444 Mr. South on the discordances between the 
Table XX. shows us, that the mean of 31 observations 
made at Greenwich in 1821 , gave the observed right ascen- 
sion of the sun, greater than his computed right ascension, 
0.627 of a second of time. 
And Table XXL informs us, that by the mean of 45 ob- 
servations, made at Greenwich in 1822, the observed right 
ascension, was found greater than the computed, 0.420 of a 
second. 
Table XXII. presents us with the mean of 16 observations 
of the sun, made at the Royal Observatory of Paris in 1821, 
whereby his observed right ascension, exceeds his computed 
right ascension, 0.584 of a second. 
And Table XXIII. indicates, that by 28 observations made 
at the Paris Observatory in 1822, the observed right ascension, 
was found greater than the computed right ascension, 0.558 
of a second. 
Table XXIV. offers to our notice, 9 observations of the 
sun, made in the year 1821, at Dublin ; whereby the observed 
right ascension, was determined to be greater than the com- 
puted, 0.666 of a second. 
And Table XXV. exhibits 15 observations made in 1822, 
at the Observatory of Dublin, giving the observed right 
ascension of the sun, greater than his computed, by 0.686 of a 
second of time. 
The two following Tables will facilitate the comparison of 
the results, as obtained at the respective observatories. 
