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.
| Western Portion of Well-Preserved Impact Crater: ESP_032334_1615 ESP_032835_1615 (Interval in Earth days: 40) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.1 | 41.4 | 3.16 | 22.47 | 33.4 | 37.4 |
| Light-Toned Materials Exposed along Ladon Valles Floor: ESP_032218_1625 ESP_040539_1625 (Interval in Earth days: 649) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -17.4 | 328. | 7.83 | -3.22 | 32.1 | 34.1 |
| Dunes: ESP_032354_1165 ESP_023664_1165 (Interval in Earth days: 677) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -63.3 | 228. | -26. | -5.34 | 62.6 | 63.2 |
| Exposure of South Polar Layered Deposits: ESP_032251_0910 ESP_032303_0910 (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 | -88.8 | 189. | 24.6 | 28.32 | 79.2 | 79.7 |
| Intra-Crater Dune Changes in Arabia Terra: ESP_032481_1885 ESP_032771_1885 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.429 | 344. | 2.93 | 29.60 | 35.5 | 32.7 |
| Lava Flow in Syria Planum: ESP_032326_1605 ESP_032827_1605 (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 | -19.1 | 259. | 7.00 | 25.67 | 33.4 | 37.6 |
| Dark V-Shaped Feature Cutting across Layers or Bands on a Slope: ESP_032227_2040 ESP_040271_2040 (Interval in Earth days: 627) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.62 | 78.8 | -8.7 | 3.583 | 46.4 | 56.7 |
| Gullies with Light-Toned Apron Material Near Atlantis Chaos: ESP_032408_1425 ESP_049168_1425 (Interval in Earth days: 1306) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.0 | 183. | -0.8 | 12.53 | 43.0 | 32.7 |
| Region Dubbed Inca City Monitoring: ESP_032352_0985 ESP_032444_0985 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -81.3 | 295. | -6.7 | 8.548 | 76.3 | 77.0 |
| Probable Impact Crater in South Polar Layered Deposits: ESP_032212_0905 ESP_041127_0905 (Interval in Earth days: 695) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -89.3 | 168. | 28.9 | 27.20 | 78.7 | 80.5 |
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