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.
| 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 |
| 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 |
| Complex Superposition of Fractures: ESP_027618_2235 ESP_027974_2235 (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 | 43.02 | 268. | -17. | 0.935 | 47.7 | 49.6 |
| 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 |
| 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 |
| Fractured Source Region of Kasei Valles: ESP_027406_2020 ESP_027261_2020 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.79 | 295. | 4.55 | -14.6 | 45.0 | 46.1 |
| 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 |
| Candidate Future Landing Site in Elysium Planitia: ESP_027702_1815 ESP_026792_1815 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.616 | 138. | -0.1 | 20.11 | 52.8 | 50.8 |
| Field of Shallow Depressions: ESP_027581_2185 ESP_028504_2185 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.22 | 197. | -3.7 | 29.11 | 45.6 | 52.4 |
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