History of the Royal Sappers and Miners, Volume 2 (of 2): From the Formation of the Corps in March 1712 to the date when its designation was changed to that of Royal EngineersConnolly, T. W. J. (Thomas William John)
History
History of the Royal Sappers and Miners, Volume 2 (of 2): From the Formation of the Corps in March 1712 to the date when its designation was changed to that of Royal Engineers
Connolly, T. W. J. (Thomas William John)
Great Britain. Army. Royal Sappers and Miners
To Unst, in Shetland, the northern extremity of the arc just mentioned,
sergeant Steel now repaired, and ascertained the existence of a
disturbance at Saxavord, but in the contrary direction. This was fully
established by taking a similar series of observations at the Gerth of
Scaw, near Lambaness, and on the small uninhabited island of Balta. The
relative position of these stations he fixed astronomically as to
latitude, and geodetically by triangulation and levelling from the mean
level of the sea, which involved observations with regard to the ebb and
flow of the tides. By the series of observations so far made, it was
clearly proved, that the latitude of a place could not be measured with
the degree of certainty formerly supposed, and that though astronomers
may profess to give seconds, tenths, and even hundredths of a second of
their latitude, yet the real truth is, that the record may often be
_several whole seconds in error_. The discovery, now confirmed by
sergeant Steel’s inflexible accuracy, is likely to produce some
interesting discussion in the scientific world, and has already been
made the subject of an article in the ‘Philosophical Journal of Science’
for April, 1853, embraced in a review of Captain Yolland’s Sector
Volume.[59]
After passing a station at Cowhythe Hill, in Banffshire, to verify the
sector operations of 1813, and which object was satisfactorily attained,
the sergeant fixed his observatory at Southampton, where, in carrying on
the duty, he made various experiments to ascertain the cause of apparent
errors. In taking the usual readings of the telescope micrometers, the
value of the zenith point, derived from each double observation of a
star, varied sensibly. To determine this more accurately, by
ascertaining the true value of the divisions of the screw, and
correcting the error involved in the reduction of the whole of the
observation, he adopted the method of making two distinct observations
of the same star without reversal of the revolving frame, in the manner
described in the Sector Volume, page xxvii, and so excellent was this
method considered, that the value of the screw thus obtained, was
finally applied to all the observations.
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