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 Terraced Crater in Arcadia Planitia: ESP_033053_2245 ESP_033330_2245 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.95 | 202. | 5.36 | -17.6 | 50.1 | 49.1 |
| Possible Future Landing Site in Nili Fossae: ESP_033084_2020 ESP_033295_2020 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.58 | 78.5 | 13.0 | 2.611 | 37.5 | 38.0 |
| Possible Terraced Bullseye-Like Crater in Arcadia Planitia: ESP_033172_2265 ESP_033594_2265 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.20 | 193. | -2.1 | -13.6 | 50.8 | 48.0 |
| Polygons in Lyot Crater Ejecta: ESP_032980_2345 ESP_033059_2345 (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 | 54.13 | 33.2 | 6.25 | 23.47 | 58.0 | 56.0 |
| Deep Crevasses in Glacier-Like Form: ESP_032978_1390 ESP_033400_1390 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.8 | 102. | -5.3 | -23.2 | 55.1 | 63.2 |
| Light-Toned Layered Deposits Exposed along Coprates Chasma Floor: ESP_032931_1645 ESP_040975_1645 (Interval in Earth days: 627) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.4 | 302. | -8.6 | 15.73 | 39.8 | 32.4 |
| Small Pedestal Crater on Ejecta of Larger Craters: ESP_032961_1385 ESP_033251_1385 (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 | -40.9 | 206. | -1.0 | 18.10 | 54.6 | 58.4 |
| Tilted Layers in Center of Oudemans Crater: ESP_033275_1700 ESP_033697_1700 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.92 | 268. | 8.73 | -8.81 | 40.6 | 47.1 |
| Recent Crater in Isidis Planitia: ESP_033281_2020 ESP_033703_2020 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.60 | 100. | 6.50 | -8.36 | 37.7 | 39.4 |
| Crater on the Northern Plains: ESP_032904_2300 ESP_033181_2300 (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 | 49.41 | 309. | 4.58 | -17.5 | 55.6 | 53.8 |
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