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. 



Hour 



Sun's 



Sun's 



Hour 



Sun's 



Sun's 



from Noon 



Azimuth 



Altitude 



from Noon 



Azimuth 



Altitude 







0° 



82°-75 



4 



95° 



34°-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 







3-5 



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. 2. 



