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.
| Downslope Movement on Escarpment: ESP_066051_2085 ESP_065919_2085 (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 | 28.10 | 74.3 | 7.45 | 28.37 | 68.4 | 67.8 |
| Central Structure in Impact Crater: ESP_065737_1930 ESP_073664_1930 (Interval in Earth days: 618) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 12.71 | 6.68 | -3.5 | 6.845 | 61.3 | 60.4 |
| Gullies in Crater in Nereidum Montes: ESP_066095_1350 ESP_066504_1350 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -44.8 | 324. | -3.4 | -24.2 | 44.1 | 43.7 |
| Bisected Polygonal Bedrock: ESP_065918_1935 ESP_083234_1935 (Interval in Earth days: 1349) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 13.13 | 106. | -3.5 | 4.659 | 60.4 | 61.0 |
| Leveed Candidate Mudflow: ESP_065910_1995 ESP_066042_1995 (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 | 19.36 | 323. | 1.75 | -22.4 | 63.9 | 64.6 |
| Ares Vallis: ESP_065791_1920 ESP_066200_1920 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.67 | 333. | -3.6 | -25.0 | 60.4 | 58.6 |
| West Rim of Impact Crater in Coprates Chasma: ESP_065832_1675 ESP_065344_1675 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.3 | 294. | 21.2 | 11.53 | 47.2 | 52.3 |
| Channel in Southern Highlands Crater: ESP_066064_1530 ESP_074281_1530 (Interval in Earth days: 640) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.6 | 87.9 | -7.6 | 2.974 | 43.6 | 48.8 |
| Valles Marineris: ESP_066004_1745 ESP_065938_1745 (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 | -5.45 | 282. | -8.2 | 6.452 | 50.2 | 49.9 |
| Lava-Filled Crater near Athabasca Valles: ESP_065481_1875 ESP_065969_1875 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.224 | 154. | -0.2 | 16.82 | 59.3 | 55.2 |
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