FREE BOOKS

Author's List




PREV.   NEXT  
|<   149   150   151   152   153   154   155   156   157   158   159   160   161   162   163   164   165   166   167   168   169   170   171   172   173  
174   175   176   177   178   179   180   181   182   183   184   185   186   187   188   189   190   191   192   193   194   195   196   197   198   >>   >|  
effect upon magnetic terrestrial phenomena, but how this is produced remains unknown. Besides sun-spots, there are seen on the solar disc bright flocculent streaks or ridges of luminous matter called _faculae_; they are found over the whole surface of the Sun, but are most numerous near the limb and in the immediate vicinity of the spots. They have been compared to immense waves--vast upheavals of photospheric matter, indicative of enormous pressure, and often extending in length for many thousands of miles. Nearly all observers have arrived at the conclusion that sun-spots are depressions or cavities in the photosphere, but considerable difference of opinion exists as to how they are formed. The most commonly accepted theory is that they are caused by the pressure of descending masses of vapour having a reduced temperature, which absorb the light and prevent it reaching us. Our knowledge of the Sun is insufficient to admit of any accurate conclusion on this point; though we are able to perceive that the surface of the orb is in a state of violent agitation and perpetual change, yet his great distance and intense luminosity prevent our capability of perceiving the ultimate minuter details which go to form the _texture_ of the solar surface. 'Bearing in mind that a second of arc on the Sun represents 455 miles, it follows that an object 150 miles in diameter is about the _minimum visible_ even as a mere mathematical point, and that anything that is sufficiently large to give the slightest impression of shape and extension of surface must have an area of at least a quarter of a million square miles; ordinarily speaking, we shall not gather much information about any object that covers less than a million.'[13] Since the British Islands have only an area of 120,700 square miles, it is evident that on the surface of the Sun there are many phenomena and physical changes occurring which escape our observation. Though the changes which occur in the spots and faculae appear to be slow when observed through the telescope, yet in reality they are not so. Tremendous storms and cyclones of intensely heated gases, which may be compared to the flames arising from a great furnace, sweep over different areas of the Sun with a velocity of hundreds of miles an hour. Vast ridges and crests of incandescent vapour are upheaved by the action of internal heat, which exceeds in intensity the temperature at which the most refractory of terr
PREV.   NEXT  
|<   149   150   151   152   153   154   155   156   157   158   159   160   161   162   163   164   165   166   167   168   169   170   171   172   173  
174   175   176   177   178   179   180   181   182   183   184   185   186   187   188   189   190   191   192   193   194   195   196   197   198   >>   >|  



Top keywords:

surface

 
conclusion
 

compared

 

pressure

 

million

 

square

 

prevent

 

matter

 
vapour
 

object


phenomena

 

faculae

 

ridges

 

temperature

 

information

 
covers
 

gather

 

visible

 
mathematical
 

minimum


diameter

 

represents

 

sufficiently

 

quarter

 
ordinarily
 

extension

 

slightest

 

impression

 

speaking

 

velocity


furnace

 

flames

 
arising
 
hundreds
 

exceeds

 

intensity

 

refractory

 

internal

 

action

 

crests


incandescent

 
upheaved
 

heated

 

intensely

 

occurring

 

physical

 

escape

 

observation

 
Though
 
evident