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.
| High-Latitude Exposure of North Polar Layered Deposits : ESP_045251_2720 ESP_045223_2720 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.16 | 87.4 | -8.4 | -18.6 | 69.0 | 70.1 |
| Rifts and Pitted Cones in Utopia Planitia : ESP_045057_2120 ESP_052006_2120 (Interval in Earth days: 541) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.65 | 96.3 | 0.79 | -8.62 | 41.6 | 38.8 |
| North Polar Gypsum Dunes : ESP_045263_2605 ESP_045500_2605 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.40 | 213. | 4.05 | 18.68 | 61.7 | 63.6 |
| Rift in Utopia Planitia : ESP_045334_2125 ESP_052863_2125 (Interval in Earth days: 587) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.20 | 95.2 | 0.58 | 12.28 | 43.0 | 38.2 |
| Young Surface East of Olympus Mons : ESP_045395_1980 ESP_045817_1980 (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 | 17.82 | 232. | -1.7 | -21.5 | 44.6 | 48.5 |
| Scarp Transition into Ganges Chasma Floor : ESP_045326_1715 ESP_046315_1715 (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 | -8.44 | 318. | 8.37 | -12.8 | 54.3 | 53.7 |
| Mesas and Ridges in Utopia Planitia : ESP_045176_2130 ESP_045242_2130 (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 | 32.71 | 87.3 | 6.66 | -8.05 | 41.7 | 43.3 |
| Pits on Kasei Valles Lava : ESP_045063_2070 ESP_045775_2070 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.95 | 293. | 2.76 | 27.90 | 41.8 | 43.7 |
| Mawrth Vallis : ESP_045048_2025 ESP_045971_2025 (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 | 22.18 | 343. | -2.7 | 16.97 | 43.0 | 46.3 |
| Well-Preserved Impact Crater : ESP_045111_1975 ESP_063915_1975 (Interval in Earth days: 1465) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.32 | 64.1 | 1.91 | -11.6 | 43.8 | 56.1 |
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