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.
| Candidate Future Landing Site: ESP_034894_2000 ESP_034960_2000 (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 | 19.89 | 342. | 5.87 | -15.7 | 42.9 | 44.9 |
| 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 |
| Secondary Impacts Near Domoni Crater: ESP_034700_2330 ESP_035333_2330 (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 | 52.54 | 235. | -4.3 | -19.3 | 44.6 | 45.5 |
| InSight Mission Candidate Landing Site: ESP_034783_1850 ESP_034928_1850 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.698 | 136. | -1.1 | 12.06 | 49.0 | 48.8 |
| Sand Dunes on Crater Floor West of Herschel Crater: ESP_034744_1650 ESP_034810_1650 (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 | -14.7 | 122. | 3.67 | -20.3 | 59.8 | 61.8 |
| Layered Deposits in West Candor Chasma: ESP_034804_1740 ESP_035305_1740 (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 | -5.96 | 283. | 0 | 19.77 | 54.9 | 56.0 |
| Trough with Channels in Elysium Fossae: ESP_034519_2100 ESP_035020_2100 (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 | 29.50 | 140. | 4.29 | 15.4 | 40.2 | 40.3 |
| Northern Plains Crater Expansion: ESP_034727_2310 ESP_034806_2310 (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 | 50.44 | 218. | -0.1 | 20.04 | 43.5 | 41.6 |
| Possible Terraced Crater in Arcadia Planitia: ESP_034504_2305 ESP_034636_2305 (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 | 50.19 | 186. | 5.28 | -22.2 | 43.6 | 45.6 |
| Candidate Future Landing Site: ESP_034808_1655 ESP_034874_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 | -14.3 | 175. | 1.98 | -21.3 | 60.1 | 62.0 |
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