Spectral Anisotropy in 2D plus Slab Magnetohydrodynamic Turbulence in the Solar Wind and Upper Corona

The 2D + slab superposition model of solar wind turbulence has its theoretical foundations in nearly incompressible magnetohydrodynamics (NI MHD) in the plasma beta ∼1 or

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Bibliographic Details
Published in:The Astrophysical journal 2020-09, Vol.900 (2), p.115
Main Authors: Zank, G. P., Nakanotani, M., Zhao, L.-L., Adhikari, L., Telloni, D.
Format: Article
Language:English
Subjects:
Anisotropy
Astrophysics
Computational fluid dynamics
Corona
Fluid flow
Interplanetary turbulence
Magnetic fields
Magnetism
Magnetohydrodynamic turbulence
Magnetohydrodynamics
Power spectra
Solar wind
Solar wind flow
Solar wind turbulence
Spectral analysis
Spectrum analysis
Theoretical analysis
Turbulence measurements
Two dimensional models
Wavelengths
Wind flow
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Description
Summary:The 2D + slab superposition model of solar wind turbulence has its theoretical foundations in nearly incompressible magnetohydrodynamics (NI MHD) in the plasma beta ∼1 or
ISSN:0004-637X
1538-4357
DOI:10.3847/1538-4357/abad30