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.
| Landslide in Southern Mid-Latitude Crater : ESP_043963_1550 ESP_044741_1550 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.4 | 87.4 | -2.0 | 20.53 | 67.4 | 66.1 |
| Candidate Landing Site for 2020 Mission in Gusev Crater : ESP_043907_1650 ESP_043841_1650 (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 | -14.6 | 175. | -8.9 | 12.57 | 60.7 | 59.2 |
| Well-Preserved 5-Kilometer Impact Crater North of Gale Crater : ESP_044106_1800 ESP_053679_1800 (Interval in Earth days: 746) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.147 | 139. | 5.54 | 20.38 | 50.9 | 50.5 |
| Possible Layered Ejecta Deposits from Bakhuysen Crater : ESP_043913_1590 ESP_044190_1590 (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 | -20.8 | 11.6 | 1.25 | -20.0 | 64.4 | 66.3 |
| Mounds with Cracks and Smooth Terrain in Lyot Crater : ESP_044189_2310 ESP_044268_2310 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 50.88 | 28.4 | -5.6 | 17.15 | 42.3 | 40.4 |
| Small Crater in Center of Bakhuysen Crater : ESP_043992_1565 ESP_045047_1565 (Interval in Earth days: 82) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.1 | 15.6 | -3.4 | 6.983 | 66.6 | 64.8 |
| Candidate Landing Site for 2020 Mission in Mclaughlin Crater : ESP_044191_2020 ESP_044336_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 | 21.87 | 337. | -5.9 | 12.55 | 42.1 | 40.8 |
| Pitted Cones in Melas Chasma : ESP_043850_1685 ESP_043916_1685 (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 | -11.4 | 290. | -2.4 | -22.8 | 58.0 | 59.6 |
| Mound in Elysium Planitia with Unusual Apron : ESP_043986_1910 ESP_044263_1910 (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 | 10.94 | 174. | 7.11 | -13.5 | 44.9 | 46.8 |
| Depressions with Layering and Faulting : ESP_044141_1730 ESP_044497_1730 (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 | -6.90 | 267. | -23. | -2.42 | 57.2 | 55.9 |
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