Publications

Savage, Mark E.; Austin, Kevin N.; Coffey, Sean K.; Jones, Peter A.; Joseph, Nathan R.; Kirschner, Debra S.; Lott, John A.; Oliver, Bryan V.; Spielman, Rick B.; Struve, Kenneth W.; Ulmen, Benjamin A.

Abstract not provided.

Savage, Mark E.; Austin, Kevin N.; Coffey, Sean K.; Jones, Peter A.; Joseph, Nathan R.; Kirschner, Debra S.; Lott, John A.; Oliver, Bryan V.; Spielman, Rick B.; Struve, Kenneth W.

Abstract not provided.

IEEE International Pulsed Power Conference

Savage, Mark E.; Struve, Kenneth W.; Austin, Kevin N.; Coffey, S.K.; Jones, Peter A.; Joseph, Nathan R.; Kirschner, Debra S.; Lott, John A.; Oliver, Bryan V.; Spielman, Rick B.

The Saturn X-ray generator is a 2.5 megavolt, 10 megampere electrical driver at Sandia National Laboratories. Saturn has been in operation for more than 30 years. Work is underway to identify key areas of the machine, improvement of which would benefit operational efficiency and reproducibility of the system. Saturn is used to create high-dose, short-pulse intense ionizing radiation environments for testing electronic and mechanical systems. Saturn has 36 identical modules driving a common electron beam bremsstrahlung load. Each module utilizes a microsecond Marx generator, a megavolt gas switch, and untriggered water switches in a largely conventional pulse-forming system. Achieving predictable and reliable radiation exposure is critical for users of the facility. Saturn has endured decades of continual use with minimal opportunities for research, improvements, or significant preventive maintenance. Because of degradation in components and limited attention to electrical performance, the facility has declined both in the number of useful tests per year and their repeatability. The Saturn system resides in a cylindrical tank 33m in diameter, and stores 5.6 MJ at the nominal operating Marx charge voltage. The system today is essentially identical to that described by Bloomquist in 1987. [1] Advances in technology for large pulsed power systems affords opportunities to improve the performance and more efficiently utilize the energy stored. Increased efficiency can improve reliability and reduce maintenance. The goals for the Saturn improvement work are increased shot rate, reduced X-ray dose shot-To-shot dose fluctuation, and reduced required maintenance. Major redesign with alternate pulsed power technology is considered outside the scope of this effort. More X-ray dose, larger exposure area, and lower X-ray endpoint energy are also important considerations but also deemed outside the scope of the present project due to schedule and resource constraints. The first considerations, described here, are improving the present design with better components.

Savage, Mark E.; Cuneo, M.E.; Davis, Jean-Paul D.; Hutsel, Brian T.; Jones, Michael J.; Jones, Peter A.; Kamm, Ryan J.; Lopez, Michael R.; Matzen, M.K.; McDaniel, D.H.M.; McKee, George R.; Maenchen, J.E.M.; Owen, A.C.O.; Porter, John L.; Prestwich, K.R.P.; Schwarz, Jens S.; Sinars, Daniel S.; Stoltzfus, Brian S.; Struve, Kenneth W.; Stygar, William A.; Wakeland, P.; White, William M.

Abstract not provided.

Physical Review Accelerators and Beams

Stygar, William A.; Reisman, David R.; Stoltzfus, Brian S.; Austin, Kevin N.; Benage, John F.; Breden, E.W.; Cooper, R.A.C.; Cuneo, M.E.; Davis, Jean-Paul D.; Ennis, J.B.E.; Gard, Paul D.; Greiser, G.W.G.; Gruner, Frederick R.; Haill, Thomas A.; Hutsel, Brian T.; Jones, Peter A.; LeChien, K.R.L.; Leckbee, Joshua L.; Lucero, Diego J.; McKee, George R.; Moore, James M.; Mulville, Thomas D.; Muron, David J.; Root, Seth R.; Savage, Mark E.; Sceiford, Matthew S.; Spielman, R.B.S.; Waisman, Eduardo M.; Wisher, Matthew L.

In this study, we have developed a conceptual design of a next-generation pulsed-power accelerator that is optmized for driving megajoule-class dynamic-material-physics experiments at pressures as high as 1 TPa. The design is based on an accelerator architecture that is founded on three concepts: single-stage electrical-pulse compression, impedance matching, and transit-time-isolated drive circuits. Since much of the accelerator is water insulated, we refer to this machine as Neptune. The prime power source of Neptune consists of 600 independent impedance-matched Marx generators. As much as 0.8 MJ and 20 MA can be delivered in a 300-ns pulse to a 16-mΩ physics load; hence Neptune is a megajoule-class 20-MA arbitrary waveform generator. Neptune will allow the international scientific community to conduct dynamic equation-of-state, phase-transition, mechanical-property, and other material-physics experiments with a wide variety of well-defined drive-pressure time histories. Because Neptune can deliver on the order of a megajoule to a load, such experiments can be conducted on centimeter-scale samples at terapascal pressures with time histories as long as 1 μs.

Digest of Technical Papers-IEEE International Pulsed Power Conference

Hutsel, Brian T.; Stoltzfus, Brian S.; Breden, E.W.; Fowler, W.E.; Jones, Peter A.; Justus, D.W.; Long, Finis W.; Lucero, Diego J.; Macrunnels, K.A.; Mazarakis, Michael G.; Mckenney, John M.; Moore, James M.; Mulville, Thomas D.; Porter, John L.; Savage, Mark E.; Stygar, William A.

An experiment platform has been designed to study vacuum power flow in magnetically insulated transmission lines (MITLs) the platform is driven by the Mykonos-V LTD accelerator to drive a coaxial MITL with a millimeter-scale anode-cathode gap the experiments conducted quantify the current loss in the MITL with respect to vacuum pumpdown time and vacuum pressure. MITL gaps between 1.0 mm and 1.3 mm were tested the experiment results revealed large differences in performance for the 1.0 and 1.3 mm gaps the 1.0 mm gap resulted in current losses of 40%-60% of the peak current the 1.3 mm gap resulted in current losses of less than 5% of peak current. Classical MITL models that neglect plasma expansion predict that there should be zero current loss, after magnetic insulation is established, for both of these gaps.

Savage, Mark E.; Stoltzfus, Brian S.; Austin, Kevin N.; Jones, Peter A.; Stygar, William A.; Joseph, Nathan R.; Moore, James M.

Abstract not provided.

Savage, Mark E.; Stoltzfus, Brian S.; Austin, Kevin N.; Jones, Peter A.; Stygar, William A.; Joseph, Nathan R.; Moore, James M.

Abstract not provided.

Review of Scientific Instruments

Rovang, Dean C.; Lamppa, Derek C.; Cuneo, M.E.; Owen, A.C.; Mckenney, John M.; Johnson, Drew J.; Radovich, S.; Kaye, Ronald J.; McBride, Ryan D.; Alexander, Charles S.; Awe, T.J.; Slutz, S.A.; Sefkow, Adam B.; Haill, Thomas A.; Jones, Peter A.; Argo, J.W.; Dalton, D.G.; Robertson, Grafton K.; Waisman, Eduardo M.; Sinars, Daniel S.; Meissner, J.; Milhous, M.; Nguyen, D.N.; Mielke, C.H.

Sandia has successfully integrated the capability to apply uniform, high magnetic fields (10-30 T) to high energy density experiments on the Z facility. This system uses an 8-mF, 15-kV capacitor bank to drive large-bore (5 cm diameter), high-inductance (1-3 mH) multi-turn, multi-layer electromagnets that slowly magnetize the conductive targets used on Z over several milliseconds (time to peak field of 2-7 ms). This system was commissioned in February 2013 and has been used successfully to magnetize more than 30 experiments up to 10 T that have produced exciting and surprising physics results. These experiments used split-magnet topologies to maintain diagnostic lines of sight to the target. We describe the design, integration, and operation of the pulsed coil system into the challenging and harsh environment of the Z Machine. We also describe our plans and designs for achieving fields up to 20 T with a reduced-gap split-magnet configuration, and up to 30 T with a solid magnet configuration in pursuit of the Magnetized Liner Inertial Fusion concept.

Gomez, Matthew R.; Savage, Mark E.; Stoltzfus, Brian S.; Struve, Kenneth W.; Stygar, William A.; Cuneo, M.E.; Fowler, William E.; Hutsel, Brian T.; Jones, Peter A.; Lucero, Diego J.; Matzen, M.K.; McKee, George R.

Abstract not provided.

Stygar, William A.; Fowler, William E.; Gomez, Matthew R.; Harmon, Roger L.; Herrmann, Mark H.; Huber, Dale L.; Hutsel, Brian T.; Bailey, James E.; Jones, Michael J.; Jones, Peter A.; Leckbee, Joshua L.; Lee, James R.; Lewis, Scot A.; Long, Finis W.; Lopez, Mike R.; Lucero, Diego J.; Matzen, M.K.; Mazarakis, Michael G.; McBride, Ryan D.; McKee, George R.; Nakhleh, Charles N.; Owen, Albert C.; Rochau, G.A.; Savage, Mark E.; Schwarz, Jens S.; Sefkow, Adam B.; Sinars, Daniel S.; Stoltzfus, Brian S.; Vesey, Roger A.; Wakeland, P.; Cuneo, M.E.; Flicker, Dawn G.; Focia, Ronald J.

Abstract not provided.