A Popular History of Astronomy During the Nineteenth Century: Fourth EditionClerke, Agnes M. (Agnes Mary)
History
A Popular History of Astronomy During the Nineteenth Century: Fourth Edition
Clerke, Agnes M. (Agnes Mary)
Astronomy -- History -- 19th century
Here then, at least, the sun was--in Professor Balfour Stewart's
phrase--"taken in the act"[477] of stirring up terrestrial commotions.
Nor have instances since been wanting of an indubitable connection
between outbreaks of individual spots and magnetic disturbances. Four
such were registered in 1882; and symptoms of the same kind, including
the beautiful "Rose Aurora," marked the progress across the sun of the
enormous spot-group of February, 1892--the largest ever recorded at
Greenwich. This extraordinary formation, which covered about 1/300 of
the sun's disc, survived through five complete rotations.[478] It was
remarkable for a persistent drift in latitude, its place altering
progressively from 17° to 30° south of the solar equator.
Again, the central passage of an enormous spot on September 9, 1898,
synchronised with a sharp magnetic disturbance and brilliant
aurora;[479] and the coincidence was substantially repeated in March,
1899,[480] when it was emphasised by the prevalent cosmic calm. The
theory of the connection is indeed far from clear. Lord Kelvin, in
1892,[481] pronounced against the possibility of any direct magnetic
action by the sun upon the earth, on the ground of its involving an
extravagant output of energy; but the fact is unquestionable that--in
Professor Bigelow's words--"abnormal agitations affect the sun and the
earth as a whole and at the same time."[482]
The nearer approach to the event of September 1, 1859, was
photographically observed by Professor George E. Hale at Chicago, July
15, 1892.[483] An active spot in the southern hemisphere was the scene
of this curiously sudden manifestation. During an interval of 12m.
between two successive exposures, a bridge of dazzling light was found
to have spanned the boundary-line dividing the twin-nuclei of the spot;
and these, after another 27m., were themselves almost obliterated by an
overflow of far-spreading brilliancy. Yet two hours later, no trace of
the outburst remained, the spot and its attendant faculæ remaining just
as they had been previously to its occurrence. Unlike that seen by
Carrington, it was accompanied by no exceptional magnetic phenomena,
although a "storm" set in next day.[484] Possibly a terrestrial analogue
to the former might be discovered in the "auroral beam" which traversed
the heavens during a vivid display of polar lights, November 17, 1882,
and shared, there is every reason to believe, their electrical origin
and character.[485]
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