Drop an object at the solar equator and it would drift all the way to the pole in a little more than a year.
2.
In the second half of the nineteenth century Richard Carrington and Sp�rer independently noted the migration of sunspot activity towards the solar equator as the cycle progresses.
3.
The inclination of the solar equator to the plane of the ecliptic he fixed at 7?152; the longitude of the ascending node at 73?402 ( both for 1850 ).
4.
Subsequent work demonstrated a strong tendency for east-west alignment of magnetic polarities in sunspots, with mirror symmetry across the solar equator; and that the polarity in each hemisphere switched orientation from one sunspot cycle to the next.
5.
A team of scientists led by Dr . John Phillips of Los Alamos National Laboratory in New Mexico reported that near the pole the solar wind is flowing away from the Sun at about two million miles an hour, nearly twice the velocity of the wind nearer the solar equator and where the wind continuously arrives in the vicinity of Earth.
6.
For some reason, the solar " weather " in the southern polar region is more placid than in space out from the solar equator, where the more turbulent solar winds affect Earth by causing magnetic " storms " that can interrupt communications and power transmissions and produce spectacular light shows like the aurora borealis, or northern lights.
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