Electron acceleration by Z-mode waves associated with cyclotron maser instability
Creators
- 1. Institute of Space Science, National Central University, Zhongli, Taiwan (China)
- 2. Research Institute for Sustainable Humanosphere, Kyoto University, Uji, Kyoto (Japan)
Description
We demonstrate by a particle simulation that Z-mode waves generated by the cyclotron maser instability can lead to a significant acceleration of energetic electrons. In the particle simulation, the initial electron ring distribution leads to the growth of Z-mode waves, which then accelerate and decelerate the energetic ring electrons. The initial ring distribution evolves into an X-like pattern in momentum space, which can be related to the electron diffusion curves. The peak kinetic energy of accelerated electrons can reach 3 to 6 times the initial kinetic energy. We further show that the acceleration process is related to the "nonlinear resonant trapping" in phase space, and the test-particle calculations indicate that the maximum electron energy gain Δεmax is proportional to Bw0.57, where Bw is the wave magnetic field.
Additional details
Identifiers
- DOI
- 10.1063/1.4772059;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 19
- Journal Issue
- 12
- Journal Page Range
- p. 122902-122902.5
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44032388
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ACCELERATION; CYCLOTRONS; DIFFUSION; ELECTRON RINGS; KINETIC ENERGY; MAGNETIC FIELDS; MASERS; PHASE SPACE; PLASMA INSTABILITY; PLASMA SIMULATION; TAIL ELECTRONS; TEST PARTICLES; TRAPPING; WAVE PROPAGATION
- Descriptors DEC
- ACCELERATORS; AMPLIFIERS; CYCLIC ACCELERATORS; ELECTRONIC EQUIPMENT; ELECTRONS; ELEMENTARY PARTICLES; ENERGY; EQUIPMENT; FERMIONS; INSTABILITY; LEPTONS; MATHEMATICAL SPACE; MICROWAVE AMPLIFIERS; MICROWAVE EQUIPMENT; SIMULATION; SPACE
Optional Information
- Notes
- (c) 2012 American Institute of Physics