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.
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_084894_1050 ESP_084762_1050 (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 | -75.0 | 156. | -0.7 | 14.00 | 65.3 | 62.6 |
| Gullies on Lobate Flow Feature Basin in Nereidum Montes: ESP_084532_1335 ESP_084967_1335 (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 | -46.1 | 311. | 13.9 | 23.63 | 40.7 | 44.2 |
| Terraced Impact Crater on Lobate Debris Apron: ESP_084759_1385 ESP_084825_1385 (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 | -40.9 | 232. | 2.14 | -19.6 | 40.6 | 42.6 |
| Well-Preserved 2 to 3-Kilometer Superposed Impact Crater: ESP_084530_1520 ESP_084741_1520 (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 | -27.6 | 4.19 | 6.05 | -21.1 | 34.9 | 37.3 |
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_084674_0970 ESP_084648_0970 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.8 | 55.2 | 1.85 | -13.0 | 68.4 | 69.1 |
| Hill on South Polar Layered Deposits: ESP_084887_0900 ESP_084374_0900 (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 | -89.7 | 35.5 | 29.4 | 29.44 | 75.3 | 68.6 |
| Gullies with Long Channels in Sisyphi Cavi: ESP_084781_1095 ESP_091756_1095 (Interval in Earth days: 543) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -70.4 | -1.1 | 1.26 | 29.95 | 60.1 | 60.2 |
| Southern Canyon Wall in East Coprates Chasma: ESP_084888_1645 ESP_076950_1645 (Interval in Earth days: 618) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.4 | 305. | 13.0 | -5.95 | 33.5 | 41.3 |
| Meandering Channels in Newton Crater: ESP_084246_1400 ESP_084457_1400 (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 | -39.6 | 200. | 7.37 | -7.18 | 37.9 | 39.0 |
| Olivine and Hydrated Mineral-Rich Terrain in Nili Fossae: ESP_084158_2025 ESP_084382_2025 (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 | 22.23 | 76.9 | -8.9 | 24.45 | 59.7 | 55.0 |
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