EEPOET OF THE SECRETARY. 91 



Mr. Fowle's research on the effect of water vapor and carbon 

 dioxide of the atmosphere to absorb long-wave rays, such as the earth 

 sends out, is now ready for publication. Many of the best observa- 

 tions were made by him during the past year. Some observations 

 made in February, 1917, at a time when the humidity of the atmos- 

 phere was very small, proved of special value. Opportunity was 

 taken of using some of the apparatus prepared for the South Amer- 

 ican expedition to aid in making holographic observations on the 

 solar spectrum at very great wave lengths, reaching to 17 microns. 

 By means of the spectrobolometer prepared for South America it 

 was possible to determine accurately the quantities of water vapor 

 in the pdth of the solar beam. 



Certain conclusions stated in Volume II of the Annals of the Astro- 

 physical Observatory may now be corrected to correspond with the 

 new information. We stated: 



We can by no means admit that the radiation from tlie solid and liquid sur- 

 face of the earth passes unhindered to space. * * * The clouds, whose 

 average presence includes 52 per cent of the time, * * * are even more 

 efficient screens to the radiation of the earth than they are to the radiation of 

 the sun, so during 52 per cent of the time we may regard the radiation of the 

 solid and liquid earth to space as zero. During the remainder of the time 

 water vapor presents almost as eifective a screen * * *. From the com- 

 bined work of Rubens and Aschkinass, Langley, Keeler and Very, and Nichols, 

 y^TQ * * * conclude that a tenth part of the average amount of water vapor 

 in the vertical column of atmosphere above sea level is enough to absorb more 

 than half of the radiation of the earth to space, and it is highly probable that, 

 considering the greater air mass attending the oblique passage of many of the 

 rays to space, nine-tenths of the radiation of the solid and liquid surface of 

 the earth is absorbed by the water vapor of the atmosphere even on clear days. 

 On cloudy days none is transmitted, so that the average escape of radiation 

 from the earth's surface to space probably does not exceed 5 per cent. 



Some writers have attributed a large share of the absorption of the atmos- 

 phere to the carbonic-acid gas which it contains, but * * * ji-, atmospheric 

 conditions the absorption of carbonic-acid gas in the spectrum of the earth 

 appears to be confined to two bands extending from wave lengths 3.6 to 5A/i, 

 and from 13.0 to 16.0,1*, respectively. In these bands its absorption is nearly 

 total from 4.0 to 4.8ya and from 14.0 to 15.6/t even vv^hen carbonic-acid gas is 

 present in much less quantities than the atmosphere contains. * * * Jn the 

 absence of water vapor the total absorption possible by carbonic-acid gas would 

 be 14 per cent. In all the lower regions of the atmosphere, however, water 

 vapor is present in such quantities as almost completely to extinguish the radi- 

 ation of the earth's surface in these two special regions. * * * j^ therefore 

 does not appear possible that the presence or absence, or increase or decrease, 

 of the carbonic acid contents of the air is likely to appreciably influence the 

 temperature of the earth's surface. 



It seems certain, in view of what has been said that the earth's solid and 

 liquid surfaces, and the lower parts of the atmosphere, contribute directly 

 almost nothing to the amount of radiation which the earth as a planet sends 

 to space. The earth's surface and the lower atmospliere, of course, exchange 

 radiation together, and by this process and by convection the heat of these 



