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Simulation of mode conversion at the magnetopause
  • ISSN号:1001-6538
  • 期刊名称:Chinese Science Bulletin
  • 时间:0
  • 页码:1375-1383
  • 分类:O353.2[理学—流体力学;理学—力学] S513.01[农业科学—作物学]
  • 作者机构:[1]Physics Department, Auburn University, Auburn 36849, USA, [2]Department of Geophysics and Planetary Science, University of Science and Technology of China, Hefei 230026, China, [3]princeton Plasma Physics Laboratory, Princeton University, Princeton 08543, USA
  • 相关基金:Computer resources were provided by NAS and ASC. This work was suppor- ted by NSFC grants (41028003 and 40890163), NSF grants (ATM-0852682 and ATM-0646442) and NASA grant NNXlOAK97G to Auburn University, and at PPPL by NASA grants (NNGO7EK691, NNHO7AF371, NNHOgAM531, NNHO9AK631, and NNH11AQ46I), NSF grant ATM0902730, and DOE con- tract DE-AC02-09Ch11466.
  • 相关项目:太阳风-磁层-电离层相互作用和耦合的三维混合粒子模拟和卫星与地面观测研究
中文摘要:

二维(2-D ) 并且三维(3-D ) 混合模拟从快模式为模式变换被执行有压缩性向运动 Alfv 挠汯楬楳湯敬獳洠条敮楴? 敲潣湮 ' 虡 N 湯 ? 慨 ? 敢湥猠畴楤摥映牯洠牯 ? 桴湡 ?‵敹牡 s 招手

英文摘要:

Two-dimensional (2-D) and three-dimensional (3-D) hybrid simulations are carried out for mode conversion from fast mode com- pressional wave to kinetic Alfv6n waves (KAWs) at the inhomogeneous magnetopause boundary. For cases in which the incident fast wave propagates in the xz plane, with the magnetopause normal along x and the background magnetic field pointing along z, the 2-D (xz) simulation shows that KAWs with large wave number kxpi - 1 are generated near the Alfv6n resonance surface, where Pi is the ion Larmor radius. Several nonlinear wave properties are manifest in the mode conversion process. Harmonics of the driver frequency are generated. As a result of nonlinear wave interaction, the mode conversion region and its spectral width are broadened. In the 3-D simulation, after this first stage of the mode conversion to KAWs with large kx, a subsequent generation of KAW modes of finite ky is observed in the later stage, through a nonlinear parametric decay process. Since the nonlinear cascade to ky can lead to massive transport at the magnetopause, the simulation results provide an effective transport mechanism at the plasma boundaries in space as well as laboratory plasmas.

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