Self-generated magnetic field by transverse plasmons in celestial bodies

Details Self-generated magnetic field by transverse plasmons in celestial bodies Self-generated magnetic field by transverse plasmons in celestial bodies

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...270..534l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 270, no. 1-2, p. 534-542.

Astronomy and Astrophysics

Astrophysics

21

Celestial Bodies, Cosmic Plasma, Interstellar Magnetic Fields, Plasmons, Wave-Particle Interactions, Nonlinear Equations, Wave Interaction

Scientific paper

We suggest that a quasi-steady magnetic field could be generated in plasmas with HF radiation through wave-wave and wave-particle interactions. It is shown that the behavior of self-generated magnetic fields can be described by nonlinear coupling equations. Numerical results show that a magnetic field self-generated by transverse pumping plasmons may collapse, leading to enhancement of the magnetic field up to 1000 G in a range around 200 km, which corresponds to the observed small-scale fields on the solar surface.

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