On the generation of magnetic fields due to ponderomotive forces in astrophysical plasmas

Details On the generation of magnetic fields due to ponderomotive forces in astrophysical plasmas On the generation of magnetic fields due to ponderomotive forces in astrophysical plasmas

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002jplph..67..129c&link_type=abstract

Journal of Plasma Physics, vol. 67, Issue 03, p.129-138

Physics

Plasma Physics

Scientific paper

The generation of magnetic fields due to ponderomotive forces in astrophysical plasma consisting of electrons, ions and positrons is investigated theoretically. It is seen that collisional or non-collisional interactions (between electromagnetic waves and plasma particles) via ponderomotive forces in an inhomogeneous plasma can excite a magnetic field. The growth rate of the magnetic field is illustrated graphically for different values of the temperature and concentration of positrons in the plasma.

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