Radio Radiation Mechanism of Two-Streams Plasma in the Astrophysical Jet
LU Shengzhi1, TONG Yi2, SU Yang3
1Department of Physics, Beijing Normal University, Beijing 100875
2Department of Astronomy, Beijing Normal University, Beijing 100875
3Beijing Astronomical Observatory, Academia Sinica, Beijing 100080
Radio Radiation Mechanism of Two-Streams Plasma in the Astrophysical Jet
LU Shengzhi1;TONG Yi2;SU Yang3
1Department of Physics, Beijing Normal University, Beijing 100875
2Department of Astronomy, Beijing Normal University, Beijing 100875
3Beijing Astronomical Observatory, Academia Sinica, Beijing 100080
Abstract： To explain the radio mechanism of non-relativistic jets, we investigate a nonlinear process in which ion-acoustic waves scatter into high frequency electromagnetic waves by the plasma having a non-Maxwell distribution with non-relativisical energetic electrons. The calculated reaults show that this mechanism is efficient, and may apply to the radiation of jets from active galaxies and radio bursts of sun flares.
(Waves, oscillations, and instabilities in plasmas and intense beams)
引用本文:
LU Shengzhi;TONG Yi;SU Yang. Radio Radiation Mechanism of Two-Streams Plasma in the Astrophysical Jet[J]. 中国物理快报, 1995, 12(3): 189-192.
LU Shengzhi, TONG Yi, SU Yang. Radio Radiation Mechanism of Two-Streams Plasma in the Astrophysical Jet. Chin. Phys. Lett., 1995, 12(3): 189-192.
1995, Vol. 12 
