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Anisotropic magnetohydrodynamic turbulence in a strong external magnetic field
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Montgomery, D. Turner, L. |
| Copyright Year | 1981 |
| Description | A strong external dc magnetic field introduces a basic anisotropy into incompressible magnetohydrodynamic turbulence. The modifications that this is likely to produce in the properties of the turbulence are explored for the high Reynolds number case. The conclusion is reached that the turbulent spectrum splits into two parts: an essentially two dimensional spectrum with both the velocity field and magnetic fluctuations perpendicular to the dc magnetic field, and a generally weaker and more nearly isotropic spectrum of Alfven waves. A minimal characterization of the spectral density tensors is given. Similarities to measurements from the Culham-Harwell Zeta pinch device and the UCLA Macrotor Tokamak are remarked upon, as are certain implications for the Belcher and Davis measurements of magnetohydrodynamic turbulence in the solar wind. |
| File Size | 1802201 |
| Page Count | 30 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19810013385 |
| Archival Resource Key | ark:/13960/t2j728f32 |
| Language | English |
| Publisher Date | 1981-01-01 |
| Access Restriction | Open |
| Subject Keyword | Plasma Physics Magnetic Flux Tensors Fourier Transformation Magnetohydrodynamic Turbulence Magnetohydrodynamic Waves Energy Spectra Anisotropy Reynolds Number Tokamak Devices Magnetic Fields Solar Wind Zeta Pinch Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Technical Report |