{"title":"On the coincidence of the bright lines of the oxygen spectrum with bright lines in the solar spectrum","authors":"H. Draper","doi":"10.2475/ajs.s3-18.106.262","DOIUrl":"https://doi.org/10.2475/ajs.s3-18.106.262","url":null,"abstract":"","PeriodicalId":7651,"journal":{"name":"American Journal of Science and Arts","volume":"4 1","pages":"262 - 277"},"PeriodicalIF":0.0,"publicationDate":"1879-06-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"87513735","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Notice of recent scientific publications in Brazil; O. A. Derby on the geology of the lower Amazonas","authors":"R. Rathbun","doi":"10.2475/ajs.s3-17.102.464","DOIUrl":"https://doi.org/10.2475/ajs.s3-17.102.464","url":null,"abstract":"","PeriodicalId":7651,"journal":{"name":"American Journal of Science and Arts","volume":"144 1","pages":"464 - 468"},"PeriodicalIF":0.0,"publicationDate":"1879-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"78570895","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"First catalogue of radiant points of meteors","authors":"F. Sawyer","doi":"10.2475/AJS.S3-17.102.468","DOIUrl":"https://doi.org/10.2475/AJS.S3-17.102.468","url":null,"abstract":"","PeriodicalId":7651,"journal":{"name":"American Journal of Science and Arts","volume":"s3-17 1","pages":"468 - 471"},"PeriodicalIF":0.0,"publicationDate":"1879-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"79793024","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"On the dark lines of oxygen in the solar spectrum on the less refrangible side of G","authors":"J. Draper","doi":"10.2475/ajs.s3-17.102.448","DOIUrl":"https://doi.org/10.2475/ajs.s3-17.102.448","url":null,"abstract":"IN a paper on the lines of oxygen, published in this Journal for October, 1878, the solar lines closely coincident with those of the eleetric spectrum of oxygen were given. The measurements of the solar lines in that instance were taken from photographs made in March, 1878. Since that time, under more favorable atmospheric conditions, I have succeeded in obtaining finer photographs on the less refrangible side of G. These show many faint lines, not visible in the photographs of March 1878, while many other lines are distinctly sub-divided. Three of the recent photographs were taken on the same day, during the last week in November, and two have been taken since that time i one during the last week in January, and one during the first week in Febmary. In all five of these photographs faint lines are visible between ,l. 4316 and ,l. 4320, of Angtsrom's scale, and they all show them in the position indicated by the diagram and table. The fact that aU the photographs agree iu their representation of these lines, is, I think, proof positive of the correctness of the positions assigned.","PeriodicalId":7651,"journal":{"name":"American Journal of Science and Arts","volume":"42 1","pages":"448 - 452"},"PeriodicalIF":0.0,"publicationDate":"1879-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"84126264","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"On a new absolute galvanometer","authors":"N. Hodges","doi":"10.2475/ajs.s3-17.102.475","DOIUrl":"https://doi.org/10.2475/ajs.s3-17.102.475","url":null,"abstract":"IN the ordinary form of galvanometer the current is measured by the ratio of the force it exerts on the needle to the directive force of the earth, the ratio being determined by a measurement of the angle of deflection. The moment of the force with which a unit current acts on the needle may be expressed in a series of the form G1 gl sin IJ + G,g, sin IJ Q,'(IJ) + etc. where G\" G 2 are constants depending on the dimensions of the coil, and g\" g 2 on those of the suspended apparatus, coil or magnet, as the case may be. Q/ ({}), Q/ ({}) are quantities varying with the deflection. Only in case all the terms after the first may be neglected are the values of the current proportional to the tangents of the deflections. With a single coil this is not the case. By increasing the number of coils and suitabl,V placing them, the magnetic field may be rendered more uniform. In reading the deflection ei ther a di vicled circle or a telescope and scale may be used. With the divided circle the deflection may be as great as 45°, but not more, or else the instrument would not be sensitive to changes in the current. The use of telescope and scale necessitates much smaller deflections. To regulate the strength of the current shunts of small resistance often have to be used; and the proportion of the current throngh the instrument is rendered doubtful. If, instead of placing the plane of the coils parallel with the magnetic meridian, they are placed perpendicular to it, the sum of the force of the current and of the directive force of the earth would influence the magnet.","PeriodicalId":7651,"journal":{"name":"American Journal of Science and Arts","volume":"1 1","pages":"475 - 476"},"PeriodicalIF":0.0,"publicationDate":"1879-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"81158214","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Notice of recent additions to the marine fauna of the eastern coast of North America","authors":"A. E. Verrill","doi":"10.2475/ajs.s3-17.102.472","DOIUrl":"https://doi.org/10.2475/ajs.s3-17.102.472","url":null,"abstract":"OF Polyzoa about 140 species have beeu identified by the writer from the coast between Cape Cod and Labrador. Nearly all these are Arctic or European species, already known. They are mostly described in Smitt's papers on Arctic Bryozoa. They are also mostly enumerated by the writer: in a Oheck-list of the Marine Invertebrata of this coast, now in type. The following is one of the more interesting new forms. The recent determination of so large a number of American Polyzoa, confirms the decision already arrived at, several years ago, from the study of other classes, that the fauna of northern New England is remarkably arctic and chiefly of northern origin, and that the fauna of Greenland is more allied to that of Northeastern America than to that of Northern Europe. In a valuable paper* on the Podophthalmous Crustacea of our northern coast, just published, Professor S. I. Smith has arrived at the same results for that group.","PeriodicalId":7651,"journal":{"name":"American Journal of Science and Arts","volume":"91 1","pages":"472 - 474"},"PeriodicalIF":0.0,"publicationDate":"1879-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"90944080","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"On ethylidenamine silver sulphate","authors":"W. Mixter","doi":"10.2475/ajs.s3-17.102.427","DOIUrl":"https://doi.org/10.2475/ajs.s3-17.102.427","url":null,"abstract":"ALDEHYDE AMMONIA precipitates metallic silver from many of its salts almost as readily as from the nitrate. A mixture of solutions of silvet' sulphate and aldehyde ammonia produces a mirror when warmed, and at common temperatures evaporates to dryness, with but slight decomposition. The fact that a sulphate solution decomposed less readily than the nitrate led to the hope that an investigation of the sulphate compound would throw more light on the constitution of silver amines. The first experiments were made with ammoniacal aqueous solutior.s of silver sulphate and aldehyde ammonia. Analyses proved the crystalline product to be a mixture. Alcoholic ammonia was next used as a solvent, and the analysis of the first crop of crystals showed nearly pure Ag2S04(NH~)4' 0'6 per cent of carbon was found and a solution of the crystals reacted for aldehyde. Aqueous solutions of silver sulphate and a lal'ge excess of aldehyde ammonia, over four molecules of the latter to olle of the former, yielded either mixtures or ammonio silver sulphate. When, however, aldehyde ammonia is dissolved in a small quantity of water, and silver sulphate, in the proportion of one molecule of the lat.ter to four molecules of the formel', is slowly added with constant agitation; and after some hours the small black residue filtered off and the solution left to spontaneous evaporation, few or no crystals of the ammonio, sulphate form, but colo1'less tl'ansparent crystals separate, whICh react strongly for aldehyde. At summer temperatures tabulat' crystals, and at from 10° to 15° C. elongated crystals, predominate. The following analyses were made of carefully selected and well-defined tabular crystals, which were from 2 to 5mm in diameter, and which were freed as much as possible from the mother liquor by blotting paper, then washed with alcohol and finally with ether. They were considel'ed dry when they did not lose weight on the balance in five or ten minutes.","PeriodicalId":7651,"journal":{"name":"American Journal of Science and Arts","volume":"26 1","pages":"427 - 429"},"PeriodicalIF":0.0,"publicationDate":"1879-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"80271141","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"On the force of effective molecular action","authors":"W. A. Norton","doi":"10.2475/ajs.s3-17.102.433","DOIUrl":"https://doi.org/10.2475/ajs.s3-17.102.433","url":null,"abstract":"should then be the value of the minimum repulsive ordinate, that obtains when x=3r, in the curve for water at the point of ebullition (2120 F.). This result gives for this curve k=4·931. In this curve the same molecular repulsion occurs again at x=1l5r. Now taking 1581 for the ratio of expansion by volume of water converted into steam at 212 0 F., and for the distance between the effective molecules of the steam, 1151', and putting y= distance of the inner surface of the effective envelope from the center of the molecule, I have","PeriodicalId":7651,"journal":{"name":"American Journal of Science and Arts","volume":"9 1","pages":"433 - 447"},"PeriodicalIF":0.0,"publicationDate":"1879-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"76176387","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"The forests of central Nevada, with some remarks on the those of adjacent regions","authors":"C. Sargent","doi":"10.2475/ajs.s3-17.102.417","DOIUrl":"https://doi.org/10.2475/ajs.s3-17.102.417","url":null,"abstract":"To the traveler crossing the Great Basin by the line of the Pacific Railroad the country will appear almost as destitute of trees as the great plateau over which he has passed in approaching the Rocky Mountains from the east. This first impression will disappear, however, should he penetrate farther south, and ascend some of the low mountain ranges, which, with a general north-and-south trend, everywhere cut up this elevated interior region into long, narrow valleys. As compared with our Atlantic forests, or those still nobler ones which, farther to the west, owe their existence to the influence of the Pacific, the forests which clothe, with a scanty and stunted vegetation, the mountain slopes of Nevada are miserably poor in extent, productiveness, and especially in the number of species of which they are composed. Actually they are of immense value. For scanty as they are, they regulate and protect the rare and uncertain streams on which the agl'lculture of Nevada depends, and furnish a large population with fuel and lumber; a population, too, which, while consuming and wasting enormously its forests in vast mining operations, is practically cut off, by its isolation and the cost of transportation, from outside supply. A hurried journey made in Septemper last, undertaken for the purpose of studying in situ the trees of the\" Great Basin,\" and of introducing into cultivation some of the peculiar plants of that region, took me to the great mining center of Eureka, and then throllgh Dry and Fish-spring valleys seventy-five , miles further southwest into the Monitor Range, to the point","PeriodicalId":7651,"journal":{"name":"American Journal of Science and Arts","volume":"186 1","pages":"417 - 426"},"PeriodicalIF":0.0,"publicationDate":"1879-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"78887174","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Notes on the satellites of Saturn","authors":"M. Mitchell","doi":"10.2475/AJS.S3-17.102.430","DOIUrl":"https://doi.org/10.2475/AJS.S3-17.102.430","url":null,"abstract":"THE object glass of the telescope used in the observations which follow is of twelve and one-third inches diameter. Its deo ni tion is good. The telescope is used in such observations as its very imperfect mechanism will allow; the;;e are observations of the conjunctions of the satellites with the edge of Saturn's ring, of size and color, and of differences of right ascension. The last are made b.y connecting with the chronograph, and recording the time of passage of the satellites over a fixed wire. In the course of these observations such different relati ve magnitudes have been given to the small satellites, on different evenings, as to lead to the suspicion that some of them are variable. 'rhe sparkle of Tethys and the grayish blue color of Hhea make it seem unlikely that sUlall stars can have been taken for these two satellites; 'in the case of Encelad us and Dione m istakes are more easily made; but the rapid motion of Enceladus soon establishes its identity. The most noticeable changes are in Rhea. In 1877, Hhea is recorded as small on Nov. 30th; as dull on Dec. 3d; as blurry and large, Dee. 14th; and as ruddy, Dec. 18th. In 1878 Rhea is recorded as faint Oct. 3d and Oct. 16th; as bright on Oct. 25th, and on Dec. 3d it is called nearly as bright as 'ritan.","PeriodicalId":7651,"journal":{"name":"American Journal of Science and Arts","volume":"11 1","pages":"430 - 432"},"PeriodicalIF":0.0,"publicationDate":"1879-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"87446411","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}