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.
| Possible Future Landing Site in Sabrina Vallis Delta: ESP_026601_1920 ESP_034605_1920 (Interval in Earth days: 623) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.68 | 313. | 3.61 | 21.97 | 46.6 | 43.1 |
| Dunes and North Polar Outlier in MOC Image R03-00181: ESP_026963_2595 ESP_026660_2595 (Interval in Earth days: 24) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.21 | 124. | 13.6 | -1.03 | 56.0 | 56.1 |
| Possible Future Landing Site in Mawrth Vallis: ESP_026600_2060 ESP_034736_2060 (Interval in Earth days: 634) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.53 | 339. | -0.1 | -23.6 | 42.1 | 43.7 |
| Gullies in Crater North of Iani Chaos: ESP_026956_1800 ESP_027523_1800 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.120 | 345. | -21. | -2.25 | 54.9 | 53.7 |
| Cones at Edge of North Polar Layered Deposits: ESP_026694_2605 ESP_026602_2605 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.44 | 268. | 7.91 | -6.06 | 56.4 | 57.1 |
| South Coprates Chasma Dune Changes: ESP_026905_1660 ESP_027182_1660 (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 | -14.0 | 296. | 6.57 | -16.4 | 61.6 | 62.9 |
| Intracrater Dune Changes: ESP_026675_1655 ESP_026609_1655 (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 | -14.5 | 97.7 | -15. | 6.789 | 63.1 | 61.6 |
| Depression East-Southeast of Hale Crater and Neighboring Landforms: ESP_026983_1420 ESP_035264_1420 (Interval in Earth days: 645) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.5 | 329. | 17.6 | -4.01 | 77.4 | 79.1 |
| Unconformities in North Polar Layered Deposits: ESP_026636_2630 ESP_026596_2630 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.75 | 57.8 | -8.5 | 6.574 | 58.8 | 58.0 |
| North Polar Crater Dune Changes: ESP_026888_2550 ESP_026585_2550 (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 | 74.87 | 14.8 | 22.9 | 3.348 | 52.3 | 53.1 |
Page 568 of 885 (8,850 images) | |||||