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.
| Well-Preserved 4-Kilometer Impact Crater on Northern Plain: ESP_034133_2405 ESP_035491_2405 (Interval in Earth days: 106) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 60.24 | 233. | 3.18 | 21.12 | 50.3 | 44.9 |
| Possible Offset Terraced Crater in Arcadia Planitia: ESP_034161_2275 ESP_034649_2275 (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 | 46.89 | 192. | -0.4 | -25.9 | 44.1 | 45.1 |
| Possible Hydrated-Silica-Bearing Material in Northwest Hellas Planitia: ESP_034364_1520 ESP_034575_1520 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.8 | 60.5 | -0.9 | -14.1 | 65.8 | 68.6 |
| Possible Terraced Bullseye-Like Crater in Arcadia Planitia: ESP_034108_2245 ESP_034174_2245 (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 | 44.15 | 199. | 4.85 | -9.02 | 42.8 | 43.8 |
| Candidate Future Landing Site in Nili Fossae Carbonate Plains: ESP_034284_2020 ESP_034007_2020 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.94 | 78.6 | -3.8 | 16.99 | 40.9 | 38.1 |
| Kasei Valles Cataract: ESP_034329_2065 ESP_042518_2065 (Interval in Earth days: 638) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.03 | 289. | -2.5 | 16.73 | 40.5 | 38.0 |
| Crater in Marte Vallis: ESP_034346_2025 ESP_034557_2025 (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 | 22.26 | 186. | -8.1 | -20.1 | 41.4 | 43.3 |
| Meander in Central Channel in Nanedi Valles: ESP_034236_1855 ESP_035792_1855 (Interval in Earth days: 121) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.183 | 310. | 3.71 | -19.7 | 44.7 | 53.6 |
| Possible Terraced Crater in Arcadia Planitia: ESP_034332_2265 ESP_035110_2265 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.23 | 203. | 6.63 | -8.13 | 42.6 | 42.9 |
| Infrared-Distinct Crater: ESP_034253_2230 ESP_034899_2230 (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 | 42.83 | 201. | -0.0 | 16.32 | 42.4 | 40.1 |
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