The Life of Sir Rowland Hill and the History of Penny Postage, Vol. 1 (of 2)Hill, Rowland, Sir
History
The Life of Sir Rowland Hill and the History of Penny Postage, Vol. 1 (of 2)
Hill, Rowland, Sir
Hill, Rowland, Sir, 1795-1879; Postal service -- Great Britain -- Rates
“‘By my operations I make the distance to be 48,362 feet,
differing by only seven feet in upwards of nine miles. The
distance of Wednesbury spire from the station at Bar beacon
is, according to Colonel Mudge, 25,140 feet. This, reduced
to the distance from the flagstaff, is 25,098 feet. I have
found the same line to measure 25,102 feet, differing by
only four feet in nearly five miles.[43]
* * * * *
“‘Besides measuring these distances, I reduced the latitude
and longitude of St. Philip’s church, and of the station on
this house [my father’s], from the latitude and longitude
of Bar beacon as given by Colonel Mudge.’[44]
“One other line measured in the course of my operations (I
think it was the one from the station on Bar beacon to that
on Clent Hill near Hagley) was of yet greater length than
those mentioned above, being no less than fourteen miles.
Indeed, the triangles became so large that I had to make
allowance for spherical excess, the rotundity of the earth
becoming otherwise a source of error.
“Whenever it was practicable I measured all three angles
of each triangle; and, after allowance for the spherical
excess, there was no instance, I believe, in which the sum
of the three angles differed from 180° by so much as half a
minute.
“Those possessed of such instruments as are used at the
present day will perhaps smile at the self-satisfaction
with which I regarded this approximate accuracy; but they
must remember that I had only a common theodolite, such as
was in use fifty years ago.
“It may be mentioned here that, on account of the length of
the lines, communication between our stations was a matter
of some difficulty and much interest. When two divisions of
the surveying class had to set out in different directions
for places many miles apart, for the purpose of acting
in concert with each other, of course a certain amount
of forethought and injunction before starting, and sharp
watchfulness on the spot, were indispensable: spare flags
were carried for telegraphic purposes, and telescopes
for observation of the signals previously agreed upon. I
need not say that each signal at one station was eagerly
welcomed at the other, and that its repetition, given by
way of acknowledgment at the latter, was no less warmly
hailed at the former.
Public-domain text, read in full here on John Shaqi.
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