0 Ju l 2 00 4 Weibel instability on weakly relativistic produced plasma by circular polarization microwave electric field ∗
نویسنده
چکیده
Analyzing the production of weakly relativistic plasma produced by microwave fields with circular polarization the electron distribution function is obtained to be non-equilibrium and anisotropic. Furthermore, it is shown that produced plasma is accelerated on the direction of propagation of microwave electric fields. The electron velocity on this direction strongly depends on electron origination phase, electric field phase, and amplitude of microwave electric field. Making use of the dielectric tensor obtained for this plasma, it is shown that the wiebel instability develops due to the anisotrpic property of PACS52.40.Db,52.35.Hr E-mail:[email protected]
منابع مشابه
7 A ug 2 00 4 Low - frequency instability of circularly polarized microwave - pulsed - field - produced plasmas ∗
The plasma produced by a high-power pulsed circularly polarized microwave field which is much weaker than the atomic fields is investigated in the non-relativistic limit. It is shown that the resulting electron distribution function is non-equilibrium and anisotropic. Furthermore, the dispersion equations derived to study and analyze low-frequency ion oscillations. It is shown an instability ma...
متن کامل2 0 Ju l 2 00 5 Forces between electric charges in motion : Rutherford scattering , circular Keplerian orbits , action - at - a - distance and Newton ’ s third law in relativistic classical electrodynamics
Standard formulae of classical electromagnetism for the forces between electric charges in motion derived from retarded potentials are compared with those obtained using an instantaneous Coulomb force described by a 4-vector electromagnetic potential. Problems discussed include small angle Rutherford scattering, Jackson's recent 'torque paradox' and circular Keplerian orbits. Results consistent...
متن کاملar X iv : a st ro - p h / 04 10 19 3 v 1 7 O ct 2 00 4 Relativistic Shocks : Particle Acceleration , Magnetic Field Generation , and Emission
Shock acceleration is an ubiquitous phenomenon in astrophysical plasmas. Plasma waves and their associated instabilities (e.g., Buneman, Weibel and other two-stream instabilities) created in collisionless shocks are responsible for particle (electron, positron, and ion) acceleration. Using a 3-D relativistic electromagnetic particle (REMP) code, we have investigated particle acceleration associ...
متن کاملMagnetic field generation in relativistic shocks
We present an analytical estimate for the magnetic field strength generated by the Weibel instability in ultra-relativistic shocks in a hydrogen plasma. We find that the Weibel instability is, by itself, not capable of converting the kinetic energy of protons penetrating the shock front into magnetic field energy. Other (nonlinear) processes must determine the magnetic field strength in the wak...
متن کاملParticle Acceleration and Magnetic Field Generation in Electron - Positron Relativistic Shocks
Shock acceleration is an ubiquitous phenomenon in astrophysical plasmas. Plasma waves and their associated instabilities (e.g., Buneman, Weibel and other two-stream instabilities) created in collisionless shocks are responsible for particle (electron, positron, and ion) acceleration. Using a 3-D relativistic electromagnetic particle (REMP) code, we have investigated particle acceleration associ...
متن کامل