MHD Turbulence in the Solar Wind as Observed at Low and High Heliographic Latitude

Details MHD Turbulence in the Solar Wind as Observed at Low and High Heliographic Latitude MHD Turbulence in the Solar Wind as Observed at Low and High Heliographic Latitude

Nov 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aps..dpp.bm101b&link_type=abstract

American Physical Society, 41st Annual Meeting of the Division of Plasma Physics, November 15-19, 1999 Seattle, WA, abstract #BM

Physics

Plasma Physics

Scientific paper

Within the past three decades there has been a large production of theoretical and observational papers which shed some light on the main mechanisms governing the generation and subsequent evolution of solar wind MHD turbulence. In-situ observations recorded in the past by several spacecraft on the ecliptic and, much more recently, by Ulysses out of the ecliptic are of particular interest. As a matter of fact, although these different space programs operated at different epochs, they do provide a consistent three dimensional view of the phenomenology characterizing the heliospheric MHD turbulence. This work intends to summarize the main conclusions reached so far.

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