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.
| Layered Blocks Leaning against Slopes in Deuteronilus Mensae: ESP_027574_2245 ESP_028339_2245 (Interval in Earth days: 59) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.05 | 26.1 | 6.68 | -15.5 | 45.5 | 55.9 |
| Light-Toned Layered Deposits in Ladon Valles: ESP_027471_1600 ESP_027537_1600 (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 | -19.9 | 327. | -8.1 | -26.1 | 65.5 | 66.6 |
| Dune Migration: ESP_027467_2570 ESP_027836_2570 (Interval in Earth days: 29) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 76.96 | 60.3 | -10. | 6.902 | 59.2 | 62.0 |
| Candidate Future Landing Site North of Hellas Planitia: ESP_027481_1540 ESP_025714_1540 (Interval in Earth days: 137) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.8 | 54.6 | 3.40 | -6.59 | 68.7 | 65.5 |
| Complex Superposition of Fractures: ESP_027486_2240 ESP_027631_2240 (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 | 43.43 | 269. | -1.1 | 13.86 | 45.3 | 45.2 |
| North Polar Gypsum Dune Changes: ESP_027488_2615 ESP_027514_2615 (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 | 81.22 | 201. | -7.5 | 7.709 | 61.8 | 61.2 |
| North Polar Gypsum Dune Changes: ESP_027699_2610 ESP_027725_2610 (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 | 80.94 | 202. | -7.6 | 8.192 | 63.8 | 63.1 |
| Deformation of North Polar Layered Deposit Strata: ESP_027537_2640 ESP_027643_2640 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.70 | 283. | 7.94 | -6.02 | 63.1 | 64.8 |
| Central Uplift of an Impact Crater: ESP_027705_1820 ESP_062966_1820 (Interval in Earth days: 2747) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.118 | 56.5 | 2.84 | -7.37 | 52.4 | 54.2 |
| Small Crater on North Polar Layered Deposits: ESP_027548_2635 ESP_027443_2635 (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 | 83.46 | 346. | 6.21 | -8.50 | 63.1 | 62.9 |
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