Ill 11] on Recent Experiments with, fuvisible Lii/hf. 188 



by means of the obscure rays at the extreme red end of the spectrum. 

 A screen can be prepared which transmits these rays, and is at the 

 same time opaque to all other radiations, by combining a sheet of the 

 densest blue cobalt glass with a solution of bichromate of potash or 

 some suitable orange dye. 



Such a screen transmits a region of the spectrum comprised 

 between wave-lengths G900 and 7500. Though this region is visible 

 to the eye if all other rays are cut off, it is so t'eeble in its action that 

 it plays no part in ordinary vision, being overpowered by the other 

 radiations. "We may thence, for convenience, call photographs made 

 through such a screen infra-red pictures, though the infra-red region 

 is usually considered as beginning at the point where all action upon 

 the human retina ceases. 



The photographs which I am now going to show you were taken 

 through such a screen, with the spectrum plates made by Wratten and 

 Wainwright. The time of exposure was about three minutes in full 

 sunlight, with the lens stop set at //S. The views were, for the 

 most part, made in Sicily and Italy, and have a very curious appear- 

 ance, for while the sky comes out in all of them almost as black as 

 midnight, the foliage of the trees and the grass come out snow white. 

 This peculiar effect results from the failure of the atmosphere to 

 scatter these long rays. The green leaves, however, reflect them very 

 powerfully, or more correctly, transmit them, since we are dealing 

 with pigment or transmission colour. If we look at a landscape 

 through the screen, carefully protecting the eye from all extraneous 

 light with a black cloth, we shall find that the trees shine with a 

 beautiful rich red light against a black sky. This condition obtains 

 only on very clear days, for the presence of the least haze in the air 

 enables it to scatter the long rays, and you will notice that in those 

 pictures which show the sky down to the horizon, there is a pro- 

 gressive increase in its luminosity as we pass from the zenith down- 

 wards, as a result of the greater thickness of the mass of air sending 

 the scattered rays to the camera. 



Another point to be noticed is the intense blackness of the 

 shadows in the infra-red pictures, due to the fact that most of the 

 light comes directly from the sun and little or none from the sky, 

 which reminds one forcibly of the conditions which obtain on the 

 moon, where there is no atmosphere at all to form a luminous sky. 



When we come to the subject of photographs made with ultra- 

 violet light, we shall find that we have the conditions reversed, for 

 practically all of these very short waves are scattered by the atmo- 

 sphere, and we have no shadows even in full sunlight. 



We will now run through the series of infra-red pictures as rapidly 

 as possible, for I have a considerable number of them. The one 

 which is on the screen is one of the finest in the collection (Fig. 1). It 

 was made in the park at Florence, and shows the long drive, over- 

 shadowed by trees, the one in the foreground being particularly fine 



