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.
| Flow in Tharsis Region: ESP_088055_2035 ESP_088345_2035 (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 | 23.45 | 241. | -21. | -5.64 | 46.3 | 45.7 |
| Ridges in Nilosyrtis Mensae: ESP_088312_2135 ESP_088246_2135 (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 | 33.36 | 60.4 | 2.84 | 21.93 | 43.1 | 41.2 |
| Dark Material in Coprates Chasma: ESP_087697_1660 ESP_088198_1660 (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 | -13.7 | 298. | 0.73 | 12.47 | 61.2 | 62.7 |
| Light-Toned Fractured Material West of Nectaris Montes: ESP_087710_1655 ESP_087644_1655 (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 | -14.4 | 303. | 1.75 | 21.48 | 61.6 | 59.9 |
| North-Pole-Facing Deposit in Crater Associated with Headwall Erosion: ESP_087725_2165 ESP_087659_2165 (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 | 36.39 | 248. | -8.9 | 6.861 | 43.1 | 41.7 |
| Crater with Steep Slopes: ESP_087605_2480 ESP_088040_2480 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 67.87 | 277. | -2.1 | 12.63 | 52.1 | 49.6 |
| 4-Kilometer Diameter Rayed Crater: ESP_087802_1915 ESP_088448_1915 (Interval in Earth days: 51) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.13 | 309. | 0.34 | 12.37 | 48.0 | 49.1 |
| North-Pole-Facing Deposit in Crater: ESP_087778_2285 ESP_088068_2285 (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 | 48.34 | 240. | -10. | 2.734 | 44.8 | 43.5 |
| Isolated Dune Field in Crater Northwest of Syrtis Major Planum: ESP_087903_2050 ESP_089050_2050 (Interval in Earth days: 90) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.85 | 71.6 | -17. | 0.922 | 45.3 | 47.0 |
| Inverted Drainage Network Deep in Central Valles Marineris: ESP_087816_1705 ESP_088027_1705 (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 | -9.41 | 289. | 6.89 | -9.49 | 58.7 | 60.7 |
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