The solar wind in the third dimension

Details The solar wind in the third dimension The solar wind in the third dimension

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sowi.conf...43n&link_type=abstract

International Solar Wind 8 Conference, p. 43

Physics

Solar Wind, Solar Activity, Solar Cycles, Solar Corona, Ulysses Mission, Ecliptic, Scintillation, Remote Sensing, Three Dimensional Models

Scientific paper

For many years, solar-wind physicists have been using plasma and field data acquired near the ecliptic plane together with data on the scintillation of radio sources and remote sensing of structures in the solar corona to estimate the properties of the high-latitude solar wind, Because of the highly successful Ulysses mission, the moment of truth is now here. This talk summarizes the principal differences between the high and low latitude solar winds at the declining phase of the solar-activity cycle and between the Ulysses observations and expectations.

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