Any offers of collaboration are welcome!

Upcoming 3D PIC simulations

1. Plasma cloud expansion in magnetized background plasma (uniform/dipole magnetic field).

  • Structure of magnetic field perturbation. T heir velocity (for example, on overshoot).
  • Cloud front velocity.
  • Cloud and background ions dynamics (phase trajectories, velocity vector field, particle trajectories). Thiir relation with electromagnetic fields.
  • Compare results for various numbers of the Mach-Alfven and MLM numbers.

2. Magnetized flow interaction with the magnetic dipole.


  • Numerical modeling of plasma spread in non-uniform magnetic field. International conference of computational technologies. Institute of Computational Technologies. Novosibirsk, Russia. Sep. 2000.
  • D. A. Osipyan, H. B. Nersisyan, and H. H. Matevosyan. Collisionless slowing down of nova and supernova shells in magnetized interstellar medium. Astrophysics Journ. T46 #4. 2003 [pdf]
  • H. B. Nersisyan, D. A. Osipyan. The moving boundary problem in the presence of a dipole magnetic field.
    J. Phys. A: Math. Gen. 39. 2006. []
  • D. A. Osipyan. Collisionless scattering of plasma cloud in dipole magnetic field.
    Proc. NAS of Armenia. T41 #4. 2006
  • H.B. Nersisyan, D.A. Osipyan, G. Zwicknagel. Renormalized cluster expansion of the microfield distribution in a strongly coupled two-component plasmas.Phys. Rev. E 77, 2008 []
  • H.B. Nersisyan, D.A. Osipyan. Collisionless plasma expansion in the presence of a dipole magnetic field .
    Contrib. Plasma Phys. 49, 351, (2009). []




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