Statistical properties of the solar wind

Details Statistical properties of the solar wind Statistical properties of the solar wind

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..382..483r&link_type=abstract

Proceedings of the eigth international solar wind conference: Solar wind eight. AIP Conference Proceedings, Volume 382, pp. 483

Physics

4

Particle Emission, Solar Wind

Scientific paper

This paper presents some new and some updated data on the variation of the solar wind with solar cycle and distance from the Sun. The dynamic pressure of the solar wind is a minimum at solar maximum, the same time the standard deviation in pressure is a maximum, so the crossing of the termination shock is most likely at the next solar maximum in 2001. The degree of correlation between plasma parameters maximizes at solar minimum, possibly because stream interactions are a minimum then. The standard deviations of the radial velocity decrease rapidly out to 20 AU, then flatten out. Standard deviations of the density and temperature decrease with distance less steeply than those of the speed.

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