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
His experiments were begun towards the end of May, 1882, and by
September 28 he had obtained a fair earnest of success. The exclusion of
all other qualities of light save that with which he desired to operate,
was accomplished by using chloride of silver as his sensitive material,
that substance being chemically inert to all other but those precise
rays in which the corona has the advantage.[544] Plates thus sensitised
received impressions which it was hardly possible to regard as spurious.
"Not only the general features," Captain Abney affirmed,[545] "are the
same, but details, such as rifts and streamers, have the same position
and form." It was found, moreover, that the corona photographed during
the total eclipse of May 6, 1883, was intermediate in shape between the
coronas photographed by Sir William Huggins before and after that event,
each picture taking its proper place in a series of progressive
modifications highly interesting in themselves, and full of promise for
the value of the method employed to record them.[546] But experiments on
the subject were singularly interrupted. The volcanic explosion in the
Straits of Sunda in August, 1883, brought to astronomers a peculiarly
unwelcome addition to their difficulties. The magnificent sunglows due
to the diffractive effects on light of the vapours and fine dust flung
in vast volumes into the air, and rapidly diffused all round the globe,
betokened an atmospheric condition of all others the most prejudicial to
delicate researches in the solar vicinity. The filmy coronal forms,
accordingly, which had been hopefully traced on the Tulse Hill plates
ceased to appear there; nor were any substantially better results
obtained by Mr. C. Ray Woods, in the purer air either of the Riffel or
the Cape of Good Hope, during the three ensuing years. Moreover,
attempts to obtain coronal photographs during the partial phases of the
eclipse of August 29, 1886, completely failed. No part of the lunar
globe became visible in relief against circumfluous solar radiance on
any of the plates exposed at Grenada; and what vestiges of "structure"
there were, came out almost better _upon_ the moon than _beside_ her,
thus stamping themselves at once as of atmospheric origin.
That the effect sought is a perfectly possible one is proved by the
distinct appearance of the moon projected on the corona, in photographs
of the partially eclipsed sun in 1858, 1889, and 1890, and very notably
in 1898 and 1900.[547]
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