II. Contributions to terrestrial magnetism. — No. III

1842 ◽  
Vol 132 ◽  
pp. 9-41 ◽  

In the present number of these Contributions, I propose to give an account of the observations on the magnetic intensity made at sea by the officers of Her Majesty’s ships Erebus and Terror, on their passage from England to Kerguelen Island, the unreduced observations, transmitted to the Admiralty by the Commanders, Captains Ross and Crozier, having been placed in my hands for that purpose. They will be divided for convenience into two sections, viz. 5. Observations between England and the Cape of Good Hope . 6. Observations between the Cape of Good Hope and Kerguelen Island . 5. Observations between England and the Cape of Good Hope . The observations in the Erebus were made by the statical method devised by Mr. Fox, with one of his instruments of 7½ inches diameter. The intensities were measured by the angles of deflection produced, in different localities, by a constant weight applied to a grooved wheel on the axle of the needle; and the ratio of the intensities is inversely as the sines of the angles of deflection, subject to a correction for differences of temperature of the needle, computed by the formula ⋅00016 I' ( t ' — t ), in which t is the standard and t ' the observed temperature in degrees of Fahrenheit, ⋅00016 a coefficient determined experimentally by Mr. Fox, and I' the observed intensity. At sea, where the manipulation of the weights causes an exposure of the needle, which, in bad weather particularly, is liable to occasion injury, the plan recommended by Mr. Fox, of using deflecting magnets instead of weights, was frequently resorted to. In this case the ratio of the intensity in different localities is inversely as the sines of the angles of deflection, and directly as the weights equivalent to the deflecting force of the deflector on the needle at the respective angles; or I' = I. w' / w ⋅ sin v /sin v' where I, v , and w are the intensity, angle of deflection, and equivalent weight at a base station; and I', v' and w' corresponding values at another station. A table is usually formed for each instrument experimentally, under Mr. Fox’s own direction, of the equivalent, or as they are termed by him, the coercing weights, for each deflector on each of the needles at the different angles which are likely to occur in the course of the observations. This is done by placing the deflector successively at angles from the dip, each differing one degree from the preceding; the needle is thereby deflected to a smaller angle on the side of the dip opposite to the deflector, and is brought back to the dip by a weight applied to the grooved wheel on the axle; this weight is called the coercing weight corresponding to the angle from the dip at which the deflector was placed. For greater accuracy, the table is formed from results obtained by placing the deflector successively on either side of the needle. Owing to accidental circumstances, no table of this description was prepared for this instrument before the Expedition sailed; the pressure of other duties prevented its being done at St. Helena, the Cape of Good Hope, or at Kerguelen Island; and at Van Diemen Island the end of the axle of the needle being accidentally broken, the needle was returned to England to be repaired, and was thus separated from the instrument and from the deflectors. Under these circumstances we have no other resource for reducing the observations made with the deflectors, than to form a table from the observations of the weights and deflectors (when both methods have been employed at the same station), which shall answer the same purpose as a table of coercing weights. Fortunately the number of such stations is considerable.

1878 ◽  
Vol 27 (185-189) ◽  
pp. 1-11 ◽  

In a previous paper, on the elements of terrestrial magnetism observed at Kerguelen, the reason is mentioned why it was not deemed advisable to take magnetic observations at sea during the voyage; the results, therefore, in this paper are entirely confined to the determina­tions of the Dip, Intensity, and Declination of the earth’s magnetic force at the several places at which we landed. On our outward journey we had no opportunity of using our instruments, except at the Cape of Good Hope, but on our return we were much more fortunate, as H.M.S. “Volage” made a stay of at least two days at Point de Galle, at Bombay, Aden, Port Said, and Malta, and we utilised all these opportunities except the first. From Malta, the Rev. W. Sidgreaves and myself returned to England by Sicily, Italy, and France, and, taking our magnetic instruments with us, we were able to observe at Palermo, Naples, Rome, Florence, and Moncalieri. As we had previously made a complete survey of France in 1868 and 1869, we thought it too early to repeat the observations. The instrumental corrections and constants have already been given in the former paper on Kerguelen, it will, therefore, suffice to refer to that communication for any necessary details. The long sea voyage, with its great variation ,of temperature, was very trying for the delicate portions of the instruments, and as we found that No. 1 Needle had been slightly injured by rust, it was never used during our home journey. In the last column of Table II the daily mean values of the dip are entered, but it was only at Cape Town and at Bombay that observations could be taken on more than a single day. Needle No. 2 seems to read about 30” higher than No. 3, but no correction has been applied to either, as the amount is considerably less than the usual errors of observations.


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.


1879 ◽  
Vol 168 ◽  
pp. 193-199 ◽  

Owing to the absence of any published accounts of the Polyzoa collected at Kerguelen Island by the Challenger, the American Transit of Venus, and the German Surveying and Transit of Venus Expeditions in 1874-75, the subjoined list treats exclusively of Mr. Eaton’s collection. The 26 or 27 species comprised in it are all of them inhabitants of the littoral or Laminarian zone, and were obtained with the grapple in Swain’s Bay and Observatory Bay. Of the whole number 17 or 18 belong to the suborder Cheilostomata , 9 to the Cyclostomata . No representative of the Ctenostomata was collected. The collection affords nine or ten forms previously undescribed; the remainder belong to a fauna which ranges from the southern extremity of S. America (which may be regarded as its “centre”) to New Zealand in a westerly direction, one or two species extending even farther, to Australia and the Cape of Good Hope. It is observable that no Arctic form has been brought from Kerguelen Island, although some have been met with further south, two instances of the occurrence of the Arctic Horneva lichenoides obtained during the voyage of H. M. SS. “Erebus” and “Terror” having been communicated to me by Sir J. Hooker. Mr. Eaton suspects their absence may be attributed to the shallowness of the areas searched by him, the greatest depth being not more than 10 fathoms.


1866 ◽  
Vol 156 ◽  
pp. 453-543

Resume in this Number of the Contributions the discussion and coordination of the observations of the Antarctic Magnetic Survey executed by Her Majesty’s Ships ‘Erebus’ and ‘Terror,’ under the direction of Sir James Clark Ross, R. N., aided by Captain Francis Rawdon Crozier, R. N., between the years 1839 and 1843. I purpose in the present communication to complete the detailed exposition of the Survey by the reduction of the observations of the three magnetic elements in its con­cluding year, on the same general plan on which similar accounts were given of those of the preceding years in earlier communications, viz., between the Cape of Good Hope and Hobarton in 1840, and between the departure from Hobarton in November 1840, and the return to the same station in April 1841, in No. V. (Philosophical Transactions, 1843, Art. X ) ; and between Hobarton in July 1841 and the Falkland Islands in April 1842 in No. VI. (Philosophical Transactions, 1844, Art. VII.). The observations discussed in the present memoir are those made from the departure from the Falkland Islands in September 1842 to the second arrival at the Cape of Good Hope in April 1843. In a subsequent and concluding memoir, which I hope to present to the Society early in the ensuing session, it will be my endeavour to connect and thoroughly coordinate the several portions of the Survey, comprising in its three portions the circumnavigation of the Southern Ocean from the departure from the Cape of Good Hope in March 1840, to the return of the ships to the same station in April 1843.


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. 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.


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