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.
| Possible Breached Crater near Jezero Crater: ESP_070352_1990 ESP_069574_1990 (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 | 18.71 | 75.6 | -20. | -5.69 | 52.1 | 50.0 |
| Alluvial Fans in Ganges Chasma: ESP_070185_1715 ESP_071899_1715 (Interval in Earth days: 133) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.34 | 317. | -6.0 | 19.25 | 63.5 | 58.8 |
| Collapse Pit in Graben with Ice Fill: ESP_070055_2235 ESP_070134_2235 (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 | 43.40 | 260. | -6.3 | 17.25 | 48.0 | 45.7 |
| Active Gully Monitoring and Characterization: ESP_070369_2300 ESP_070791_2300 (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 | 49.54 | 325. | 1.24 | -14.7 | 47.2 | 48.2 |
| Fractures East of Olympus Mons: ESP_070122_1975 ESP_069621_1975 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.23 | 233. | 10.6 | -5.07 | 50.1 | 50.6 |
| Idaeus Fossae: ESP_070251_2195 ESP_071609_2195 (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 | 38.97 | 308. | 3.65 | 21.74 | 46.6 | 46.0 |
| Phlegra Montes: ESP_070375_2160 ESP_070441_2160 (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 | 35.54 | 164. | -6.1 | -23.9 | 47.4 | 49.0 |
| Collapse Pit in Graben with Ice Fill: ESP_070042_2190 ESP_070332_2190 (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 | 38.59 | 256. | -8.8 | 6.011 | 48.0 | 46.2 |
| Layering in Arabia Terra: ESP_070012_1825 ESP_070078_1825 (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 | 2.477 | 358. | 9.85 | -16.0 | 56.2 | 58.3 |
| Peanut-Shaped Crater with Glacial Fill: ESP_070350_2135 ESP_070917_2135 (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 | 33.05 | 126. | -2.4 | -14.5 | 47.3 | 48.0 |
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