Density fluctuation spectra in magnetohydrodynamic turbulence

Physics

Scientific paper

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124

Density Distribution, Interstellar Matter, Magnetohydrodynamic Turbulence, Solar Wind, Incompressible Fluids, Kinetic Energy, Magnetic Flux

Scientific paper

It is shown that within the framework of nearly incompressible magnetohydrodynamics, but not within that of neutral-fluid hydrodynamics, a k-5/3 inertial-range wave number density fluctuation spectrum is to be expected at the same times that k-5/3 kinetic energy and magnetic energy cascade spectra are present. A previous discrepancy between theory and observation in the local interstellar medium and solar wind is thereby resolved.

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