Planned stereo pairs have suitable stereo convergence angles and illumination by design.
In addition to planned stereo pairs, the Pairendipity software can identify overlapping
HiRISE images that are serendipitously suitable for stereo processing and find stereo
pairs within the CTX dataset.
Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below.
Since this list is based on produced stereo anaglyphs it also contains a few serendipitous
pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed
in the “Pairendipity Stereo” link, while CTX stereo pairs are listed
in “Pairendipity CTX Stereo”.
Images taken close together in time minimize illumination and frost differences and are
especially useful (see the Delta-Days column in the Pairendipity files or difference
the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs
with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.
| Impact Crater Exposing Stratigraphy in Eos Chasma: ESP_017463_1630 ESP_018241_1630 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.6 | 315. | 4.08 | -7.28 | 63.1 | 65.0 |
| Fan at Intersection of Valley and Crater Wall in Xanthe Terra: ESP_017555_1875 ESP_018544_1875 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.594 | 321. | 2.99 | -13.2 | 48.9 | 51.8 |
| Sinuous Ridges in Zephyria Planum: ESP_017548_1740 ESP_019104_1740 (Interval in Earth days: 122) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.03 | 153. | 2.13 | -16.8 | 56.6 | 58.1 |
| Unnamed Crater on Rim of Valles Marineris: ESP_017556_1650 ESP_018268_1650 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.7 | 297. | -12. | 0.635 | 63.2 | 63.2 |
| Well-Preserved Impact Crater in Tempe Terra: ESP_017345_2200 ESP_017846_2200 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.72 | 291. | -6.3 | 7.647 | 41.8 | 41.2 |
| Volcanic Rootless Constructs in the Western Tartarus Colles: ESP_017389_2070 ESP_017890_2070 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.51 | 171. | -9.2 | 7.114 | 42.8 | 42.5 |
| Mini-Chaos in Crater Floor: ESP_017459_1990 ESP_053827_1990 (Interval in Earth days: 2834) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.80 | 61.3 | -4.8 | -27.4 | 44.6 | 46.9 |
| Ostrov Crater Fans and Playa: ESP_017357_1530 ESP_026561_1530 (Interval in Earth days: 718) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.5 | 331. | -6.1 | -18.2 | 70.2 | 71.3 |
| Pits on Fan Surfaces in Mojave Crater: ESP_017568_1870 ESP_018069_1870 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.120 | 326. | -6.1 | 13.95 | 49.9 | 49.5 |
| 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 |
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