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NASA NTRS · 20210001217

The Solar Wind in the Third Dimension

Neugebauer, Marcia
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Abstract

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 Ulysses observations and expectations.

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Neugebauer, Marcia. 1995-06-01. The Solar Wind in the Third Dimension. https://ntrs.nasa.gov/citations/20210001217

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