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- W2746808212 abstract "A 100-μm-thick Cu foil is isochorically heated by a ∼100-ns-long electron bunch with an energy of 19.8 MeV and current of 1.7 kA to Te > 1 eV. After 100 ns of heating and 20 ns of expansion, the plasma exhibits a stable, quiescent temperature and density distribution for >200 ns. Several intense Cu-I emission lines are observed after ∼20 J of electron beam energy is deposited. These lines have well known Stark widths providing a direct measurement of ne. The Los Alamos ATOMIC code [Magee et al., AIP Conf. Proc. 2004, 168–179 and Hakel et al., J. Quant. Spectrosc. Radiat. Transfer 99, 265 (2006)] was run in local-thermodynamic-equilibrium mode to estimate Te and ne. Spatially and temporally resolved measurements are presented in both the vertical and horizontal directions adjacent to the foil indicating temperatures >1 eV and densities ranging from 1–3 × 1017 cm−3 after expansion and cooling." @default.
- W2746808212 created "2017-08-31" @default.
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- W2746808212 date "2017-08-01" @default.
- W2746808212 modified "2023-10-03" @default.
- W2746808212 title "Spatially and temporally resolved measurements of a dense copper plasma heated by intense relativistic electrons" @default.
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- W2746808212 doi "https://doi.org/10.1063/1.4989797" @default.
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