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.
| Bench in Mangala Valles: ESP_088109_1710 ESP_088676_1710 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.95 | 208. | 5.01 | -16.7 | 59.8 | 62.3 |
| Dune Field: ESP_088035_2385 ESP_088378_2385 (Interval in Earth days: 26) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 57.96 | 58.8 | 6.11 | -24.3 | 45.9 | 48.8 |
| Dune Monitoring in Northern Mid-Latitude Crater: ESP_088171_2295 ESP_088395_2295 (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 | 49.11 | 309. | -5.5 | 19.83 | 44.5 | 42.6 |
| Candidate ExoMars Landing Site in Oxia Planum: ESP_088078_2000 ESP_088012_2000 (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 | 19.56 | 334. | -28. | -7.03 | 48.3 | 46.2 |
| Obstacle within Lobate Debris Apron: ESP_088359_1435 ESP_088570_1435 (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 | -36.0 | 225. | 7.68 | -5.73 | 78.9 | 79.8 |
| Dunes in Crater in Northern Plains: ESP_088303_2400 ESP_088224_2400 (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 | 59.87 | 302. | -4.4 | -19.2 | 47.6 | 48.8 |
| Gullies on North Wall of Nier Crater: ESP_088073_2235 ESP_088007_2235 (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 | 43.08 | 106. | -6.6 | 11.04 | 43.6 | 42.0 |
| Kasei Valles Scarps and Terraces: ESP_088145_2055 ESP_088567_2055 (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 | 25.39 | 302. | -3.6 | -28.6 | 44.6 | 48.0 |
| Group of Channels along Old Crater Wall: ESP_088288_2130 ESP_088499_2130 (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 | 32.59 | 357. | -6.7 | -18.5 | 44.0 | 45.7 |
| Potential Landing Site in Capri Chasma: ESP_088158_1665 ESP_088224_1665 (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 | -13.4 | 311. | 6.00 | -19.7 | 62.8 | 64.6 |
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