ve some men still at work. The men applaud and shew their
respect very gracefully. There are present some two or three persons
who attended my former lectures, and they say that I lecture exactly
as I did formerly. One of my attendants is a man that they say cannot,
from years and infirmity and habit, be induced to go anywhere else: Dr
Archdall, the Master of Emmanuel. I find that some of my old
lecturing habits come again on me. I drink a great deal of cold water,
and am very glad to go to bed early."--From June 10th-30th he was
travelling in Scotland, and staying at Barrow House near Keswick (the
residence of Mr Langton), with his son Hubert.--Subsequently, from
Aug. 17th to 31st, he was again in the Lake District, with his
daughter Christabel, and was joined there by his son Hubert on the
24th. The first part of the time was spent at Tarn Bank, near
Carlisle, the residence of Mr Isaac Fletcher, M.P. From thence he made
several expeditions, especially to Barrow in Furness and Seascale,
where he witnessed with great interest the Bessemer process of making
steel. From Barrow House he made continual excursions among the
Cumberland mountains, which he knew so well.
1870
"In this year Mr Stone, the First Assistant, was appointed to the Cape
of Good Hope Observatory, and resigned his post of First Assistant. Mr
Christie was appointed in his place.--From the Report to the Visitors
it appears that 'A few months since we were annoyed by a failure in
the illumination of the field of view of the Transit Circle. The
reflector was cleaned, but in vain; at last it was discovered that one
of the lenses (the convex lens) of the combination which forms the
object-glass of a Reversed Telescope in the interior of the
Transit-axis, and through which all illuminating light must pass, had
become so corroded as to be almost opaque.'--The South-East Equatoreal
has been partly occupied with the thermo-multiplier employed by Mr
Stone for the measure of heat radiating from the principal stars. Mr
Stone's results for the radiation from Arcturus and alpha Lyrae appear
to be incontrovertible, and to give bases for distinct numerical
estimation of the radiant heat of these stars.--In my last Report I
alluded to a proposed systematic reduction of the meteorological
observations during the whole time of their efficient
self-registration. Having received from the Admiralty the funds
necessary for immediate operat
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