In addition to planned stereo pairs, the Pairendipity software can identify all overlapping images suitable for stereo processing. Global lists of such image pairs for the HiRISE and CTX datasets are provided here ordered by latitude. Images taken close together in time minimize illumination and frost differences and are especially useful (see the Delta-Days column). Stereo images planned within the same 14-day operations cycle are known as SPORCs.
| Crater on Zephyria Planum: PSP_005826_1780 PSP_006749_1780 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.76 | 151. | -5.1 | -17.8 | 34.6 | 39.9 |
| Exposure of South Polar Layered Deposits: PSP_004994_1040 PSP_005297_1040 (Interval in Earth days: 24) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -75.7 | 201. | 2.74 | 25.62 | 58.6 | 60.5 |
| Light-Toned Layering on Plains Next to Ganges Chasma: PSP_005161_1720 ESP_016237_1720 (Interval in Earth days: 863) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.14 | 307. | 6.27 | -10.6 | 35.3 | 48.9 |
| Ridges in Nili Fossae Phyllosilicates: PSP_005855_2020 PSP_006712_2020 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.80 | 77.1 | -2.4 | 7.233 | 44.7 | 38.7 |
| Young Double-Layer Ejecta Crater: PSP_006816_2120 PSP_007027_2120 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.47 | 116. | 5.98 | -4.03 | 42.0 | 41.9 |
| Avalanche Features of Dune Slip Face Seen in MOC Image R06-00380: PSP_006899_1330 PSP_006965_1330 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -46.7 | 20.1 | 8.63 | -9.75 | 65.3 | 67.4 |
| 25-Kilometer Diameter Impact Crater of Hellas Basin Floor: PSP_006766_1355 ESP_020387_1355 (Interval in Earth days: 1062) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -44.0 | 51.8 | 1.99 | -12.8 | 61.4 | 64.8 |
| Study Spider Evolution: PSP_005513_0950 PSP_005817_0950 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.0 | 95.0 | 0.87 | -16.4 | 72.9 | 79.4 |
| Small Valley Delta in Crater Near Maja Valles: PSP_005926_1850 ESP_011279_1850 (Interval in Earth days: 417) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.925 | 301. | -8.3 | 17.11 | 36.4 | 55.6 |
| Cover 3 Gullies Previously Identified in Mesa Walls in MOC Image M04-00235: PSP_005673_1305 PSP_005739_1305 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -49.4 | 14.5 | 5.28 | -10.8 | 47.1 | 49.0 |
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