scholarly journals III. Magnetic observations at Kerguelen

1878 ◽  
Vol 26 (179-184) ◽  
pp. 95-102

The Government expedition to Kerguelen Island for the observation of the Transit of Venus on December 8th, 1874, presented a very favour­able opportunity for the accurate determination of the magnetic elements of an important station in the South-Indian Ocean, and one which will at most be visited only at distant intervals for the purpose of scientific investigations. When, therefore, I heard of my appointment to that station, I at once brought the question of terrestrial magnetism under the notice of the Astronomer Royal, and he readily agreed to my pro­posal of taking a complete set of magnetic instruments to Kerguelen, and of making any observations that would not interfere with the main object of our expedition. Being in charge of the whole Kerguelen party of observers, I could not expect to be able to devote much time personally to the magnetic work; but the Rev. W. Sidgreaves, whom long experience, both at the Stony-hurst Observatory and during our magnetic survey of Prance in 1868 and 1869, had made perfectly conversant with all the details both of instruments and observations connected with terrestrial magnetism, had already been placed on the staff of astronomical observers for Kerguelen. The assistance of a very efficient observer being thus secured, the next step was to procure the necessary instruments. Fortunately I experi­enced no difficulty in this matter, as the authorities at Kew immediately placed at my disposal a Jones unifilar and a Barrow dip-circle. There was no question of the want of a good chronometer, as the astronomers were to be supplied with nine of these, besides the eight reserved exclu­sively for longitude connexions, which remained always undisturbed in their quiet berth on shipboard.

In the recent magnetic surveys conducted in different countries, the details of which have been published, one point stands out prominently from the rest, that the more minute the survey, the more surely do the observations show that the needle is subject to “local” and “regional” magnetic disturbances, varying in amount from the normal values of the magnetic elements, as deduced from extended observations made over the whole country. A reference alone to that recent and most valuable contribution to terrestrial magnetism, “A Magnetic Survey of the British Isles,” by Professors A. W. Rücker, F. R. S., and T. E. Thorpe, F. R. S., is quite sufficient to show the certainty of these disturbances.


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.


1870 ◽  
Vol 160 ◽  
pp. 33-50 ◽  

The Magnetic Survey of the West of France, of which the following is a report, was undertaken by the Rev. W. Sidgreaves and myself at the request of the authorities of Stonyhurst College, who generously undertook to defray all the expenses of the expedi­tion. A similar survey of the East of France will be made during the coming autumn, so as to complete the series of observations of the magnetic elements for the whole of France. The instruments employed were those which have been in constant use at Stonyhurst Observatory for the determination of the monthly absolute values of the Dip, Declination, and Intensity. They consisted of a dip-circle by Barrow, No. 32, a unifilar by Jones, and Frodsham’s marine chronometer, No. 3148. A beautiful transit-theodolite and an aneroid barometer were kindly placed at our disposal by the late Mr. Cooke.


1877 ◽  
Vol 167 ◽  
pp. 461-508 ◽  

The paper now offered to the Society forms the XVth and last of a series of papers printed in the Philosophical Transactions, entitled “Contributions to Terrestrial Magnetism.” The whole Fifteen. Numbers are related to each other as “Contributions to the Magnetic Survey of the Globe.” Four of them (viz. XI., XIII., XIV., and the present paper) contain the complete statement of this Survey in the double form of “Catalogue” or “Tables” and of “Magnetic Maps; ” of these maps there are twelve,one for each of the three magnetic elements in each of the four papers. The present paper consists (as did its last predecessor, No. XIV.) of four zones, each 10° in breadth:— Zone 1, comprehending from the equator to 10° S. Zone 2, „ „ lat. 10° S. „ 20° S. Zone 3, „ „ lat. 20° S. „ 30° S. Zone 2, „ „ lat. 30° S. „ 40° S. In the Tables the observations are entered in each zone in the succession of their longitudes, beginning with the meridian of Greenwich. The statements in the introduction to No. XIII. regarding the different magnetic elements apply to the present paper, as they did also to the preceding paper (No. XIV.).


1867 ◽  
Vol 15 ◽  
pp. 209-209

In this number of the Contributions to Terrestrial Magnetism the author resumes the discussion of the results obtained in the Magnetic Survey of the Southern Ocean by the Expedition under Sir James Clark Ross, R. N., and Captain Francis Rawdon Crozier, R. N., between the years 1839 and 1843. The proceedings during the two first years of this Survey have been the subjects of two preceding numbers of the Contributions, viz. of Nos. V. and VI., in the Philosophical Transactions for 1843 and 1844. The present number contains a similarly detailed exposition of the operations of the third year of the Survey, comprehending the Southern Atlantic between Cape Horn and the Cape of Good Hope, and completing the circumnavigation of the southern hemisphere, from the departure of the expedition from the Cape of Good Hope in March 1840, to the return to the same station in April 1843. In a subsequent memoir, which will be presented to the Royal Society early in the ensuing Session, the author proposes to connect and thoroughly coordinate the three portions of the Survey, and to supply from them the numerical data at equidistant points on each of the three parallels of 50°, 60°, and 70° of south latitude, of the three magnetic elements, which will be required for a revision of the 'Allgemeine Theorie des Erdmagnetismus’ of M. Gauss—the 40th parallel having been the most southern available at the epoch of the publication of the original work. The instruments employed in this Survey, as well as the methods of employing them, and of eliminating the disturbing influence of the iron in the equipment of the vessels, having been in a great measure of a novel character, a discussion of considerable length bearing on all such points is prefixed to a full detail of the observations themselves, arranged in Tables, showing in every instance both the immediate results of the observations, and the corrections which have been applied in conformity with the principles contained in the preliminary discussion. Tabular abstracts are also furnished, exhibiting the results of the determinations of each day, with the appropriate geographical positions.


1877 ◽  
Vol 25 (171-178) ◽  
pp. 148-148 ◽  

The paper now offered to the Society forms the fifteenth and last of a series of papers printed in the Philosophical Transactions, entitled “Contributions to Terrestrial Magnetism.” The whole fifteen numbers are related to each other as “Contributions to the Magnetic Survey of the Globe.” Four of them, viz. XI., XIII., XIV. and the present paper, contain the complete statement of this survey in the double form of “Catalogue” or “Tables” and of “Magnetic Maps;” of these maps there are twelve, one for each of the three magnetic elements in each of the four papers. The present paper consists (as did its last predecessor, No. XIV.) of four zones, each 10° in breadth:— Zone 1, comprehending from the equator to 10° S. Zone 2, comprehending from the lat. 10° S. to 20° S. Zone 3, comprehending from the lat. 20° S. to 30° S. Zone 4, comprehending from the lat. 30° S. to 40° S. In the Tables the observations are entered in each zone in the succession of their longitudes, beginning with the meridian of Greenwich. The statements in the introduction to No. XIII. regarding the different magnetic elements apply to the present paper, as, they did also to the preceding paper, No. XIV.


1872 ◽  
Vol 20 (130-138) ◽  
pp. 443-443

The author presents this paper as the companion of No. XI. of his Contributions to Terrestrial Magnetism, which contained the Magnetic Survey of the Southern Hemisphere from 40° south latitude to the extreme limit towards the southern pole, as does the present memoir, No. XIII. of the same series, the three magnetic elements from 40° north latitude to the furthest attained limit towards the northern pole. In both papers the mean epoch is the same, viz. 1842·5. Where it has been possible to do so, corrections to this mean epoch have been obtained and applied to earlier and later observations. The determinations are derived from observers of all countries, and are arranged in zones, each of 5° of latitude, passing round the globe. The Table thus formed contains between 3000 and 4000 stations at which the magnetic elements have been determined. The observers are named, and references are made to the sources from whence their observations are taken. The paper is accompanied by maps of the resulting Isogonic, Isoclinal, and Isodynamic Lines, executed at the Hydrographic Office.


1872 ◽  
Vol 162 ◽  
pp. 7-27

This survey, which occupied a considerable portion of the months of August and September 1869, is a continuation of the series of observations made in the west of France during the preceding year. The instruments used were the same on both occasions, the only changes made for the second expedition being (1°) the substitution of a theodolite by Jones in lieu of Cooke’s transit-theodolite, which was slightly too heavy for carrying in the hand, and (2°) the procuring, through the kindness of Dr. Stewart, a second tripod stand similar to our own, which rendered the series of observations with two observers much more rapid than on the previous occasion. The observations were undertaken, as before, by the Rev. W. Sidgreaves and myself, the Vibrations and Deflections falling to his share, and the Declination and Chronometer comparisons remaining in my hands, whilst the Dip was in general observed by both. The method of reduction is almost identical with that adopted for the observations taken in the west of France. The geographical positions of the different stations have been calculated, as far as possible, from the data given in the 'Connaissance des Temps,’ but where this could not be done I have had recourse to the most reliable sources of information at my command. For the accurate determination of the positions of Mont Rolland (near Dôle), of N. D. de Myans (near Chambéry), of Mongré (near Villefranche-sur-Soane), of Iseure (near Moulins), and of our station at Marseilles I am indebted to the kindness of the Rev. N. Larcher, S. J., Membre de la Société Météorologique de France. The coordinates of Vaugirard were readily obtained from a good map of Paris, and for Issenheim and Monaco I have to depend on Cassini’s ‘Carte Générale de la France’ and on Philip’s 'Imperial Atlas.’ The Imperial Observatory at Paris is chosen as the natural position for the origin of coordinates, in lieu of our central station of observation at Vaugirard, which lies on the outskirts of the city; the resulting mean values will thus require no correction, and will be immediately comparable with those of most other observers.


This paper is the second of a series, in which the author purposes to communicate to the Royal Society the results of magnetic observations in different parts of the globe, having for their object to supply the requisite data for deducing the numerical elements corresponding to the present epoch of the general theory of terrestrial magnetism. It consists of two sections; the first comprises the observations of Captain Belcher, R. N., and the officers of H. M. S. Sulphur, at twenty-nine stations on the west coast of America, and the adjacent islands, between the latitudes of 60° 21' N. and 18° 05' S, The second contains a new determination, by the same officers, of the magnetic elements at Otaheite, made in consequence of the discrepancies in the results obtained by previous observers, and of a note in M. Gauss’s Allgemeine Theorie, in which Otaheite is spoken of as a highly important station for the future improvement of the calculations of the theory. Abstracts are given of the original observations which are deposited in the Hydrographic Office of the Admiralty, as well as a full detail of the processes of reduction by which their results have been computed. The values of the horizontal and total intensities are expressed in terms by which the results of observation are immediately comparable with the maps of MM. Gauss and Weber in the “Atlas des Erdmagnetismus.” By an investigation into the “probable error” of a single independent determination of the magnetic intensity with Hansteen’s apparatus, derived from the data furnished by Captain Belcher’s observations, the author shows the extreme improbability that the differences in the results obtained at Otaheite by Messrs. Erman, FitzRoy and Belcher, should be occasioned by instrumental or observational error. They are also far greater than can, with any degree of probability, be ascribed to periodical or accidental variations in the magnetic force from its mean value. The only known cause adequate to their explanation is what may with propriety be termed Station error ; that is, local disturbing influences, in an island composed chiefly of volcanic rocks, and where the spot of observation selected by the different observers may not have been precisely the same.


2020 ◽  
Vol 5 (5) ◽  
pp. 45-52
Author(s):  
R. P. Pavliuk ◽  

The Rhesus system is the second most important erythrocyte system for transfusion after ABO. Accurate determination of the Rhesus status of the donor, recipient, pregnant allows to prevent the development of post-transfusion hemolytic complications of the fetus or newborn associated with incompatibility of the blood of the mother and the fetus by D antigen. Generally, determination of the Rhesus affiliation of a person is performed by serological methods using anti-Rhesus reagents with full or incomplete antibodies. However, the results of serological studies are not always clear. Mutations and other effects of the RH gene locus disrupt the production of the normal D antigen and lead to the emergence of numerous varieties of antigen D. The variant of antigen D was described in 1946 and was designated as Du. The study showed that the differences between Du antigen and normal D were quantitative rather than qualitative. The Du antigen was later designated as Dweak - a weak D-antigen or a weak D-phenotype. In the early 1950s, anti-D antibodies were detected in recipients with a weak D-antigen after transfusion with Rh-positive blood and in pregnant women with the Du phenotype during pregnancy and at the birth of a D+ baby. It was suggested that the D antigen was not homogeneous and consisted of numerous partial variants: D1, D2, D3, etc. A complete set of partial variants corresponds to a complete D-antigen. The absence of any of one or more partial factors leads to the appearance of attenuated forms of the D antigen, denoted as Dpartial. People lacking certain partial antigens can produce anti-D antibodies against them. Differentiation of weak D phenotypes has great clinical importance, because transfusion of Rh-erythrocytes to recipients with Dweak and who are actually Rh-positive, has no scientific justification and leads to unjustified consumption of deficient blood and unnecessary immunoprophylaxis of anti-Rh immunoglobulin to pregnant women. International laboratory practice has no unified policy regarding the diagnosis of weak variants of D antigen and the interpretation of the results. Polymerase chain reaction allows to accurately define the Rh status of an individual and to avoid unreasonable transfusions of Rh-negative blood and unnecessary immunoprophylaxis


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