Any offers of collaboration are welcome!

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.

Publications

• Numerical modeling of plasma spread in non-uniform magnetic field. International conference of computational technologies. Institute of Computational Technologies. Novosibirsk, Russia. Sep. 2000.http://www.ict.nsc.ru/ws/show_abstract.dhtml?ru+8+815
• 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. [http://arxiv.org/abs/physics/0603239v1]
• D. A. Osipyan. Collisionless scattering of plasma cloud in dipole magnetic field.
  Proc. NAS of Armenia. T41 #4. 2006.[pdf]
• 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 [http://arxiv.org/abs/0711.4945v1]
• H.B. Nersisyan, D.A. Osipyan. Collisionless plasma expansion in the presence of a dipole magnetic field .
  Contrib. Plasma Phys. 49, 351, (2009). [http://arxiv.org/abs/0905.0051]