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.
| Fresh Impact Near Airy Crater : ESP_053671_1745 ESP_060423_1745 (Interval in Earth days: 526) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.40 | 0.40 | 5.21 | 15.40 | 54.8 | 44.8 |
| Possible Fan-Like Form in Crater in North Arabia Terra : ESP_053829_2115 ESP_054119_2115 (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 | 31.21 | 2.40 | 0.91 | 24.13 | 42.4 | 42.0 |
| Sample Terrain between Candidate Landing Sites for 2020 Mission : ESP_053734_1985 ESP_055145_1985 (Interval in Earth days: 110) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.27 | 77.3 | 5.83 | -7.23 | 43.9 | 52.3 |
| Pitted Cones in Chryse Planitia : ESP_053659_2115 ESP_054081_2115 (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 | 31.09 | 323. | 4.27 | -8.77 | 41.3 | 44.7 |
| Triple Exit Breach in Fresh Crater : ESP_053736_2180 ESP_053670_2180 (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 | 37.57 | 21.4 | -6.7 | 10.46 | 42.6 | 40.8 |
| Light-Toned Deposits along Ius Chasma Floor : ESP_053819_1715 ESP_053753_1715 (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 | -8.59 | 280. | -1.3 | 21.45 | 57.0 | 55.5 |
| Exposure of North Polar Layered Deposits : ESP_053615_2670 ESP_053339_2670 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 86.98 | 64.0 | -17. | -28.9 | 63.7 | 63.4 |
| North Polar Residual Cap Topography : ESP_053780_2715 ESP_053491_2715 (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 | 88.33 | 75.7 | -26. | -19.2 | 68.5 | 66.1 |
| Scarps in North Polar Layered Deposits : ESP_053717_2645 ESP_053835_2645 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.60 | 157. | -8.0 | 7.552 | 62.2 | 62.5 |
| Dunes with Fans : ESP_053847_2605 ESP_053939_2605 (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 | 80.21 | 217. | -7.0 | 6.999 | 60.2 | 60.2 |
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