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.
| Landslides in Valles Marineris: ESP_089701_1660 ESP_090400_1660 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.7 | 303. | 0.48 | -16.6 | 62.3 | 61.2 |
| Probing Below the Surface with Impact Craters: ESP_089323_2180 ESP_089600_2180 (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 | 37.68 | 175. | 5.18 | -15.4 | 47.3 | 51.5 |
| Planned ExoMars Landing Site in Oxia Planum: ESP_090715_1975 ESP_090781_1975 (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 | 17.07 | 336. | 4.71 | -21.1 | 58.0 | 60.7 |
| Capri Chasma Interior with Possible Sulfate-Rich Terrain: ESP_090782_1670 ESP_091494_1670 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.8 | 310. | -2.7 | -27.8 | 58.4 | 56.6 |
| Crater Floor Outcrop: ESP_090762_1905 ESP_091487_1905 (Interval in Earth days: 57) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.57 | 134. | -5.1 | 25.16 | 58.2 | 58.3 |
| Fluvial Valley in Arabia Terra: ESP_090820_2085 ESP_090754_2085 (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 | 28.33 | 349. | -19. | 3.726 | 63.7 | 61.0 |
| Survey of Terrain around Ice-Exposing Crater: ESP_090417_2195 ESP_090628_2195 (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 | 39.25 | 190. | 8.58 | -5.83 | 59.5 | 63.6 |
| Morphologically Fresh Incision in Potentially Ice-Rich Mantling Deposit: ESP_090370_2225 ESP_090436_2225 (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 | 41.91 | 34.0 | -3.7 | -16.2 | 60.6 | 62.6 |
| Vent East of Ascraeus Mons: ESP_090375_1925 ESP_090520_1925 (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 | 12.13 | 261. | -5.8 | 10.07 | 56.2 | 55.7 |
| Alluvial Fan in Coprates Catena Trough: ESP_090308_1650 ESP_090453_1650 (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 | -14.6 | 294. | -16. | 8.504 | 61.8 | 59.4 |
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