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.
| Western Half of Well-Preserved 9 Kilometer Diameter Crater: ESP_012871_1565 ESP_013016_1565 (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 | -23.1 | 43.0 | -4.2 | 13.08 | 45.4 | 42.2 |
| Seasonal Monitoring Candidate: ESP_013787_0955 ESP_014037_0955 (Interval in Earth days: 20) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -84.4 | 274. | -7.7 | 8.965 | 66.4 | 67.8 |
| Multi-Aprons of Ganges Region Landslide: ESP_013217_1715 ESP_013718_1715 (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 | -8.33 | 315. | -5.3 | 17.64 | 45.4 | 37.8 |
| Mounds in Tractus Fossae: ESP_012797_2075 ESP_012942_2075 (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 | 27.32 | 256. | -0.3 | 14.02 | 68.7 | 67.3 |
| South Polar Layered Deposits Exposed in Ultimum Chasma: ESP_013778_0985 ESP_013659_0985 (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 | -81.2 | 147. | -12. | 4.816 | 63.8 | 61.6 |
| Light-Toned Layered Material in Trough on North Melas Chasma Wall: ESP_013495_1720 ESP_014128_1720 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.82 | 284. | 6.24 | -18.3 | 41.5 | 36.9 |
| Recent Gullies in a Crater in Noachis Terra: ESP_013222_1410 ESP_013288_1410 (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 | -38.8 | 182. | 0.69 | -18.8 | 40.4 | 41.3 |
| Rootless Cones in Isidis Planitia: ESP_013212_1890 ESP_020082_1890 (Interval in Earth days: 536) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.729 | 88.8 | 2.89 | 20.63 | 53.9 | 52.9 |
| Gullied Crater Wall: ESP_013207_1365 ESP_031180_1365 (Interval in Earth days: 1401) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -43.0 | 232. | 3.74 | -6.73 | 41.3 | 38.2 |
| Landforms in Southern Tartarus Colles: ESP_012642_1895 ESP_013710_1895 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.266 | 170. | 0.88 | 24.43 | 58.7 | 46.9 |
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