Inverse liner z-pinch: an experimental pulsed power platform for studying radiative shocks
Autor: | Jingtan Ma, Thomas Clayson, Eleanor Tubman, Francisco Suzuki-Vidal, Jack Hare, Sergey Lebedev, Lee Suttle, J. W. D. Halliday, G. C. Burdiak |
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Přispěvatelé: | AWE Plc, The Royal Society, Engineering & Physical Science Research Council (EPSRC), Royal Society, U.S Department of Energy |
Rok vydání: | 2018 |
Předmět: |
ASTROPHYSICS
Nuclear and High Energy Physics Astrophysics::High Energy Astrophysical Phenomena Fluids & Plasmas chemistry.chemical_element Pulsed power 01 natural sciences 010305 fluids & plasmas law.invention Optics 0202 Atomic Molecular Nuclear Particle And Plasma Physics Physics Fluids & Plasmas law 0103 physical sciences medicine Radiative transfer Magnetic pressure 010306 general physics Astrophysics::Galaxy Astrophysics Physics Argon Science & Technology Electric shock business.industry 0906 Electrical And Electronic Engineering Condensed Matter Physics medicine.disease Laser Interferometry chemistry Z-pinch Physical Sciences LASER radiative shocks business |
Popis: | We present a new experimental platform for studying radiative shocks using an ``inverse liner z-pinch'' configuration. This platform was tested on the MAGPIE pulsed power facility (~1 MA with a rise time of ~240 ns) at Imperial College London, U.K. Current is discharged through a thin-walled metal tube (a liner) embedded in a low-density gas-fill and returned through a central post. The resulting magnetic pressure inside the liner launched a cylindrically symmetric, expanding radiative shock into the gas-fill at ~10 km/s. This experimental platform provides good diagnostic access, allowing multiframe optical self-emission imaging, laser interferometry, and optical emission spectrography to be fielded. Results from experiments with an Argon gas-fill initially at 0.04 mg/cm³are presented, demonstrating the successful production of cylindrically symmetric, expanding shocks that exhibit radiative effects such as the formation of a radiative precursor. |
Databáze: | OpenAIRE |
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