Consequences of plasma-maser in plasma astrophysics

Details Consequences of plasma-maser in plasma astrophysics Consequences of plasma-maser in plasma astrophysics

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ppcn.conf..265n&link_type=abstract

In ESA, Fourth International Toki Conference on Plasma Physics and Controlled Nuclear Fusion p 265-268 (SEE N94-22624 05-75)

Physics

Plasma Physics

Interstellar Masers, Magnetohydrodynamic Stability, Plasma Interactions, Plasma-Particle Interactions, Turbulent Flow, Astrophysics, Magnetohydrodynamic Waves, Plasma Physics

Scientific paper

The plasma-maser interactions are discussed and possible applications to astrophysical plasmas are presented. The total energy conservation relation between particles, kinetic energy, and wave energy is studied. The Manley-Rowe relation among plasma waves is violated, and as a result an efficient energy up conversion from the low frequency mode to the high frequency mode is possible even for a normal unreversed electrons population in plasma turbulence. The plasma-maser process always coexists with the quasilinear interaction and is important in interpreting observations in astrophysical plasmas.

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