( 9 ^ ) 
E. The Appearance of two Segments of Circles, at 
about the lame Diftance from the Sun, as the 
helia^ being perpendicularly above it, the Colours 
being fainter than in the Tarhelia, but the fame Way 
difpos’d, the lower Lines next the Sun expre/fing 
the red, and the upper the yellow. 
The Colours at D, and E, as they were not fo in- 
tenle, neither were they quite fo broad as thofe at B 
- and C ; the two Colours being added together were 
about I of the Disk at B, and the Colours in the fame 
Proportion at C ; the Diameter of the Tarhelion at 
B, being about double the apparent Diameter of the 
Sun, as near as I could compute, as in the Scheme is 
exprefs’cf. 
The Centres of the Segments of the Halo's mark’d 
E, if not in the ^arhelia^ were very little below ’em. 
Below the Sun and Parhelia the Cloud was too 
thick to difcover any thing thro’ it ; and above them, 
;; till near the Segments mark’d E, the Sky was ferene 
and nothing obfcured; but at E, where the Rays, 
which pointed upwards from the Sun, terminated, it 
appear’d hazy, and fb thick as to refled: the Colours. ' 
CaJHe "Hobbs^ 
1711. 
Arthur "Hobbs. 
II. A 
