期刊
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
卷 118, 期 6, 页码 2824-2833出版社
AMER GEOPHYSICAL UNION
DOI: 10.1002/jgra.50365
关键词
whistler fluctuations; plasma turbulence; particle-in-cell simulations
资金
- National Aeronautics and Space Administration [NNX12AJ96G]
- DOE/National Science Foundation
- National Science Foundation [AGS-1202603]
- Directorate For Geosciences
- Div Atmospheric & Geospace Sciences [1202603] Funding Source: National Science Foundation
Three-dimensional particle-in-cell (PIC) simulations of whistler turbulence at three different initial values of (e) are carried out on a collisionless, homogeneous, magnetized plasma model. The simulations begin with an initial ensemble of relatively long-wavelength whistler modes and follow the temporal evolution of the fluctuations as wave-wave interactions lead to a forward cascade into a broadband, turbulent spectrum at shorter wavelengths with a wave vector anisotropy in the sense of k>k(vertical bar). Here and vertical bar denote directions perpendicular and parallel to the background magnetic field, respectively. In addition, wave-particle interactions lead to fluctuating field dissipation and electron heating with a temperature anisotropy in the sense of T-vertical bar>T. At early times, the wave-wave cascade dominates energy transport, whereas wave-particle Landau damping dominates at late simulation times. Larger values of (e) correspond to a faster forward cascade in wave number and to a faster rate of electron heating, as well as to a less anisotropic wave vector distribution and to a less anisotropic electron velocity distribution.
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