Sep 1878
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1878natur..18..487s&link_type=abstract
Nature, Volume 18, Issue 462, pp. 487 (1878).
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Scientific paper
WHEN Broun and Hornstein detected the existence of a terrestrial magnetic inequality, of which the period is nearly that of the sun's rotation, it was natural to regard this inequality as a direct result of the rotation of our luminary. Nevertheless, there are grave reasons against this hypothesis. In the first place, it is extremely difficult to imagine the sun to be one-sided in its magnetic influence. From what we know of our luminary, it must in a great measure be composed of gaseous matter, of which the outer layers are in violent motion, so that we can hardly imagine one meridian to be permanently different from another.
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