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.
| How Did Valles Marineris Form?: ESP_025415_1675 ESP_026259_1675 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.3 | 294. | 0 | -17.9 | 53.1 | 60.5 |
| A Volcanic Pit Chain and Dust Avalanches : ESP_026249_2025 ESP_026750_2025 (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 | 22.26 | 202. | -7.3 | 17.82 | 42.6 | 41.8 |
| Intersection of Ridges in Pavonis Mons: ESP_025997_1850 ESP_026630_1850 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.788 | 244. | 0 | -19.2 | 47.9 | 51.6 |
| Cut Crater and Fault Scarp along Candor Chasma: ESP_026114_1745 ESP_025547_1745 (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 | -5.51 | 290. | 5.32 | -4.4 | 53.9 | 50.6 |
| Oudemans Crater Layered Central Uplift: ESP_026194_1700 ESP_026339_1700 (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 | -9.86 | 268. | -8.2 | 8.812 | 57.9 | 57.5 |
| Terrain with Layered Material and Circular Pits: ESP_025976_2290 ESP_026464_2290 (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 | 48.73 | 91.1 | 1.38 | -19.8 | 42.0 | 43.7 |
| Fan with Light-Toned Deposits: ESP_025990_1995 ESP_026135_1995 (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 | 19.10 | 76.1 | -27. | -15.8 | 44.5 | 43.8 |
| Source Area for Channel Network Near Gigas Sulci: ESP_025905_1980 ESP_026327_1980 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.74 | 232. | 19.4 | 5.703 | 40.5 | 43.1 |
| Light-Toned Material along Coprates Chasma Wallrock and Plateau: ESP_025929_1645 ESP_026430_1645 (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 | -15.5 | 303. | -6.5 | 17.74 | 60.0 | 61.1 |
| Dark Slope Streak Extending to Channel Floor: ESP_026064_2045 ESP_026697_2045 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.17 | 212. | 0 | -15.4 | 41.0 | 44.0 |
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