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.
| Inlet Valley: ESP_069653_1990 ESP_071011_1990 (Interval in Earth days: 106) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.77 | 78.3 | 9.32 | 24.07 | 49.2 | 48.0 |
| Xanthe Dorsa: ESP_069763_2235 ESP_070053_2235 (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 | 43.13 | 313. | -4.8 | 7.205 | 48.9 | 46.9 |
| Layer Exposure in Candidate Alluvial Fan Deposits: ESP_069936_2020 ESP_070938_2020 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.63 | 272. | -6 | 6.892 | 50.1 | 48.6 |
| Channel and Crater in Rahway Valles: ESP_069755_1910 ESP_070177_1910 (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 | 10.90 | 174. | 13.4 | -18.2 | 51.7 | 54.8 |
| Recent Crater on Northern Plains: ESP_069968_2390 ESP_069889_2390 (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 | 58.81 | 110. | 9.20 | -6.73 | 50.1 | 51.9 |
| Undeveloped Collapse Pit: ESP_069849_1975 ESP_070060_1975 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.41 | 127. | 7.78 | -7.90 | 50.1 | 51.5 |
| Scalloped Depressions in Utopia Planitia: ESP_069692_2290 ESP_069982_2290 (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 | 48.45 | 90.9 | -4.2 | 10.12 | 49.7 | 47.4 |
| Fluvial Feature South of Candidate ExoMars Landing Site in Oxia Planum: ESP_069815_1975 ESP_072017_1975 (Interval in Earth days: 171) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.56 | 335. | 10.7 | -21.7 | 49.9 | 53.3 |
| Mounds in Southern Jezero Crater: ESP_069864_1985 ESP_069930_1985 (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 | 18.13 | 77.5 | 12.6 | -11.4 | 49.5 | 51.5 |
| Layering in Western Arabia Terra: ESP_069933_1900 ESP_070856_1900 (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 | 9.694 | 355. | 4.27 | -17.8 | 53.3 | 55.2 |
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