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.
| Tributary of Mamers Valles: ESP_034695_2175 ESP_034972_2175 (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 | 37.10 | 15.0 | -5.1 | -28.5 | 41.4 | 43.9 |
| Lava-Ejecta Interaction in Cerberus Region: ESP_034664_1865 ESP_034954_1865 (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 | 6.328 | 144. | 7.04 | 29.64 | 46.9 | 46.6 |
| Fan-Shaped Landform at Valley Terminus in Lyot Crater: ESP_034813_2315 ESP_061912_2315 (Interval in Earth days: 2111) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 50.94 | 31.0 | -5.0 | -24.6 | 43.9 | 45.0 |
| Gullies: ESP_034618_2280 ESP_036530_2280 (Interval in Earth days: 149) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 47.62 | 315. | 0.53 | 9.725 | 42.9 | 48.5 |
| Crater with Light and Dark Layers Exposed in Walls: ESP_034733_1675 ESP_035023_1675 (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 | -12.4 | 63.9 | -7.9 | 19.17 | 59.0 | 59.1 |
| Domoni Crater Secondary Craters: ESP_034766_2310 ESP_035201_2310 (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 | 50.40 | 232. | 5.29 | 27.17 | 42.9 | 40.6 |
| Crater with Yardangs and Interior Mound in Arabia Terra: ESP_034629_1885 ESP_035130_1885 (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 | 8.434 | 20.8 | -7.1 | 9.011 | 46.9 | 48.1 |
| Active Dune Monitoring in Ganges Chasma: ESP_034671_1725 ESP_035172_1725 (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 | -7.55 | 314. | 7.97 | 23.88 | 54.5 | 56.2 |
| Depression with Concentric Features: ESP_034772_1515 ESP_052297_1515 (Interval in Earth days: 1366) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.4 | 80.7 | -1.9 | -25.0 | 69.8 | 68.6 |
| Transverse Aeolian Ridges in Aram Chaos: ESP_034881_1825 ESP_036437_1825 (Interval in Earth days: 121) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.510 | 340. | 0.54 | 14.10 | 50.6 | 53.1 |
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