期刊
PHYSICAL REVIEW LETTERS
卷 109, 期 12, 页码 -出版社
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.109.125003
关键词
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资金
- NSF [ATM-0852682, ATM-0646442, S.- ATM0902730]
- NASA [NNX10AK97G]
- PPPL by NASA [NNG07EK69I, NNH07AF37I, NNH09AM53I, V NNH09AK63I, NNH11AR07I]
- DOE [DE-AC02-09CH11466]
- [NSFC 41028003]
- [NSFC 40890163]
- Direct For Mathematical & Physical Scien
- Division Of Physics [0903794] Funding Source: National Science Foundation
- Div Atmospheric & Geospace Sciences
- Directorate For Geosciences [0852682] Funding Source: National Science Foundation
- NASA [NNX10AK97G, 130105] Funding Source: Federal RePORTER
We report the first three-dimensional (3D) ion particle simulation of mode conversion from a fast mode compressional wave to kinetic Alfven waves (KAWs) that occurs when a compressional mode propagates across a plasma boundary into a region of increasing Alfven velocity. The magnetic field is oriented in the (z) over cap direction perpendicular to the gradients in the background density and magnetic field ((x) over cap direction). Following a stage dominated by linear physics in which KAWs with large wave numbers k(x)rho(i) similar to 1 (with rho(i) being the ion Larmor radius) are generated near the Alfven resonance surface, the growth of KAW modes with k(y)rho(i) similar to 1 is observed in the nonlinear stage when the amplitude of KAWs generated by linear mode conversion becomes large enough to drive a nonlinear parametric decay process. The simulation provides a comprehensive picture of mode conversion and shows the fundamental importance of the 3D nonlinear physics in transferring energy to large perpendicular k(y) modes, which can provide large transport across plasma boundaries in space and laboratory plasmas.
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