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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
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| Cite this article: |
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LU Shengzhi, TONG Yi, SU Yang 1995 Chin. Phys. Lett. 12 189-192 |
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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.
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98.62.Nx
52.35.-g
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Published: 01 March 1995
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| PACS: |
98.62.Nx
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(Jets and bursts; galactic winds and fountains)
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52.35.-g
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(Waves, oscillations, and instabilities in plasmas and intense beams)
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