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.
| Trough and Ridges along Crater Slope: ESP_036151_2195 ESP_036507_2195 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.27 | 224. | -5.7 | 8.905 | 45.5 | 46.9 |
| Mawrth Vallis Region: ESP_036305_2025 ESP_035804_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 | 22.21 | 341. | 10.3 | -24.9 | 46.4 | 47.6 |
| Well-Preserved Crater with Central Uplift and Layered Ejecta: ESP_036011_1650 ESP_045598_1650 (Interval in Earth days: 747) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.9 | 93.2 | -5.5 | 9.012 | 64.1 | 56.9 |
| Flank of Nia Tholus: ESP_036294_1730 ESP_036571_1730 (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 | -6.77 | 284. | 18.7 | -7.97 | 57.4 | 59.0 |
| Branched and Curving Ridges among Yardangs: ESP_036167_1730 ESP_046031_1730 (Interval in Earth days: 769) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.75 | 152. | 5.51 | -24.7 | 58.4 | 54.6 |
| Pitted Surfaces Near Marte Vallis: ESP_036021_1825 ESP_086897_1825 (Interval in Earth days: 3964) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.569 | 177. | 0 | -14.0 | 53.7 | 47.0 |
| Ridge and Circular Forms in Central Arabia Terra: ESP_036066_2045 ESP_037266_2045 (Interval in Earth days: 94) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.37 | 25.7 | 8.57 | -8.81 | 45.1 | 54.5 |
| Exposure of North Polar Layered Deposits: ESP_036164_2660 ESP_036414_2660 (Interval in Earth days: 19) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 85.70 | 198. | -6.4 | 3.176 | 63.6 | 65.4 |
| Chasma Boreale Gypsum Dune Changes: ESP_036118_2650 ESP_027495_2650 (Interval in Earth days: 672) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.97 | -1.9 | 8.93 | -5.29 | 62.2 | 64.2 |
| Fissure and Channel Southeast of Olympus Mons: ESP_036098_1975 ESP_036375_1975 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.41 | 233. | 6.07 | -11.5 | 47.3 | 49.6 |
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