scholarly journals LXXXVI. Observations for proving the going of Mr. Ellicott's clock, at St. Helena

1761 ◽  
Vol 52 ◽  
pp. 534-539 ◽  
Keyword(s):  

In my return from the cape of Good Hope, the clock, used in the observations made there, was set going at James's sort, St. Helena, the pendulum remaining as at the Cape.

1764 ◽  
Vol 54 ◽  
pp. 348-386 ◽  

The following observations were taken with a reflecting telescope, of two feet focal length, made by Mr. Short (of a similar size and construction to those used in the observation of the transit of Venus, by himself at Saville House, by Mr. Green at Greenwich, and by Mess. Mason and Dixon at the Cape of Good Hope), with an equal altitude instrument made by Mr. Bird, and a clock, with a gridiron pendulum, made by Mr. Shelton, an account of whose going, at Greenwich, before my departure of St. Helena, and immediately upon my arrival there, is contained in Phil. Trans. Vol. LII. Part. II. Page 434. and the difference of gravity between those two places thence deduced.


In this communication the author has arranged and presented together the Annual variations which the magnetic declination undergoes at every hour of the day at the four Colonial Observatories established by the British government, at Toronto, Hobarton, the Cape of Good Hope and St. Helena. This has been done by means of a graphical representation, in which the annual variations at every hour are shown by vertical lines varying in length according to the amount of the range of the annual variation at each hour; each line having also small cross lines marking the mean positions of the several months in the annual range. The mean declination in the year at the respective hours is marked by a horizontal line which crosses all the verticals at each station. The hours are those of mean solar time at each station, the day commencing at noon.


1894 ◽  
Vol 55 (331-335) ◽  
pp. 210-217 ◽  

In a paper which was read before the Royal Society in June, 1890, I showed that the principal phenomena of terrestrial magnetism and the secular changes in its horizontal and vertical components could be explained on the assumption of an electro-dynamic substance (presumably liquid or gaseous) rotating within the crust of the earth in the plane of the ecliptic, and a little slower than the diurnal rotation. By means of some electro-mechanism, new to experimental science, which I termed a magnetarium, the period of backward rotation of the internal electro-dynamic sphere required for the secular variations of the magnetic elements on different parts of the earth’s surface was found to be 960 years, or 22.5 minutes of a degree annually. It was also demonstrated that the inclination of the axes of the electro-dynamic and terrestrial globes to each other of 20° 30', was the cause of the inequality of the declination periods about the same meridian in the northern and southern hemispheres; as instanced in the short period of outward westerly declination at London, and the long period of outward westerly declination at the Cape of Good Hope and St. Helena.


1761 ◽  
Vol 52 ◽  
pp. 21-25 ◽  

Dr. Watson lately received a letter from the Abbé De la Caille at Paris, in which he takes notice, "That although the pa- "rallax of the moon seems sufficiently well deter"mined, by the observations made in 1751, in "Europe and at the Cape of Good Hope; never- "theless, an element of this importance cannot be “too well ascertained.


My dear Sir, The Annales de Chimie et de Physique for March last contains a letter from M. De la Rive to M. Arago, in which a theory is proposed, professing to explain on physical principles the general phenomena of the diurnal variation of the magnetic declination, and, in particular, the phenomena observed at St. Helena and at the Cape of Good Hope, described in a paper communicated by me to the Royal Society in 1847, and which has been honoured with a place in the Philosophical Transactions. Although I doubt not that the inadequacy of the theory proposed by M. De la Rive for the solution of this interesting problem will be at once recognised by those who have carefully studied the facts which have become known to us by means of the exact methods of investigation adopted in the magnetic observatories of recent establishment, yet there is danger that the names of De la Rive and Arago, held in high and deserved estimation as authorities on such subjects, attached to a theory, which moreover claims reception on the ground of its accordance with “well-ascertained facts” and “with principles of physics positively established,” may operate prejudicially in checking the inquiries which may be in progress in other quarters into the causes which really occasion the phenomena in question; I have thought it desirable therefore to point out, in a very brief communication, some of the important particulars in which M. De la Rive’s theory fails to represent correctly the facts which it professes to explain, and others which appear to me to be altogether at variance with, and opposed to it.


1857 ◽  
Vol 3 ◽  
pp. 208-215
Author(s):  
Traill

The discussions which arose about four years ago on the animal reported to have been seen on 6th August 1848, by Captain M'Quhae, the officers and crew of H.M.S. Dædalus, in the Southern Atlantic, between the Cape of Good Hope and St Helena, about 300 miles off the African shore, recalled my attention to the materials I had collected respecting the vast animal cast ashore on Stronsey, one of the Orkneys, in 1808.I was not there at the time, but copies of the depositions made by those who had seen and measured it were transmitted to me by order of Malcolm Laing, Esq., the historian of Scotland, on whose property it was stranded; and I obtained other notes from several individuals resident in Orkney.


In this communication the author has arranged, in tables, the disturbances of the magnetic declination at St. Helena and the Cape of Good Hope, for the purpose of exhibiting the systematic laws by which those phenomena are regulated, which were long described as irregular variations, because they were of occasional and apparently uncertain occurrence. The frequency of the disturbances, and their amount, whether viewed separately as easterly or westerly movements, or as general abnormal variations (easterly and westerly being taken together), is shown to be dependent upon the hour of the day, the period of the year, and upon the year of observation.


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