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37 2 NATURE [DECEMBER I I, 1919

to· the "Age of ," which is illustrated by LETTERS TO THE EDITOR. such huge forms as Brontosaurus and Diplodocus, himself responsible for might be a fThe· Editor does not hold Stegosaurus and Triceratops, which opinions expressed by his correspondents. Neither first attempt at a Pachyderm, together with can he undertake to return, or to correspond with Megalosaurus, , and , the write.rs of, rejected manuscripts .intended for besides and Ichthyosaurus in the sea, this or any other part of NATURE. No notice is with flying creatures like Pterodactyles and taken of anonymous communications.] Archreopteryx, half , half ; and then dentigerous , which pass on to the Kainozoic, Gravitation and Light. and end the present part of the work, which when JUPITER ought just to show the Einstein deflectii)n, completed will be a broad survey of the world for if it pass between two stars a couple of diameters throughout time. of the planet apart, their temporary relative displace• Mr. \Vells has undertaken a d.ifficult task, and ment will be a "third" of arc, the sixtieth of a second, and this could be measured with a heliometer. it is not too much to say that no other· writer of OLIVER J. LODGE. the present day is so well equipped as he is to Mariemont, Edgbaston, December 6. bring it to a successful completion. He possesses the rare combination of brilliant literary power with comprehensive and precise knowledge, and The Deflection of Light during a Solar Eclipse. this distinctive quality makes his work one in PROF. ANDERSON suggested in NATURE of Decem• which all intelligent readers will find profit and ber 4 (p. 354) a possible source of systematic error delight. in the determination of the deflec tion of light at an eclipse, owing to lateral refraction caused by a tem• OUR BOOKSHELF. perature-gradient in the shadow-cone in our atmo• Principles of Electric Spark Ignition in Internal• sphere. Having carefully considered this suggestion, I feel convinced that the effects of a ny possible combustion Engines. By J. D. Morgan. temperature-gradient would be small. · Pp. vii+ 88. (London : Crosby Lockwood and Taking the height of the atmosphere as 10 miles, Son, 1920.) Price 8s. 6d. net. the ray from a star 3o' from the sun's centre would IN the eighty or so pages of this little book Mr. traverse a distance of 150 yards in the direction per• Morgan gives the result of certain experiments by pendicular to the shadow-axis whilst passing through a tem• others and himself to determine the nature of elec• our atmosphere. Prof. Anderson estimates perature-drop of 1 / 18 of a degree as required to pro• tric spark ignition in internal-combustion engines. duce the observed deflection. Thus the lateral tem• A wide circle of readers will feel grateful to the perature-gradient must be 1° C. per 1½ miles. The author for providing in this convenient form an shadow moves over the earth at about 30 miles a account of the more important work along these minute, so that for a stationary observer the fall of lines, and for the reference which he provides to temperature would have to be at the rate of 20° a the sources from which information in fuller !detail minute to produce the observed effect. single surface of discontinuity, be obtained. Mr. ;\forgan puts them still In the case of a may considered for simplicity by Prof. Anderson, the dis• further in his debt by the lucidity with which he placement by lateral refraction is inversely proportional writes, and his manifest endeavour-almost to the distance from the sun's centre ; but this Jaw always successful-to ensure that, even in the does not apply in the actual case of a continuous more intricate parts of the subject, his phraseology temperature-gradient. shall be free from the ambiguity which is so often It seems possible that the effect might amount to the despair of readers of technical books. as much as r / 20 of the Einstein de fl ection in some the rather high value found at ingeniously and cases, and possibly Mr. Morgan explains most Sobral has been increased by this cause. At Principe simply his view of the double nature of the spark, there was no perceptible change of temperature during its important "capacity " component and the less the eclipse, but the climatic conditions there are valuable "inductance" oscillation. Experiment exceptional. A. S. Eoor,-;GTON. so · far has failed to show anv effect on the result• Observatory, Cambridge. ant gaseous explosion, or o~ the upper and lower limits of richness at which explosion will occur, of change in the size, temperature, energy, or PROF. ANDERSON'S letter in NATURE of December 4 other feature of the spark. Any one individual raises a point well worthy of consideration-that is, the possibility of abnormal refraction due to the spark seems to be as good as any other, pro• lmvering of temperature in the air by the passage vided that explosion is caused; but the apparatus of the shadow cone. I do not, however, think that must be unfailing in the succession of sparks more than a very small portion of the e ffect noted at which it is designed to provide. Sobral could be explained in this way. The shadow The book is one which should be in the hands ellipse was 194 miles long {direction of motion) and of all who are interested in the scientific side of 137 miles broad. I have drawn a section in the former .-he design of internal-combustion engines in their direction to scale, taking the height as 20 miles. It is certainlv unnecessary to take it 'highe,·, as the many forms. That further work along these lines temperature of the upper air is unaffected by the will cause spark gaps to be less sensitive than passage of the shadow. they now are to short circuiting caused by the Photographs were taken at Sobral at uniform inevitable gradual loss of insulation is greatly to intervals throughout totality, and all give tolerably be hoped. · accordant values of the shift. NO. 2615, VOL. 104] © 1919 Nature Publishing Group