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Excitation of Electromagnetic Waves by an Electron Ring Beam in a Magnetized Plasma Waveguide |
| ZHOU Guo-Cheng1;WU Ching-Sheng2,3;WANG De-Ju1;CHEN Yan-Ping4,5 |
| 1Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing 100080
2Department of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026
3Institute for Physical Science and Technology, College Park, MD 20742, USA
4National Astronomical Observatory, Chinese Academy of Sciences, Beijing 100012
5Institute of Physics, Chinese Academy of Sciences, Beijing 100080
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| Cite this article: |
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ZHOU Guo-Cheng, WU Ching-Sheng, WANG De-Ju et al 2002 Chin. Phys. Lett. 19 1556-1559 |
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Abstract We study the resonant interactions between an electron ring eam and plasma waveguide modes. This is motivated by the research of radio emission in low solar corona. We consider a density-depleted duct (above an active region near a flare site) that may be treated as a magnetized plasma waveguide. The electromagnetic waves excited in the waveguide are classified into the so-called E- and B-type waves. The results show that there are two unstable modes of B-type waves propagating parallelly and anti-parallelly to the direction of the electron beam, and the effect of the finite radius and boundary conditions of the waveguide on the excitation of waveguide modes is important. For a given B-type mode, the smaller the radius R, the larger the temporal and spatial amplification rate. We suggest that these excited waveguide modes could be one of the processes responsible for the observed solar radio emission.
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| Keywords:
95.30.Gv
95.30.Qd
95.85.Bh
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Published: 01 October 2002
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| PACS: |
95.30.Gv
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(Radiation mechanisms; polarization)
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95.30.Qd
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(Magnetohydrodynamics and plasmas)
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95.85.Bh
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(Radio, microwave (>1 mm))
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