Computer Science
Scientific paper
Jul 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..382..245b&link_type=abstract
Proceedings of the eigth international solar wind conference: Solar wind eight. AIP Conference Proceedings, Volume 382, pp. 245
Computer Science
Interplanetary Magnetic Fields, Particle Emission, Solar Wind, Plasma Turbulence, Magnetohydrodynamic Waves
Scientific paper
MHD turbulence features in the solar wind are briefly reviewed. Focus is first on the evolution of fluctuations of Alfvénic type. The role of interplanetary sources and the influence of interactions with structures convected by the solar wind are discussed. Compressible fluctuations are then examined, with special attention to their nature and origin.
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