This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.
The partial solar eclipses on March 27, 1884 (part of Saros 108) and December 24, 1916 (part of Saros 111) are also a part of this series but are not included in the table below.
| Series members between 1971 and 2200 | ||||
|---|---|---|---|---|
 July 22, 1971 (Saros 116) |
 June 21, 1982 (Saros 117) |
 May 21, 1993 (Saros 118) |
 April 19, 2004 (Saros 119) |
 March 20, 2015 (Saros 120) |
 February 17, 2026 (Saros 121) |
 January 16, 2037 (Saros 122) |
 December 16, 2047 (Saros 123) |
 November 16, 2058 (Saros 124) |
 October 15, 2069 (Saros 125) |
 September 13, 2080 (Saros 126) |
 August 15, 2091 (Saros 127) |
 July 15, 2102 (Saros 128) |
 June 13, 2113 (Saros 129) |
 May 14, 2124 (Saros 130) |
 April 13, 2135 (Saros 131) |
 March 12, 2146 (Saros 132) |
 February 9, 2157 (Saros 133) |
 January 10, 2168 (Saros 134) |
 December 9, 2178 (Saros 135) |
 November 8, 2189 (Saros 136) |
 October 9, 2200 (Saros 137) | |||