FREE BOOKS

Author's List




PREV.   NEXT  
|<   44   45   46   47   48   49   50   51   52   53   54   55   56   57   58   59   60   61   62   63   64   65   66   67   68  
69   70   71   72   73   74   75   76   77   78   79   80   81   82   83   84   85   86   87   88   89   90   91   92   93   >>   >|  
f night. In the Sahara itself, when the sun's rays cease to impinge on the burning soil, the temperature runs rapidly down to freezing, because there is no vapour overhead to check the calorific drain. And here another instance might be added to the numbers already known, in which nature tends as it were to check her own excess. By nocturnal refrigeration, the aqueous vapour of the air is condensed to water on the surface of the earth; and, as only the superficial portions radiate, the act of condensation makes water the radiating body. Now experiment proves that to the rays emitted by water, aqueous vapour is especially opaque. Hence the very act of condensation, consequent on terrestrial cooling, becomes a safeguard to the earth, imparting to its radiation that particular character which renders it most liable to be prevented from escaping into space. It might however be urged that, inasmuch as we derive all our heat from the sun, the selfsame covering which protects the earth from chill must also shut out the solar radiation. This is partially true, but only partially; the sun's rays are different in quality from the earth's rays, and it does not at all follow that the substance which absorbs the one must necessarily absorb the other. Through a layer of water, for example, one tenth of an inch in thickness, the sun's rays are transmitted with comparative freedom; but through a layer half this thickness, as Melloni has proved, no single ray from the warmed earth could pass. In like manner, the sun's rays pass with comparative freedom through the aqueous vapour of the air: the absorbing power of this substance being mainly exerted upon the invisible heat that endeavours to escape from the earth. In consequence of this differential action upon solar and terrestrial heat, the mean temperature of our planet is higher than is due to its distance from the sun. ******************** 13. Liquids and their Vapours in relation to Radiant Heat. The deportment here assigned to atmospheric vapour has been established by direct experiments on it taken from the streets and parks of London, from the downs of Epsom, from the hills and sea-beach of the Isle of Wight, and also by experiments on air in the first instance dried, and afterwards rendered artificially humid by pure distilled water. It has also en established in the following way: Ten volatile quids were taken at random and the power of these quids, at a c
PREV.   NEXT  
|<   44   45   46   47   48   49   50   51   52   53   54   55   56   57   58   59   60   61   62   63   64   65   66   67   68  
69   70   71   72   73   74   75   76   77   78   79   80   81   82   83   84   85   86   87   88   89   90   91   92   93   >>   >|  



Top keywords:
vapour
 

aqueous

 
comparative
 

condensation

 
substance
 
thickness
 
freedom
 

terrestrial

 

radiation

 

partially


instance

 

temperature

 

experiments

 

established

 

rendered

 

single

 

proved

 

Melloni

 

manner

 

warmed


artificially

 

distilled

 

random

 

transmitted

 
volatile
 
absorbing
 

Vapours

 

relation

 

Radiant

 

Liquids


distance

 
London
 
assigned
 

atmospheric

 

direct

 

streets

 

deportment

 

invisible

 

endeavours

 
escape

exerted
 
consequence
 

planet

 

higher

 
differential
 

action

 

selfsame

 

excess

 

nature

 
numbers