scholarly journals III. Action of an intermittent beam of radiant heat upon gaseous matter

1881 ◽  
Vol 31 (206-211) ◽  
pp. 307-317 ◽  

The Royal Society has already done me the honour of publishing a long series of memoirs on the interaction of radiant heat and gaseous matter. These memoirs did not escape criticism. Distinguished men, among whom the late Professor Magnus and the late Professor Buff may be more specially mentioned, examined my experiments, and arrived at results different from mine.

We have come to hear on these three days from as many members of the Expedition as we could assemble the results of their work in the Solomon Islands. We have the pleasure, also, in looking forward to contributions from six other scientists who, though not Expedition members, have independently added much to the exploration and study of the Solomons. We hope to enjoy the first occasion for a lengthy biogeographical discussion about the islands. This was the purpose of the Expedition set by its originator, the late Professor Carl Pantin, when he was chairman of the Southern Zone Research Committee. We owe to him and to the generosity of the Royal Society the grand opportunity we have had to visit those beautiful islands, to have explored them according to our predilections, and to be gathered here in such hospitality. Professor Pantin decided that the zoological side should be confined to marine and land invertebrata, being the groups most likely to assist in evaluating the geological connexions of the islands. To increase this aspect, and to test the results, we have the contribution by Professor Cain on the birds and of Dr Torben Wolff on the zoology of Rennell Island, which the Expedition was unable to visit. A geological setting has been prepared by Dr Thompson, which in his absence will be read by Dr Allum, who has himself investigated the occurrence and nature of faulting, particularly on Guadalcanal. Pantin left the botanists to decide for themselves and they have covered most groups of plant life, from the sea, where Dr Womersley and his assistant studied the seaweeds, to the totality of the land-flora excepting the microscopic algae and fungi. But we botanists have also invited Dr Thorne to inform to us on the remarkable differences between New Caledonia and the Solomons, as great as the differences between the British and Japanese floras, yet so much closer together. And we have invited Professor Good to put our findings in the general field of Melanesian and Malaysian plant-geography. Our sixth outside contribution is from Dr Brookfield on the new field of climatology in the Solomons. Regrettably, neither Dr Brookfield nor Dr Thorne is able to be with us.


1881 ◽  
Vol 172 ◽  
pp. 307-353 ◽  

1. In Vol. XX. (1872) of the Proceedings of the Royal Society (pp. 160-168) is a beautiful paper by the late Professor Clerk Maxwell giving an investigation of the induction of currents in an infinite plane sheet of uniform conductivity. For the purposes of the investigation the sheet is supposed infinitely thin; and when it is at rest and influenced by a varying external magnetic system, the effect of the currents induced in it is found to be equivalent to an infinite train of images, at the sheet, of the external system, which, after being formed, move off to infinity with uniform velocity. When the external system revolves uniformly round an axis normal to the sheet, the effect is shown to be the same as if the sheet itself revolved round the axis and the magnetic system remained fixed. The images will then lie in a spiral trail in the form of a helix whose axis is perpendicular to the sheet. This theory was afterwards reproduced in his ‘Treatise on Electricity and Magnetism,’ and the latter part proved directly from the equations. The analysis there given is somewhat difficult to follow, though it is doubtless possible to present it in a more logically exact form. The problem of the induction of currents has also been treated by Felici (Tertolini’s ‘Annali,’ 1853-54) and by Jochmann (Crelle, 1864, and Pogg. Ann., 1864). Jochmann has solved the case of a sphere which rotates uniformly in a magnetic field symmetrical about the axis of revolution and finds that no currents will be generated in it, but that there will be a certain distribution of free electricity throughout its interior and over its surface. He has also handled the case of an infinite plate of finite thickness, which revolves uniformly round a normal, by neglecting the inductive action of the currents on themselves, and shows that the conditions of the problem may then be satisfied by a system of currents parallel to the faces of the plate; he has also traced the forms of the current and equipotential lines in some simple cases. The solution, however, as Maxwell has shown in the case of a thin copper disc, can be true only for very small values of the angular velocity.


In the preliminary note on the Radio-micrometer which I had the honour to present to the Royal Society last year (1887), I promised to complete, as far as I might be able, the development of the instrument, and, in case of any great improvement in the proportions of the parts, to exhibit an instrument in the improved form. In the present paper I have shown how the best sizes of the several parts may be determined, and how the best result may be attained. I must, however, first refer to the fact that on February 5, 1886, M. d’Arsonval showed, at a meeting of the Physical Society of France, an instrument called by him the Thermo-galvanometer, with which mine is in all essential respects identical. The invention of an instrument for measuring radiant heat, in which one junction of a closed thermo-electric circuit suspended in a strong magnetic field is exposed to radiation, is due entirely to M. d’Arsonval, and I need hardly say that it was in ignorance of the fact that he had preceded me that my communication was made to the Royal Society. As soon as I became acquainted with M. d’Arsonval’s work, I took the earliest opportunity of admitting his claim to priority (see ‘Nature,’ vol. 35, p. 549).


1869 ◽  
Vol 159 ◽  
pp. 637-660 ◽  

§ 1. The passage of heat through matter has been mainly examined in reference to the diathermancy of solids, liquids, and gases to radiant heat, and to the conduction of contact-heat through solids and gases. The conduction of contact-heat through liquids forms a chapter in heat transference which has not hitherto received as much attention from experimental physicists as it merits. § 2. In the following pages I have the honor of submitting to the Royal Society certain experimental results and considerations to which I have been led during an investigation of this subject. These results are necessarily incomplete. The inquiry is fraught with very numerous and considerable experimental difficulties; but I venture to hope that such as the results are, they may be found useful to those who shall hereafter pursue the subject with greater skill and more perfect appliances.


2020 ◽  
pp. 096777202094273
Author(s):  
Michael T Tracy

The Royal Society of Edinburgh (RSE) is Scotland’s national academy of science and letters and has been in existence since the eighteenth century. On 23 November 1868, a general meeting was held by the RSE at which members nominated the German academic, Professor Rudolf Virchow, as an Honorary Fellow in recognition of his key contributions to cellular theory. This nomination was opposed by the Reverend Joseph Taylor Goodsir, brother of the late Professor of Anatomy at Edinburgh University, John Goodsir. Reverend Goodsir went on to accuse the German professor of plagiarising his late brother’s pioneering work in the formulation of cell theory. The resultant furore created by the Reverend Goodsir led to an acrimonious scientific dispute in the Edinburgh medical establishment, then one of the leading centres of medical education. The current work describes the history of cellular theory as it pertains to John Goodsir and Rudolf Virchow, discusses the history behind the scientific dispute and interprets Reverend Joseph Taylor Goodsir’s role relating his actions to his continuing battle with mental illness, and the aftermath of the dispute as it affected the reputation of John Goodsir.


1779 ◽  
Vol 69 ◽  
pp. 139-159 ◽  

Sir, Being lately informed by Dr. Poemmering, whom on account of his singular industry and talents I have recommended to your favour, that you, as well as l'Abbé Fontana and Dr. Ingenhousz, were suprized to hear from M. Febroni, the keeper of the Duke of Tuscany's Museum, that I had discovered the true organical reason for which the Orang Outang, and several other apes and monkies, are unable to speak; I take the liberty of addressing to you this anatomical essay upon the organ of speech of the Orang Outang and other monkies, in hopes you will judge it worthy to be read to the Royal Society; in whose most valuable Transactions I should be very proud to see these observations; the rather, as it is the first essay I have offered to that respectable body.


1881 ◽  
Vol 31 (206-211) ◽  
pp. 478-479 ◽  

In the concluding paragraph of the note communicated on the 10th of January to the Royal Society these words occur:—“The vapours of all compound liquids will, I doubt not, be found sonorous in the intermittent beam.” Since that time I have examined eighty different liquids, both at the ordinary temperature of the air and at their boiling temperatures, and have verified so far the prediction just quoted. In all cases I have obtained musical sounds—some feeble, some moderate, and some exceedingly strong. I have, moreover, determined by thermometric expansion the absorptions exerted by the vapours of more than twenty of these liquids, and it is my intention to subject the whole' of them to this test. The harmony and mutual support exhibited by two series of experiments, conducted in accordance with these two diverse methods, are on the whole admirable.


There are a number of references in the scientific literature to a burning mirror designed by Sir Isaac Newton (1). Together, they record that it was made from seven separate concave glasses, each about a foot in diameter, that Newton demonstrated its effects at several meetings of the Royal Society and that he presented it to the Society. Nonetheless, neither the earliest published list of instruments possessed by the Royal Society nor the most recent one mentions the burning mirror; the latest compiler does not even include it amongst those items, once owned, now lost. No reference to the instrument apparently survives in the Society’s main records. It is not listed by the author of the recent compendium on Newton’s life and work (2). There is, however, some contemporary information still extant (Appendix 1). Notes of the principles of its design and some of its effects are to be found in the Society’s Journal Book for 1704; some of the dimensions and the arrangement of the mirrors are given in a Lexicon published by John Harris which he donated to the Royal Society at the same meeting, 12 July 1704, at which Newton gave the Society the speculum. The last reference in the Journal Book is dated 15 November that year, when Mr Halley, the then secretary to the Society, was desired to draw up an account of the speculum and its effects (3). No such account appears to have been presented to the Royal Society. There is no reference in Newton’s published papers and letters of his chasing Halley to complete the task, nor is there any mention of it in the general references to Halley. The latter was, of course, quite accustomed to performing odd jobs for Newton; that same year he was to help the Opticks through the press. The only other contemporary reference to the burning mirror, though only hearsay evidence since Flamsteed was not present at the meeting, is in a letter the latter wrote to James Pound; this confirms that there were seven mirrors and that the aperture of each was near a foot in diameter (4). Because John Harris gave his Dictionary to the Royal Society in Newton’s presence, it is reasonable to assume that his description is accurate. As Newton would hardly have left an inaccurate one unchallenged, then, belatedly, the account desired of Mr Halley can be presented. In some respects, the delay is advantageous, since the subject of radiant heat and its effects, although already by Newton’s period an ancient one, is today rather better understood. On the other hand, some data has to be inferred, that could have been measured, and some assumptions made about Newton’s procedures and understanding that could have been checked (5).


1887 ◽  
Vol 4 (12) ◽  
pp. 531-540
Author(s):  
T. Sterry Hunt

The present writer in 1883 reviewed the history of the rocks of the Alps and the Apennines with especial reference to the geological relations of serpentine and its associates, in a paper which appeared in the first volume of the Transactions of the Royal Society of Canada, and is reprinted, revised and with some additions, as the tenth chapter of his volume entitled “Mineral Physiology and Physiography” (Boston, 1886). Therein he gave a somewhat detailed account of the labours in Italian geology of the late Professor Bartolomeo Gastaldi, of Turin, a list of whose publications on that subject from 1871 to 1878, so far as known to the writer, will there be found, including his letter to Quintino Sella, in 1878, on the general results of explorations made in 1877 (loc. cit., 458).


In 1882 the late Professor F. M. Balfour suggested my undertaking the study of the development of the peculiar Australian Mammalia and Ceratodus . In 1883 I decided to carry out this suggestion, and was elected to the travelling studentship founded in Balfour’s memory. The Committee of the Royal Society appointed to administer the Government Grant for the endowment of research gave me a sum of £400 for equipment.


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