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.
| Pitted Mounds in Aurorae Chaos : ESP_058196_1700 ESP_057774_1700 (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 | -10.0 | 323. | 2.01 | -6.81 | 31.1 | 35.5 |
| Crescentic Feature on South Polar Layered Deposits : ESP_057951_0925 ESP_057831_0925 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.6 | 240. | 7.09 | 20.50 | 68.9 | 66.4 |
| Dissected Fan or Delta in Terby Crater : ESP_058192_1510 ESP_059405_1510 (Interval in Earth days: 95) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.6 | 75.2 | -4.3 | 8.821 | 31.6 | 44.4 |
| Gullies Monitoring : ESP_058049_1275 ESP_058115_1275 (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 | -52.1 | 23.0 | 3.26 | -14.7 | 41.7 | 43.4 |
| Terrain in Utopia Planitia : ESP_057980_2110 ESP_058626_2110 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.80 | 96.3 | -8.1 | 5.121 | 59.7 | 50.2 |
| Well-Preserved Simple High-Latitude Crater : ESP_058001_1095 ESP_058581_1095 (Interval in Earth days: 46) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -70.3 | 257. | 7.53 | 20.94 | 54.5 | 61.5 |
| Candidate Landing Site for 2020 Mission Near Jezero Crater : ESP_058139_1985 ESP_058429_1985 (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 | 18.17 | 76.9 | -8.4 | 6.967 | 47.9 | 43.3 |
| Rayed Crater : ESP_058182_1720 ESP_076012_1720 (Interval in Earth days: 1389) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.07 | 345. | 0 | 18.19 | 32.0 | 34.1 |
| Gale Crater Rim : ESP_058216_1750 ESP_049051_1770 (Interval in Earth days: 714) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.81 | 136. | -4.2 | -21.2 | 33.2 | 37.9 |
| Crater Wall in Nepenthes Mensae West of Elysium Planitia : ESP_058111_1895 ESP_076152_1895 (Interval in Earth days: 1406) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.214 | 122. | -3.9 | 6.274 | 41.8 | 40.6 |
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