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A fast parallel code for calculating energies and oscillator strengths of many-electron atoms at neutron star magnetic field strengths in adiabatic approximation.

Dirk EngelMatthias KlewsGünter Wunner
Published in: Comput. Phys. Commun. (2009)
Keyphrases
  • magnetic field
  • electromagnetic fields
  • eddy current
  • parallel processing
  • markov random field
  • source code
  • real time
  • higher order
  • graph cuts
  • electron microscopy