Properties of the solar wind

Details Properties of the solar wind Properties of the solar wind

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993adspr..13...49v&link_type=abstract

Advances in Space Research, Volume 13, Issue 9, p. 49-58.

Physics

3

Scientific paper

Solar wind observations reveal a wealth of variations in physical properties on a wide range of temporal and spatial scales. While the largest spatial scales are dominated by the average radial expansion of the plasma and the magnetic sector structure, significant amounts of energy are present also in the so called mesoscale fluctuations between several hours and one minute, which may be interpreted as examples of MHD turbulence. This paper attempts to summarize, from an observational and theoretical point of view, our present knowledge of the dynamical interactions between solar wind structures at the different scales.

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