Energetic Particle Transport in Regions of Enhanced Compressive Wave Turbulence

Details Energetic Particle Transport in Regions of Enhanced Compressive Wave Turbulence Energetic Particle Transport in Regions of Enhanced Compressive Wave Turbulence

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..719..341l&link_type=abstract

PHYSICS OF THE OUTER HELIOSPHERE. AIP Conference Proceedings, Volume 719, pp. 341-346 (2004).

Physics

Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

The nature of energetic particle transport needs to be reinvestigated during times of high solar activity when systems of closely spaced fast transient solar wind streams form large regions with strong compressive fluctuations in the solar wind. A nonlinear theory is presented for diffusive energetic particle transport in enhanced mesoscale compressive wave turbulence on which incompressible small-scale MHD turbulence is superposed. The theory suggests that suprathermal ions such as pickup ions would develop hard power law spectra inside a system of transient flows during solar maximum conditions in the inner heliosphere.

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