scholarly journals IX. The araucarieæ, recent and extinct

"The Coniferæ undoubtedly constitute one of the most interesting families in the vegetable kingdom, whether considered in connection with the former vegetation of the earth or in reference to their peculiarities of structure.” These introductory words to a memoir by David Don, published in 1841, are applicable with equal force to the Arauearieæ and afford a fitting preface to the present communication.

The present communication records the final stages of an investigation, of a somewhat exhaustive character, into the various problems which were presented by the necessity for constructing a magnetic shield suitable for large spaces, and capable of giving such a degree of shielding that the internal field caused by the earth should not exceed the order of magnitude 10 -3 C. G. S. unit. The theoretical calculation of the best form of shield, and the details of its construction, were given, together with an examination of the various methods of testing the efficiencies of large shields, in the first paper. A study of the effect of leakage through small air spaces was made at the same time, and it became apparent that not only this problem, but several others which are vital to the production of the theoretical efficiency of a shield, needed a more careful study than they had received hitherto. The usual process adopted for removing permanent magnetism from a shell or set of shells, by the reversals of a slowly decreasing current, ceases to be efficient when the magnetisation is very small, unless special methods are introduced, and there was previously no definite indication of the degree of accuracy with which the magnetic induction at any point due to a coil, wound in a helix on one member of a set of spherical shells, could be either predicted or measured. A study of these problems was made, and the results described in a second paper.


The value of the magnetic force at a point on the earth's surface, due to a simple oscillator placed on the surface with its axis normal to the surface, has been recently calculated by Love for a wave-length of 5 kilom. at certain distances from the oscillator. His results for the case of perfect conduction are the same as the corresponding series when the surface of the earth is supposed to be imperfectly conducting, The object of the present communication is to obtain the general formula for the case of imperfect conduction. Let r, θ, ϕ be the polar co-ordinates of a point, where r is its distance from the centre of the earth, θ its angular distance from the oscillator, E r , E θ , E ϕ the components of the electric force, and α, β, γ , the corresponding components of the magnetic force. Then, Since there is symmetry round the axis of the oscillator, α =0, β =0, γ =0; and throughout space outside the surface


1885 ◽  
Vol 2 (3) ◽  
pp. 129-131
Author(s):  
Herbert Goss

Up to December last the most ancient fossil insects known were the six fragments of Neuroptera, obtained by Mr. C. F. Hartt, from the Devonian rocks of New Brunswick, which were described by Mr. Scudder in Vol. V. of this Magazine. Although these six fossils were the oldest known insects, it seemed unlikely that they, or even the families or genera to which they belonged, were the most ancient representatives of their class. The first appearance of insects on the Earth was probably contemporaneous with that of land plants, and as remains of this division of the Vegetable Kingdom had been discovered in Silurian rocks, it seemed not unreasonable to assume that insects might have existed at an earlier period than the Devonian. The recent discovery of the wing of a cockroach in rocks of Silurian age at Jurques, Calvados, France, no longer leaves the question of the occurrence of insects at an earlier period than the Devonian a matter of speculation.


1892 ◽  
Vol 36 (2) ◽  
pp. 563-583 ◽  
Author(s):  
Frank E. Beddard

The worms which form the subject of the present communication were forwarded to me, in a living condition, from Kew Gardens.I have received lately a considerable number of living Oligochæta from those Gardens, through the kindness of Mr Dyer, who permitted me to have the earth arriving from different parts of the world in the Wardian cases, in which plants are packed for travelling, thoroughly sifted, with a view to preserving the worms which had been accidentally included. By these means I have succeeded in obtaining some very interesting new forms, as well as a number of others which are still imperfectly known. The species which I describe in the present paper appears to be a new species of Eisen's genus Ocnerodrilus. The genus Ocnerodrilus was formed by Eisen in 1878 [1] for a small worm found in Fresno County, California. The specimens were all met with in “an irrigation box,” where they were found crawling among the algæ which covered the boards. It is evidently, therefore, aquatic in its habits, but Eisen contrasts its slow movements with the rapid swimming of Lumbriculus and Rhynchelmis, comparing it in general appearance with a small species of Lumbricus.


1920 ◽  
Vol 39 ◽  
pp. 157-208 ◽  
Author(s):  
C. G. Knott

This paper is a continuation of two papers on Seismic Radiations published in the Proceedings of the Royal Society of Edinburgh, vol. xxviii, pp. 217–230 (1907–8) and vol. xxx, pp. 23–37 (1909). The object of the present communication is to place on record a new determination of the laws of propagation of seismic waves based upon a method of calculation in which no assumptions are made as to the functional relation between velocity of propagation and distance from the earth's centre. References to the work of others will be given incidentally as occasion arises.


1864 ◽  
Vol 13 ◽  
pp. 312-312

The results presented in the author’s paper, entitled “ On the Simul­taneous Distribution of Heat throughout the superficial parts of the Earth" , are confirmed and extended in the present communication.


MAUSAM ◽  
2021 ◽  
Vol 62 (4) ◽  
pp. 577-584
Author(s):  
S.L. JAIN

The ozone in the stratosphere is of great importance for very survival of life on the mother planet the Earth. Ozone acts as an umbrella and protects us from the harmful ultraviolet radiations coming from the Sun. The catalytic destruction of ozone by ClOx & NOx in general and ozone hole phenomenon over Antarctica during spring time in particular has generated unprecedented interest in monitoring of ozone and other trace constituents in the atmosphere. The satellites have proved to be an important tool to monitor the global ozone column on regular basis. The ozone data using various satellite platforms has been analyzed for the ozone hole studies over north and south poles. Also Ozone measurements were carried out at Maitri, Antarctica. The satellite data indicates that some recovery of ozone hole as a result of international efforts in reduction of use of CFCs which are the main culprit for ozone hole. However, it will be too early to conclude about ozone hole recovery. In the present communication current status of ozone hole will be discussed in detail.


1948 ◽  
Vol 63 (2) ◽  
pp. 149-162
Author(s):  
R. S. Barclay ◽  
W. O. Kermack

It is common knowledge that during the period 1875–1939 a very drastic fall in fertility occurred in most of the civilised countries throughout the world. This fall was particularly marked in Germany and some of the countries of North-western Europe, such as Norway, Sweden, England, Scotland, etc. The causes which have produced such important changes in the rates of reproduction in these communities are doubtless complex, and are difficult to investigate directly. It is therefore all the more important that our knowledge of the actual course of events should be as complete as possible. A major social change, such as this fall in fertility over large and important regions of the earth, can be fruitfully studied from many points of view. The present communication concentrates on one particular aspect, namely the influence of different types of geographical regions with their various social environments, and confines itself to the experiences of Scotland.


1860 ◽  
Vol 10 ◽  
pp. 648-650

This communication completes the series of the author’s papers on the subject of the Indian Arc. He commences by recapitulating the chief results of his former calculations, and adverting to the attempt which he made in his former papers to explain the difficulty which those calculations brought to light, namely, that the amplitudes of the arcs from Kaliana to Kalianpur and from Kalianpur to Damargida, determined geodetically, were so little in excess as they proved to be of the same amplitudes determined astronomically,—a difficulty which he endeavoured to get over by attributing to the Indian Arc a curvature different from that corresponding to the mean meridian of the earth. In the present communication, introducing the condition that the length of the chord of the arc must be the same in both the ellipses, the local and the mean, drawn through the stations at the extremities of the arc, he demonstrates that no change in the curvature of the arc, within reasonable and indeed within wide limits, can have any appreciable effect on the calculated amplitude.


1876 ◽  
Vol 166 ◽  
pp. 315-324 ◽  

In a paper read before the Royal Society, May 1874, I pointed out that the upward diminution of temperature in the atmosphere (known to exist under certain circumstances) must refract and give an upward direction to the rays of sound which would otherwise proceed horizontally; and it was suggested that this might he the cause of the observed difference in the distinctness with which similar sounds are heard on different occasions, particularly the very marked advantage which night has over day in this respect. At the time at which that paper was written no direct experiments or observations had been made to verify the truth of this suggestion, and therefore its probability rested on its reasonableness. Since that time, however, I have carried out a series of observations and experiments which, although far from complete, throw some light on the subject, besides revealing some remarkable facts. I hope to be able to continue the investigation; but since its nature is such as to render the chance of bringing it to any thing like a final conclusion very uncertain, it seems to me that it may be well to publish an account of what has been already done; and this is the object of the present communication. In order to render the object of the various experiments clear, it may be well to recapitulate here some of the theoretical considerations previously explained. It will be remembered that the idea that the variations of temperature would cause refraction of sound occurred to me while making experiments on the effect of wind upon sound, from which it was shown that when sound proceeds in a direction contrary to that of the wind, it is not, as had been thought, destroyed or stopped by the wind, but that it is lifted, and that at sufficiently high elevations it can be heard to as great distances as in other directions, or as when there is no wind—thus confirming the hypothesis first propounded by Professor Stokes and afterwards by myself, that the effect is owing to the retardation of the velocity of the wind near the earth, which allows the sound moving against the wind to move faster below than above, and thus causes the fronts of the waves to incline upwards, and consequently to move in that direction. Having clearly shown that this was the case, it became apparent that any thing which would cause an upward diminution in the velocity at which sound proceeds would cause a similar effect to that of the wind and lift the sound, and that since the speed of the sound depends on the temperature of the air in which it is moving, an upward diminution in the temperature must cause such an effect. That such a diminution of temperature does very often exist was proved by Mr. Glaisher’s balloon ascents in 1862, in which he found that when cloudy the mean rate of diminution for the first 300 feet was 0°·5 for each 100 feet, and that when clear it was 1°, and that on some occasions it was greater and on others less than this. A variation of 1° in the temperature of the air alters the velocity of sound nearly 1 foot per second, so that with a clear sky the sound instead of moving horizontally would move upwards on a circle of 110,000 feet radius, and with a cloudy sky on a scale of 220,000 feet radius. This rate of refraction is very small compared with that caused even by a very moderate wind; and consequently in order to verify it by experiment it is necessary to observe sounds at much greater distances. This renders the experiment very difficult to carry out; and to make it worse we have no means of determining what the upward variation of temperature is, which therefore can only be surmised by the behaviour of the sound.


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