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.
| Rayed Crater: ESP_026937_2145 ESP_027847_2145 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.12 | 137. | -0.8 | -12.9 | 41.9 | 48.3 |
| 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 |
| Exposures of North Polar Layered Deposits with Unconformities: ESP_026901_2600 ESP_028048_2600 (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 | 80.00 | 23.3 | 0 | 15.02 | 57.0 | 66.2 |
| 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 |
| Well-Preserved Crater with Layered Ejecta on Northern Plains: ESP_026910_2170 ESP_027477_2170 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.52 | 155. | -8.4 | 6.108 | 42.4 | 43.9 |
| 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 |
| 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 |
| Cones at Edge of North Polar Layered Deposits: ESP_026958_2605 ESP_027077_2605 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.62 | 262. | 5.88 | -8.25 | 57.3 | 58.6 |
| Pits and Channels in Amazonis Planitia: ESP_026605_2025 ESP_051290_2025 (Interval in Earth days: 1924) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.23 | 202. | 3.69 | 14.57 | 42.6 | 35.3 |
| Possible Phyllosilicates and Fluvial Features Near Hashir Crater: ESP_026649_1835 ESP_028060_1835 (Interval in Earth days: 109) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.323 | 84.8 | -9.5 | 13.24 | 51.7 | 51.4 |
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