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corresponding clump in the group around our time, the saros number goes up by about 19 and the inex goes up by about 2. (Notice that the inex values are higher at the bottom of the graph.) Any eclipse having inex and saros point lying along a line going through the first cluster on the right (at around inex 53 and saros 123) and the third cluster on the left occurs after perihelion and before aphelion (presently
Northern Hemisphere spring), whereas any on a line going through the second cluster on the right and the fourth on the left occurs after aphelion and before perihelion (presently Northern Hemisphere autumn).
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This shows the inex and saros numbers for the eclipses of the tetrads between AD 1000 and 2500. A
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Inex and saros for tetrads between AD 1000 and 2500
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