deeney, Christopher D.; Dunham, Gregory S.; Fehl, David L.; Franklin, James K.; Hawn, Rona E.; Hall, Clint A.; Hurst, Michael J.; Jinzo, Tanya D.; Jobe, Daniel O.; Leeper, Ramon J.; Joseph, Nathan R.; Knudson, Marcus D.; Lake, Patrick W.; Lazier, Steven E.; Lucas, J.; McGurn, John S.; Manicke, Matthew P.; Mock, Raymond M.; Moore, T.C.; Nash, Thomas J.; Bailey, James E.; Nelson, Alan J.; Nielsen, D.S.; Olson, Richard E.; Pyle, John H.; Rochau, G.A.; Ruggles, Larry R.; Ruiz, Carlos L.; Sanford, Thomas W.; Seamen, Johann F.; Bennett, Guy R.; Simpson, Walter W.; Sinars, Daniel S.; Speas, Christopher S.; Stygar, William A.; Wenger, D.F.; Seamen, Johann J.; Carlson, Alan L.; Chandler, Gordon A.; Cooper, Gary W.; Cuneo, M.E.

Abstract not provided.

Proposed for publication in Physical Review E.

Stygar, William A.; Matzen, M.K.; Mazarakis, Michael G.; McDaniel, Dillon H.; McGurn, John S.; Mckenney, John M.; Mix, L.P.; Muron, David J.; Ramirez, Juan J.; Ruggles, Larry R.; Stygar, William A.; Seamen, Johann F.; Simpson, Walter W.; Speas, Christopher S.; Spielman, Rick B.; Struve, Kenneth W.; Vesey, Roger A.; Wagoner, Tim C.; Gilliland, Terrance L.; Bennett, Guy R.; Ives, Harry C.; Jobe, Daniel O.; Lazier, Steven E.; Mills, Jerry A.; Mulville, Thomas D.; Pyle, John H.; Romero, Tobias M.; Seamen, Johann F.; Serrano, Jason D.; Smelser, Ruth S.; Fehl, David L.; Cuneo, M.E.; Bailey, James E.; Bliss, David E.; Chandler, Gordon A.; Leeper, Ramon J.

Abstract not provided.

Physics of Plasmas

Cuneo, M.E.; Vesey, Roger A.; Porter, John L.; Chandler, Gordon A.; Fehl, David L.; Gilliland, Terrance L.; Hanson, David L.; McGurn, John S.; Reynolds, Paul G.; Ruggles, Larry R.; Seamen, Hans; Spielman, Rick B.; Struve, Kenneth W.; Stygar, William A.; Simpson, Walter W.; Torres, Jose A.; Wenger, D.F.; Hammer, James H.; Rambo, Peter W.; Peterson, Darrell L.; Idzorek, George C.

Initial experiments to study the Z-pinch-driven hohlraum high-yield inertial confinement fusion (ICF) concept of Hammer, Tabak, and Porter [Hammer et al., Phys. Plasmas 6, 2129 (1999)] are described. The relationship between measured pinch power, hohlraum temperature, and secondary hohlraum coupling ("hohlraum energetics") is well understood from zero-dimensional semianalytic, and two-dimensional view factor and radiation magnetohydrodynamics models. These experiments have shown the highest x-ray powers coupled to any Z-pinch-driven secondary hohlraum (26±5 TW), indicating the concept could scale to fusion yields of >200 MJ. A novel, single-sided power feed, double-pinch driven secondary that meets the pinch simultaneity requirements for polar radiation symmetry has also been developed. This source will permit investigation of the pinch power balance and hohlraum geometry requirements for ICF relevant secondary radiation symmetry, leading to a capsule implosion capability on the Z accelerator [Spielman et al., Phys. Plasmas 5, 2105 (1998)]. © 2001 American Institute of Physics.