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.
| Northern Plains Crater Modification : ESP_043549_2265 ESP_043615_2265 (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 | 45.99 | 220. | -5.7 | -18.9 | 41.7 | 42.7 |
| Well-Preserved Impact Crater in Meridiani Planum : ESP_043557_1770 ESP_044335_1770 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.99 | 8.83 | -7.2 | 7.52 | 51.8 | 52.9 |
| Mamers Valles Source : ESP_043794_2210 ESP_044084_2210 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.59 | 12.4 | 0.68 | 25.94 | 39.7 | 37.3 |
| Bakhuysen Crater Ejecta with Mounds and Unit Contacts: ESP_043636_1565 ESP_044203_1565 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.2 | 13.9 | 0.33 | 15.53 | 65.0 | 66.0 |
| Fractured Ground in Northeast Syrtis Major Region : ESP_043739_1975 ESP_043884_1975 (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 | 17.47 | 77.0 | 0.78 | 18.10 | 42.2 | 41.1 |
| Dunes and Slopes in Crater Southwest of Xainza Crater : ESP_043597_1800 ESP_043742_1800 (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 | -0.18 | 355. | 3.97 | 21.58 | 49.6 | 49.0 |
| Fresh Crater on Northern Plains : ESP_043601_2310 ESP_044313_2310 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 50.71 | 238. | 5.53 | 24.49 | 42.0 | 39.6 |
| Mamers Valles Source : ESP_043583_2210 ESP_043649_2210 (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 | 40.56 | 12.3 | 4.01 | -11.3 | 39.7 | 40.9 |
| Flows on Fracture in Adamas Labyrinthus : ESP_043672_2170 ESP_044371_2170 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.77 | 103. | -0.0 | -18.1 | 39.5 | 41.4 |
| Central Candor Chasma : ESP_043705_1720 ESP_053766_1720 (Interval in Earth days: 783) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.76 | 287. | 4.77 | -7.87 | 54.6 | 57.0 |
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