hat Trinity College was
selected: he rode with me to Rev. Mr Rogers of Sproughton for
introductory examination; he introduced me to Rev. C. Musgrave
(subsequently of Halifax), accidentally doing duty at Grundisburgh,
who then introduced me to Sedgwick, Peacock, and T. Musgrave
(subsequently of York). In 1825, when I spent the summer at Keswick,
he introduced me to Southey and Wordsworth.
Mr Clarkson lived about thirty years at Playford Hall, and died there,
and lies interred with his wife, son, and grandson, in Playford
churchyard. I joined several friends in erecting a granite obelisk to
his memory in the same churchyard. His family is extinct: but a
daughter of his brother is living, first married to T. Clarkson's son,
and now Mrs Dickinson, of the Rectory, Wolferton.
I am, my dear Sir,
Very faithfully yours,
G.B. AIRY.
_The Very Reverend,
The Dean of Ely._
1880
"The Admiralty, on final consideration of the estimates, decided not
to proceed with the erection of a new Library near the Magnetic
Observatory in the present year. In the mean time the space has been
cleared for the erection of a building 50 by 20 feet.--I have removed
the Electrometer Mast (a source of some expense and some danger), the
perfect success of Sir William Thomson's Electrometer rendering all
further apparatus for the same purpose unnecessary.--Many years ago a
double-image micrometer, in which the images were formed by the double
refraction of a sphere of quartz, was prepared by Mr Dollond for
Capt. Smyth, R.N. Adopting the same principle on a larger scale, I
have had constructed by Mr Hilger a micrometer with double refraction
of a sphere of Iceland spar. Marks have been prepared for examination
of the scale, but I have not yet had opportunity of trying it.--The
spectroscopic determination of Star-motions has been steadily
pursued. The stars are taken from a working list of 150 stars, which
may eventually be extended to include all stars down to the fourth
magnitude, and it is expected that in the course of time the motions
of about 300 stars may be spectroscopically determined.--A new
pressure-plate with springs has been applied by Mr Browning to Osler's
Anemometer, and it is proposed to make such modification as will give
a scale extending to 50 lbs. pressure on the square foot. Other parts
of the instrument have also been renewed.--As regards the reduction of
th
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