Abstract
The observed difference in electron density between the equatorial plane and the polar direction is compared for three empirical distributions: the Allen distribution, the Saito distribution, and the Saito-Munro-Jackson distribution. It is shown that from 1.5R o to 5R o the observed difference in electron density is sufficient to result in a global azimuthal electric current flow around the sun. The dependence of the calculated current density on the radial distance and solar latitude is discussed.
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