In this section we will briefly investigate another special type of tide called the perigean spring tide. Sometimes they are also referred to as king tide. These are naturally occuring tides that are higher than usual. To understand their origin we first have to look at the orbit of the Moon.
The tidal models discussed so far were based on simplified circular orbits. Although this has been a justifiable simplification it is a tad too simple to explain the finer details of tides. Now lets have a closer look at the realities of the Moon and its orbit and how this is affecting the tides. We already learned about Spring tides and Neap tides. Now lets look into a special type of spring tide called the perigean Spring Tide. To understand perigean spring tides lets first look at the orbit of the Moon.
Moon orbits the Earth in prograde direction. Prograde direction means this is the same direction that earth is spinning. It completes one revolution with respect to the stars in 27.32 days. This is also called a siderial period. Both Earth and Moon are orbiting a common center of mass (the barycenter). The Orbit of the Moon is distinctly elliptical. Its average eccentricity is 0.0549 which brings the ellipse pretty close to a cirlce. The greatest distance between Moon and Earth is 405400 km (Apogee) the shortest distance is 362600 km (Perigee). The following image shows a schematic of the Moons orbit.
Perigean Spring Tides occur when Sun, Earth and Moon are arranged in a line and the Moon is it its Perigee at the same time. In other words: The Moon is either full or new and it is closest to Earth . Such an arrangement happens three to four times per year. The difference in water level between ordinary Spring Tides and Perigean Spring Tides is usually a couple of centimeters with a maximum difference of 15 cm being on record for parts of the Alaska coast. When seen with respect to the tidal range of 9 m in the same area the effect is rather small (<2 %).
Another property having an influence on the height of local tides is the tilt of the axis of the earth and the tilt of the Moon orbit against the ecliptic. For those who have not heard the term before: That is the plane in which the earth orbits the sun. The Earth axis is tilted 23.44° against the ecliptic. The Moons orbit is tilted 5.14° against the ecliptic. In this chapter we will focus on the effect caused by the tilt of the Moons orbit.
It is rather trivial to imagine, that spring tides are a bit stronger if the Moon happens to be located at a point in its orbit where it intersects with the ecliptic. Only then Sun, Moon and Earth are located exactly at a straight line. This is also the only arrangement under which lunar or solar eclipses will occur. From that we can draw the conclusion that at the times of lunar or solar eclipse tides are a bit stronger stronger than usual.
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