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Title: Plasma evolution from laser-driven gold disks. I. Experiments and results

Journal Article · · Physics of Fluids B; (USA)
DOI:https://doi.org/10.1063/1.859509· OSTI ID:6478072
 [1]; ;  [2];  [3]; ;  [4]
  1. Department of Physics, Eastern Michigan University, Ypsilanti, MI (USA) KMS Fusion Inc., Ann Arbor, MI (USA)
  2. KMS Fusion Inc., Ann Arbor, MI (USA)
  3. Schlumberger-Doll Research, Ridgefield, CT (USA) KMS Fusion Inc., Ann Arbor, MI (USA)
  4. Lawrence Livermore National Laboratory, Livermore, CA (USA)

Gold disk targets were irradiated with green ({lambda}=0.53 {mu}m) laser light at intensities between 0.5 and 5{times}10{sup 14} W/cm{sup 2} using shaped laser pulses. Plasma conditions near and below critical density ({ital n}{sub {ital c}}{congruent}4{times}10{sup 21}/cm{sup 3}) were determined from three diagnostics. Streaked one-dimensional images of the {ital M}-band emission (2--3.5 keV) along the laser axis yield the peak emission trajectory. Temporally and spatially averaged measurements of the hard x-ray spectrum (4--25 keV) were used to determine the average coronal electron temperature. Holographic interferometry was used to determine the electron density profiles and scale lengths along the laser axis. The peak emission trajectory, electron temperature, and scale lengths are all in good agreement with simulations, but the magnitudes of the electron density profiles are not, as discussed in an accompanying paper (Phys. Fluids B {bold 2}, 2448 (1990)).

DOE Contract Number:
AC03-87DP10560
OSTI ID:
6478072
Journal Information:
Physics of Fluids B; (USA), Vol. 2:10; ISSN 0899-8221
Country of Publication:
United States
Language:
English