Lunitidal interval


The lunitidal interval measures the time lag from lunar culmination to the next high tide at a given location. It is also called the high water interval. Sometimes a term is not used for the time lag, but instead the terms age or establishment of the tide are used for the entry that is in tide tables.
Tides are known to be mainly caused by the Moon's gravity. Theoretically, peak tidal forces at a given location would concur when the Moon reaches the meridian, but a delay usually precedes high tide, depending largely on the shape of the coastline and the sea floor. Therefore, the lunitidal interval varies from place to place - from 3 hours over deep oceans to eight hours at New York Harbor. The lunitidal interval further varies within about +/-30 minutes according to the lunar phase.
Hundreds of factors are involved in the lunitidal interval, especially near the shoreline. However, for those far away enough from the coast, the dominating consideration is the speed of gravity waves, which increases with the water's depth. By observing the age of leap tides, it becomes clear that the delay can actually exceed 24 hours in some locations.
The approximate lunitidal interval can be calculated if the moonrise, moonset, and high tide times are known for a location. In the Northern Hemisphere, the Moon reaches its highest point when it is southernmost in the sky. Lunar data are available from printed or online tables. Tide tables forecast the time of the next high water. The difference between these two times is the lunitidal interval. This value can be used to calibrate certain clocks and wristwatches to allow for simple but crude tidal predictions.