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.
| Overlapping Lanslide Deposits Within Coprates Chasma: ESP_017688_1685 ESP_018321_1685 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.5 | 292. | 3.48 | -20.3 | 60.5 | 62.6 |
| Central Peak of Unnamed Crater near Kasei Valles: ESP_017635_2085 ESP_018057_2085 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 28.38 | 294. | 4.02 | -10.6 | 41.8 | 44.1 |
| Light-Toned Layering in Noctis Region Pit: ESP_017399_1680 ESP_027236_1680 (Interval in Earth days: 766) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.8 | 263. | -4.9 | -24.5 | 60.2 | 62.0 |
| Laminar Flow in Ejecta Layer North of Tooting Crater: ESP_017625_2040 ESP_018258_2040 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.80 | 207. | 2.38 | -18.9 | 42.9 | 46.3 |
| Candidate MSL Landing Site in Northeast Syrtis Major: ESP_017498_1980 ESP_018566_1980 (Interval in Earth days: 84) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.52 | 76.9 | -8.1 | 12.23 | 45.4 | 46.2 |
| Layered Terrain in Zephyria Planum: ESP_017337_1770 ESP_017759_1770 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.12 | 153. | 6.75 | -12.3 | 53.7 | 56.4 |
| Central Peaks of Two Impact Craters: ESP_017437_1550 ESP_017859_1550 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.9 | 306. | 9.49 | -8.80 | 68.6 | 70.7 |
| Crater Next to Crater with Dark Gully Deposits: ESP_017312_1465 ESP_053825_1465 (Interval in Earth days: 2845) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.3 | 121. | -6.5 | -17.0 | 74.9 | 74.3 |
| Well-Preserved 1-Kilometer Diameter Impact Crater on Northern Plains: ESP_017480_2355 ESP_017968_2355 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 55.21 | 200. | 6.86 | -14.0 | 44.1 | 46.3 |
| Cone with Lobate Flows in Hydraotes Chaos: ESP_017634_1800 ESP_025493_1800 (Interval in Earth days: 612) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.10 | 326. | -12. | -26.9 | 54.3 | 49.1 |
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