Nature of the density-magnetic-field-intensity correlation observed in the solar wind

Details Nature of the density-magnetic-field-intensity correlation observed in the solar wind Nature of the density-magnetic-field-intensity correlation observed in the solar wind

Sep 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997phrve..56.3508m&link_type=abstract

Physical Review E (Statistical Physics, Plasmas, Fluids, and Related Interdisciplinary Topics), Volume 56, Issue 3, September 19

Physics

7

Plasma Dynamics And Flow, Magnetohydrodynamic And Fluid Equation, Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

A numerical model is set up to explain the observed behavior of the compressive fluctuations close to the heliospheric current sheet. The model assumes that large-amplitude Alfvén waves from the Sun enter the current sheet region producing a nonequilibrium state that evolves, giving rise to compressive fluctuations. The characteristics of the compressive fluctuations observed in our simulations reproduce in a detailed way how the correlation between the density and magnetic-field intensity depends on the fluctuation frequency, position with respect to the current sheet, and local β value in solar wind data.

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