Physics
Scientific paper
Apr 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998jpsj...67.1079k&link_type=abstract
Journal of the Physical Society of Japan, Vol. 67, No. 4, p. 1079 - 1082
Physics
17
Plasma Clouds: Magnetic Fields, Plasma Clouds: Stellar Winds
Scientific paper
The authors present the results of analytical studies and computer simulations of electron-ion plasma cloud collisions using 2D3V particle-in-cell and 2D two-fluid collisionless relativistic codes. They address the problem concerning the generation of a quasistatic magnetic field. Using relativistic two-fluid equations for the two counterstreaming electron populations, they show with the help of linear theory that the generation of a magnetic field can be associated with the "electromagnetic counterstreaming instability". Two-dimensional (2D) particle-in-cell provide good agreement with the results of linear theory. The authors show that the quasistatic magnetic field collisionless change of structure, leading to large-scale, long-lived structures. These processes may be important for the understanding of magnetic field generation in laser plasmas and in space plasmas in the regions where two stellar winds collide.
Bulanov Sergei
Califano Francesco
Kazimura Yoshihiro
Neubert Torsten
Pegoraro Francesco
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