at the total solar Eclipse in 1882. 39 
possible, continuous observations should be made is from 9 a.m. to 
3 p.m. 
Table I. 
1 
Hour 
from Noon 
Sun’s 
Azimuth 
Sun’s 
Altitude 
Hour 
from Noon 
Sun’s 
Azimuth 
Sun’s 
Altitude 
0 
0° 
82*75 
4 
o 
95 
3 4° 5 
0-5 
46 
79-5 
4-5 
98-5 
28 
1 
65 
74 
5 
102 
21-5 
1*5 
73-5 
67*5 
5-5 
105 
15 
2 
81 
61 
6 
108 
9 
2-5 
85*5 
54 
6*5 
111 
2 
3 
89 
48 
6-65 
112-5 
0 
3-5 
1 
93 
41 
During the three days, the 16th, 17th and 18th May, the con- 
ditions were very favourable, and particularly so on the forenoon 
Fig. 1. 
Fig. 2. 
