3D Hall MHD Modeling of Solar Wind Plasma Spectra - Physics > Space PhysicsReport as inadecuate




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Abstract: We present fully self consistent 3D simulations of compressible Hall MHDplasma that describe spectral features relevant to the solar wind plasma. Wefind that a $k^{-7-3}$ spectrum sets in for the fluctuations that are smallerthan ion gyro radius. We further investigate scale dependent anisotropy led bynonlinear processes relevant to the solar wind plasma. Our work is importantparticularly in understanding the role of wave and nonlinear cascades in theevolution of the solar wind, structure formation at the largest scales.



Author: Dastgeer Shaikh, G. P. Zank

Source: https://arxiv.org/







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