Statistical properties of the solar wind

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

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sowi.confr..90r&link_type=abstract

NASA Ames Research Center, International Solar Wind 8 Conference, p. 90

Astronomy and Astrophysics

Astronomy

Satellite Observation, Solar Cycles, Solar Wind, Statistical Analysis, Astronomical Observatories, Heliosphere, Solar Activity, Solar Wind Velocity, Solar Temperature, Density (Mass/Volume), Statistical Distributions

Scientific paper

We now have spacecraft observations spanning more than a complete 22-year solar cycle. PVO at Venus, IMP 8 at Earth, and Voyager 2 and Pioneers 10 and 11 in the outer heliosphere provide many years of data from locations scattered through the heliosphere. These large data sets enable us to look at the solar wind velocity, density, temperature and flow angles on a statistical basis. Comparison of results at the different locations will provide information on the evolution of the solar wind with radial distance and variation with latitude.

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