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.
| South Polar Layered Deposits: ESP_040126_1005 ESP_040073_1005 (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 | -79.5 | 102. | -1.6 | 14.54 | 60.9 | 59.6 |
| Crater with Breached Rim and Interior Terraced Landform: ESP_040182_1405 ESP_058485_1405 (Interval in Earth days: 1426) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.2 | 356. | 6.48 | -5.70 | 36.9 | 38.4 |
| Candidate Landing Site for 2020 Mission in Oyama Crater: ESP_040090_2035 ESP_049294_2035 (Interval in Earth days: 717) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.32 | 340. | 7.12 | -26.4 | 58.7 | 53.3 |
| Southern Mid-Latitude Crater: ESP_039983_1390 ESP_074837_1390 (Interval in Earth days: 2716) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.4 | 30.1 | 4.78 | -9.11 | 38.1 | 43.1 |
| Crater on South Polar Layered Deposits: ESP_040294_1005 ESP_040347_1005 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -79.4 | 194. | -1.5 | -17.4 | 62.1 | 63.7 |
| South Polar Dune Field: ESP_039932_1055 ESP_040064_1055 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -74.2 | 352. | 1.08 | -13.3 | 55.9 | 57.3 |
| Gullies and Lobate Material on Massif in Nereidum Montes: ESP_040131_1405 ESP_049559_1405 (Interval in Earth days: 735) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.1 | 309. | 0.39 | 20.00 | 37.4 | 35.7 |
| Circular Feature in Athabasca Region Flood Lava: ESP_040044_1805 ESP_040466_1805 (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 | 0.287 | 159. | 5.25 | -7.89 | 44.3 | 40.2 |
| Dune Gully Monitoring: ESP_040141_1340 ESP_040629_1340 (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 | -45.8 | 36.6 | 7.92 | -14.9 | 39.3 | 43.0 |
| Northwestern Ladon Valles: ESP_039906_1590 ESP_039972_1590 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.5 | 329. | 6.16 | -18.5 | 37.8 | 39.0 |
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