A possible cause of anisotropy of proton and helium ion temperatures in the solar wind plasma

Computer Science

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Helium Ions, Ion Temperature, Plasma Temperature, Solar Protons, Solar Wind, Anisotropy, Approximation, Particle Diffusion, Particle Motion, Plasma Spectra, Plasma Turbulence, Positive Ions, Solar Magnetic Field

Scientific paper

The paper solves the self-consistent problem of the low frequency wave spectrum and spectra of random velocities of positive ions of multicomponent plasma of solar wind in a quasilinear approximation with an assumption that the magnetic field is approximately equal to the inverse square of radial distance. The magnitude of expected anisotropy of temperatures of separate components of the plasma was defined.

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