Is proceeding, as has been the custom of my t of the labors of the society during the that I should acknowledge how greatly my rupulous exactness with which the reports of drawn up by our secretary, M. Ed. Claparède. ntion, many have been already communicate o, through the medium of scientific journals; al restrict myself to an indication of the titles, conclusions arrived at. In the arrangement of adopt the division into two sections, that of the sciences, first proposed by M. de la Rive, a part of the presidents who have succeeded the example of my immediate predecessor in to ons which have taken place either on the before the society or of verbal reports on recent es; not that these discussions have not often po case it is essential, if this valuable observanc the appreciation of the labors of others, the hone is sometimes led to enunciate ideas arising always sufficiently considered, should receive no ch results from the reading of the journal of our PHYSICAL SCIENCES. Or indefatigable colleague, Professor Gautier, ha ty well informed of the discoveries made in astr have been numerous and diversified; we must he n of the most important. M. Gautier presented a report on the observations of M. d'Arrest, of amber and to the variability in brightness of t in points, still doubtful, which would tend to indi Some of those bodies; secondly, an account of a men ds of the variations of magnetic declination, and t M. Maine on the flattening of Mars, which he esti on some recent observations of M. Donati on the the same author relative to stellar spectra: M. Gau 13 s SICS AND NATURAL HISTORY OF GENEVA, M JULY, 1862, TO JUNE, 1863. BY PROFESSOR MARCET, PRESIDENT. RANSLATED FOR THE SMITHSONIAN INSTITUTION. has been the custom of my predecessors, to present an s of the society during the year just elapsed, it is- but acknowledge how greatly my task has been facilitated by ness with which the reports of our several meetings have ir secretary, M. Ed. Claparède. Among the topics claiming have been already communicated to the public, or are about e medium of scientific journals; as regards these, therefore, If to an indication of the titles, or a very summary analysis rived at. In the arrangement of subjects I cannot do better ion into two sections, that of the physical and that of the st proposed by M. de la Rive, and since observed by the presidents who have succeeded him. I shall follow, moref my immediate predecessor in touching very lightly on the ave taken place either on the occasion of original memoirs ety or of verbal reports on recent discoveries made in other these discussions have not often possessed a genuine interest, sential, if this valuable observance is to be retained by us, on of the labors of others, the verbal communications in mes led to enunciate ideas arising at the moment and perhaps atly considered, should receive no greater publicity than that the reading of the journal of our sittings. PHYSICAL SCIENCES. le colleague, Professor Gautier, has continued to keep the ed of the discoveries made in astronomy. His communicamerous and diversified; we must here limit ourselves to the t important. M. Gautier presented to the society, in the first the observations of M. d'Arrest, of Copenhagen, relative to o the variability in brightness of the nebula, as well as to doubtful, which would tend to indicate a proper movement odies; secondly, an account of a memoir of M. Lamon on the tions of magnetic declination, and the analysis of researches he flattening of Mars, which he estimates at ; thirdly, a ent observations of M. Donati on the comets, and on a memoir relative to stellar spectra: M. Gautier announced on this 39 sics establishing a natural bond between I called, we shall first direct our attention to owe to Professor Plantamour. Besides the r Geneva and Saint-Bernard, published, as al and natural sciences of the "Bibliotheque communicated to the society an interesting ade at Geneva, for thirty-five years, on the He has found that in winter the number of inds balance each other; the northeast pren, the southwest in summer. The general which proceeds from the fact that the mean nearly approximates to north than does the 3 to south. The above results are somewhat s be taken into account and if local are disThe former depend chiefly on the vicinity of erature in the twenty-four hours, giving rise vening, analogous to breezes of the land and our has been lately published in his extensive (See page 15, et sequent.) to the Society during the year und society a memoir on the diurnal variations of He has satisfied himself, in ter, the existence of the oscillat . He has demonstrated experin With hydrogen, the best cond la Rive completed his communi ich has played the principal part in the communications ring the year under review. Our colleague, M. de la d to us, at two consecutive meetings, the results of his >mena which characterize and accompany the propagation rarefied elastic fluids. In the classification of his apinsists more particularly on the means which he has emintensity of the discharges or transmitted currents, by erived current taken by means of two small sounds of I water placed in the circuit of the principal current. nometer which enables him to appreciate to nearly the etre, and, for practiced eyes, even to the hundredth part, stic fluid submitted to experiment. The researches of en directed to atmospheric air, nitrogen, and hydrogen. case of each of these gases, the influence of the dimengaseous mass, as well as of the pressure, on its capacity ricity. He has described the successive appearances it assumes, in proportion as the pressure of the gas diminthe variable form and size of the stratifications of that e formation of a violet-colored photosphere around the ball electrode, and of a black space, from five to ten centich separates that photosphere from the stratified luminous tisfied himself, in the course of a great number of exe appearances of electric light in rarefied gases are effect produced by the transmission of electricity, an idea been advanced by M. Riess. M. de la Rive has sucy direct experiments, that the mechanical effect in quessiderable dilatation of the gaseous matter near the negative y alternate contractions and dilatations in the column up to e. First. He was easily able to verify, by means of the ence of the oscillatory movement in the gaseous column, n its intensity, which depends, as he has shown, on the nsion, and dimensions of the gaseous mass in question. monstrated experimentally that if, by means of small sounds ranged, derived currents are taken in different parts of the traversed by the same discharge, great differences will be 7 of these currents, differences which prove that the obgreater conducting capacity, and are consequently the most ogen, the best conductor of the gases, no derived current scure part of the column. Thirdly. M. de la Rive points ions of the thermometer placed in different parts of the duct us to the same results, by evincing great differences tures of those different parts; the more obscure parts being han the luminous, which proves that the former are better thor has obtained a great number of numerical results, inces of temperature, at different pressures of various portions in traversed by the discharges. pleted his communication at a subsequent session, by exty the modifications produced in the phenomena relative to _ectricity, through highly rarefied mediums, by the action of n of the current, the nature of the gas, and its pale electricity by M. Wheats practicable to obtain despatches y The same physicist communicated phenomenon observed by M. A the summit of the Oldenhorn. Of the persons who accompanied hir of the telegraph. In a few mom Fratessor de la Rive, on his return, red to the Society several new sei attention, in particular, to an inve at had arrived, simultaneously wi the earth cannot be liquid in its i Em that it is not necessary to rec nally into the sun, in order to e re of that body. It suffices to a undetermined cause, is now gr ding to M. Helmholtz, the cale the rapidity of refrigeration ed to take account of an imp es in volume as it grows coo 7ew heat. de la Rive presented to the Soci Kve, a memoir on the number of in of linear currents. This men to analysis. Pssor Marcet has continued to in more than is usual in an analysis of the memoir stification, not only in the importance of the subhat the results which he obtained have been hereents. The entire memoir is about to appear in Memoirs of the Society, now in the press.* owe to M. de la Rive the model of a new system odification which he has introduced into the battially calculated to render its management more instrument, which is extremely manageable, and f alumina, possesses the advantage of requiring endering superfluous the removal of the nitric or the service of several days and many experi ngle pair of this battery, M. de la Rive has been experiments of the electro-dynamics of Ampérequire five or six pairs of Grove or of Bunsen. unications by Professor Wartmann relative to arly to the limit of pressure which permits a us medium, as well as to the influence which the edium exercises on the passage of a current, the e attention of the society by an account of some ssed in the last reunion of the British Association s present. Among the communications made on cites more particularly the observations of M. ure of the sun. To avoid the inconvenience of a ustead of introducing the solar rays directly into and tural radiation; among others, hours of the day. The auth I. Mareet has taken advantage of him to repeat at Queensland, experiments on nocturnal radiation rate climates. It would seem t Domenon of the increase of temper Ascend some feet above the surfa Lticated in our temperate climate = glass a lens which is plane on the side next the zone either at the rising or sett site side, so as to disperse the luminous rays quantity of light reflected by the plane surface. le to ascertain that towards the hour of noonday resting memoir is given in this report.-See page ree scarcely sensible, hardly ef ive has recently made some obse which would appear to lead to a * See Archives des Sciences Ph |