FREE BOOKS

Author's List




PREV.   NEXT  
|<   28   29   30   31   32   33   34   35   36   37   38   39   40   41   42   43   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   >>   >|  
These undulations were noticed by Airy in 1842 about 6 minutes before totality. Blake, in America in 1869, observed the same phenomenon 8 minutes before totality. In other cases the interval would seem to have been very much shorter--a mere matter of seconds. A very singular observation was made in 1858 by Mr. J. D. Smith at Laycock Abbey, Wiltshire, on the occasion of the annular eclipse of that year. He says[13]:--"Both my brother and myself were distinctly impressed with the conviction that the withdrawal of light was not continuous, but by pulsations, or, as it were, waves of obscuration, the darkness increasing by strokes which sensibly smote the eye, and were repeated distinctly some five or seven times after we had remarked the phenomenon and before the time of greatest obscuration. This did not occur on the return of light, which came back continuously and without shock or break." Ruemker mentions that though this phenomenon was very apparent to the naked eye it was not visible in the telescope. Faint rays or brushes of light sometimes seem to spring from the diminishing crescent of the Sun. These rays generally are very transient and not very conspicuous, and perhaps must be distinguished as regards both their appearance and their origin from the more striking rays which are usually seen a few minutes before or after totality, and which are generally associated with, or even deemed to belong to, the Corona. Fig. 7 represents these rays as seen in Spain on July 18, 1860, some minutes after totality. They are described as having been well defined, but at some moments more marked than at others, and though well-defined yet constantly varying. Radiations of light more or less of the character just described may probably be regarded as a standing feature of every total eclipse. [Illustration: FIG. 7.--RAYS OF LIGHT SEEN NEAR THE TIME OF TOTALITY.] THE APPROACH OF TOTALITY. The next thing to think about and to look out for is the approach of the Moon's shadow. I have mentioned this already,[14] and also the appalling velocity with which it seems to approach. By this time the coming darkness, which characterises every total phase, will have reached an advanced stage of development. The darkness begins to be felt. The events which manifest themselves at this juncture on the Earth (rather than in the sky around the Sun) are so graphically described by the American writer whom I have alrea
PREV.   NEXT  
|<   28   29   30   31   32   33   34   35   36   37   38   39   40   41   42   43   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   >>   >|  



Top keywords:

totality

 

minutes

 

phenomenon

 

darkness

 

eclipse

 
obscuration
 

approach

 

distinctly

 
TOTALITY
 

defined


generally

 

represents

 

Corona

 
deemed
 

feature

 
belong
 

standing

 

constantly

 
varying
 

Illustration


marked

 

moments

 

Radiations

 

character

 

regarded

 

begins

 

development

 

events

 
manifest
 

advanced


reached

 
juncture
 

American

 

writer

 

graphically

 

characterises

 

coming

 

APPROACH

 

appalling

 

velocity


shadow

 

mentioned

 

Laycock

 
Wiltshire
 

occasion

 

annular

 
impressed
 
conviction
 

withdrawal

 

brother