MHD structures, waves and turbulence in the solar wind: Observations and theories

Details MHD structures, waves and turbulence in the solar wind: Observations and theories MHD structures, waves and turbulence in the solar wind: Observations and theories

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ssrv...73....1t&link_type=abstract

Space Science Reviews (ISSN 0038-6308), vol. 73, no. 1-2, p. 1-210

Computer Science

335

Heliosphere, Magnetohydrodynamic Turbulence, Magnetohydrodynamic Waves, Solar Wind, Turbulence Models, Flow Stability, Kinetic Energy, Magnetic Fields, Periodic Variations, Statistical Distributions, Transfer Functions

Scientific paper

A comprehensive overview is presented of recent observational and theoretical results on solar wind structures and fluctuations and magnetohydrodynamic waves and turbulence, with preference given to phenomena in the inner heliosphere. Emphasis is placed on the progress made in the past decade in the understanding of the nature and origin of especially small-scale, compressible and incompressible fluctuations. Turbulence models to describe the spatial transport and spectral transfer of the fluctuations in the inner heliosphere are discussed, and results from direct numerical simulations are dealt with. Intermittency of solar wind fluctuations and their statistical distributions are briefly investigated. Studies of the heating and acceleration effects of the turbulence on the background wind are critically surveyed. Finally, open questions concering the origin, nature and evolution of the fluctuations are listed, and possible avenues and perspectives for future research are outlined.

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