MR. LUBBOCK ON THE TIDES. 
263 
Table VIII., showing the Difference in the Interval between the Time of the Moon’s 
Transit and the Time of High Water, and the Interval corresponding to fifty-seven 
minutes of the Moon’s Horizontal Parallax. 
Table IX., showing the Difference between the Height of High Water and the 
Height corresponding to fifty-seven minutes of the Moon’s Horizontal Parallax. 
Table X., showing the Interval between the Apparent Solar Time of the Moon’s 
Transit and the Time of High Water, the Height of High Water, and the Interval 
between the Moon’s Transits, at the London Docks, corresponding to the Apparent 
Solar Time of the Moon’s Transit for every three degrees of her Declination north 
and south. 
Table XI. (Interpolated from Table X.), showing the Interval between the Appa- 
rent Solar Time of the Moon’s Transit and the Time of High Water at the London 
Docks for every three degrees of her Declination north and south. 
Table XII., showing the Interval between the Apparent Solar Time of the Moon’s 
Transit and the Time of Pligh Water at the London Docks, for every three degrees 
of her Declination north or south. 
Table XIII., showing the Difference in the Interval between the Apparent Solar 
Time of the Moon’s Transit and the Time of High Water at the London Docks, and 
the Interval corresponding to fifteen degrees Declination, for every three degrees 
of the Moon’s Declination north and south. 
Table XIV., showing the Difference in the Interval between the Apparent Solar 
Time of the Moon’s Transit and the Time of High Water at the London Docks, and 
the Interval corresponding to fifteen degrees Declination, for every three degrees 
of the Moon’s Declination north or south. 
Table XV. (Interpolated from Table X.), showing the Height of High Water at the 
London Docks for every three degrees of the Moon’s Declination north and south. 
Table XVI., showing the Height of High Water at the London Docks for every 
three degrees of the Moon’s Declination north or south. 
Table XVII., showing the Difference in the Pleight of High Water at the London 
Docks, and the Height corresponding to fifteen degrees Declination, for every three 
degrees of the Moon’s Declination north and south. 
Table XVIII. , showing the Difference in the Height of High Water at the London 
Docks, and the Pleight corresponding to fifteen degrees Declination, for every three 
degrees of the Moon’s Declination north or south. 
Table XIX., showing the Difference in the Height of High Water at the London 
Docks when the Moon’s Declination is north or south. 
The variation of the interval and in the height in Tables X. to XIX. inclusive, is 
partly due to the change of the sun’s declination, which is given in Table X. but not 
afterwards repeated, because interpolation for the even half-hour is not required. 
Table XX., showing the Interval between the Apparent Solar Time of the Moon’s 
Transit and the Time of High Water, and the Pleight of High Water at the London 
